2024·12·07 Joe Biden Didn’t Win (And Neither Did Kamala Harris) Daily Thread

44 days, 11 hours, 59 minutes until the Once And Future President, Donald John Trump, is restored to the office that was Rightfully his the last four years.

Not that I’m counting, mind you.

What is it that feeds our battle, yet starves our victory?

January 6 Tapes?

Where are the tapes? Anyone, Anyone? Bueller? Johnson??

Paging Speaker Johnson…this is your conscience calling you out on broken promises.

Day of Infamy

One thing that many are counting is the 83rd anniversary of the Japanese sneak attack on Pearl Harbor.

When I was a kid it seemed like every account of World War II didn’t just call it an “attack” but rather a “sneak attack.”

It seems that we were as outraged by the “sneak” as we were by the “attack.” What made it a sneak attack was that it happened with no declaration of war by Japan. Here we are at peace with each other and WHAM!! our Pacific fleet is burning or already at the bottom of the harbor. (We can argue whether Roosevelt knew it was going to happen and let it happen, or whether we just got caught napping…either way the effect on the public was the same. I do think Roosevelt was on some level happy that we were in the war; he had up to that time wanted to help the allies a lot more than the American people did.)

If the telling in Tora! Tora! Tora! is to be believed (and I tend to believe it), the Japanese didn’t intend it to be a sneak attack. They intended to pass their declaration of war on to our government and then attack almost immediately, but slow decoding of the dispatch prevented that from happening; the attack happened before the message was delivered.

Whether that would have made a difference in the level of resolve we felt, is another question entirely. And so we have a straight line from this–the photograph taken from one of the Japanese aircraft just after the start of the attack, educating us on the folly of bottling up our fleet and parking our aircraft too close together:

To these two photographs, taken from two different aircraft, the Enola Gay and the Bockscar after they did a couple of “physics package” demos to complete Japan’s education in the folly of their foreign policy:

We had learned the lesson Japan had taught us on this day in 1941.

We are excellent teachers as well as studentsl we reinforced our lesson for the Japanese by repeating it. But we did a slightly different demo the second time–plutonium instead of U-235–in order not to be too repetitive.

The lesson stuck. Japan hasn’t been a problem on that scale, since.

And now, on to the Deep State, which needs a salutary lesson of its own.

News Flash

Today, it is still the case that Joe Biden didn’t Win.

I realize that to some readers, this might be a shock; surely at some point things must change and Biden will have actually won.

But the past cannot actually be changed.

It will always and forever be the case that Joe Biden didn’t win.

And if you, Leftist Lurker, want to dismiss it as dead white cis-male logic…well, you can call it what you want, but then please just go fuck off. No one here buys that bullshit–logic is logic and facts are facts regardless of skin color–and if you gave it a moment’s rational thought, you wouldn’t either. Of course your worthless education never included being able to actually reason–or detect problems with false reasoning–so I don’t imagine you’ll actually wake up as opposed to being woke.

As Ayn Rand would sometimes point out: Yes, you are free to evade reality. What you cannot do is evade the consequences of evading reality. Or to put it concretely: You can ignore the Mack truck bearing down on you as you play in the middle of the street, you won’t be able to ignore the consequences of ignoring the Mack truck.

And Ayn Rand also pointed out that existence (i.e., the sum total of everything that exists) precedes consciousness–our consciousnesses are a part of existence, not outside of it–therefore reality cannot be a “social construct” as so many of you fucked-up-in-the-head people seem to think.

So much for Leftist douchebag lurkers. For the rest of you, the regular readers and those lurkers who understand such things: I continue to carry the banner once also carried by Wheatie. His Fraudulency didn’t win.

Let’s Go, Brandon!!

His Fraudulency

Joe Biteme, properly styled His Fraudulency, continues to infest the White House, we haven’t heard much from the person who should have been declared the victor, and hopium is still being dispensed even as our military appears to have joined the political establishment in knuckling under to the fraud.

One can hope that all is not as it seems.

I’d love to feast on that crow.

(I’d like to add, I find it entirely plausible, even likely, that His Fraudulency is also His Figureheadedness. (Apparently that wasn’t a word; it got a red underline. Well it is now.) Where I differ with the hopium addicts is on the subject of who is really in charge. It ain’t anyone we like.)

Justice Must Be Done.

The prior election must be acknowledged as fraudulent, and steps must be taken to prosecute the fraudsters and restore integrity to the system.

Nothing else matters at this point. Talking about trying again in 2024 is hopeless otherwise. Which is not to say one must never talk about this, but rather that one must account for this in ones planning; if fixing the fraud is not part of the plan, you have no plan.

Lawyer Appeasement Section

OK now for the fine print.

This is the WQTH Daily Thread. You know the drill. There’s no Poltical correctness, but civility is a requirement. There are Important Guidelines,  here, with an addendum on 20191110.

We have a new board – called The U Tree – where people can take each other to the woodshed without fear of censorship or moderation.

And remember Wheatie’s Rules:

1. No food fights
2. No running with scissors.
3. If you bring snacks, bring enough for everyone.
4. Zeroth rule of gun safety: Don’t let the government get your guns.
5. Rule one of gun safety: The gun is always loaded.
5a. If you actually want the gun to be loaded, like because you’re checking out a bump in the night, then it’s empty.
6. Rule two of gun safety: Never point the gun at anything you’re not willing to destroy.
7. Rule three: Keep your finger off the trigger until ready to fire.
8. Rule the fourth: Be sure of your target and what is behind it.

(Hmm a few extras seem to have crept in.)

Spot Prices.

Kitco Ask. Last week:

Gold $2,650.10
Silver $30.69
Platinum $954.00
Palladium $1002.00
Rhodium $4,850.00
FRNSI* 127.199-
Gold:Silver 86.351-

This week, markets closed as of 3PM MT.

Gold $2,634.20
Silver $31.11
Platinum $936.00
Palladium $982.00
Rhodium $4,850.00
FRNSI* 126.429+
Gold:Silver 84.674-

Gold down and silver up. This is good news for silver, which has been rising relative to gold, finally recovering somewhat from the disproportionate beating it took since the election.

*The SteveInCO Federal Reserve Note Suckage Index (FRNSI) is a measure of how much the dollar has inflated. It’s the ratio of the current price of gold, to the number of dollars an ounce of fine gold made up when the dollar was defined as 25.8 grains of 0.900 gold. That worked out to an ounce being $20.67+71/387 of a cent. (Note gold wasn’t worth this much back then, thus much gold was $20.67 71/387ths. It’s a subtle distinction. One ounce of gold wasn’t worth $20.67 back then, it was $20.67.) Once this ratio is computed, 1 is subtracted from it so that the number is zero when the dollar is at its proper value, indicating zero suckage.

The Final Experiment

…starts in one week.

Eric Dubay of the two hundred proofs contradicting himself, at one turn insisting he’d love to go to Antarctica to see for himself, and when offered the opportunity, refusing to concede that he had ever said so.

Disgraceful behavior from the Flerfers. Predicted by the globers. Will Duffy initially didn’t believe they’d turn on their own like this (as the globers said they would), but finally just had to come out and call them on it.

In related news, one of the globers had to back out for medical reasons. The Final Experiment is actually getting a special campsite at almost 80 degrees South–one where no terrain will occlude the Sun– and now they were below the threshold (nine) that the company doing the logistics actually needed for the special camp. So Duffy had to find someone to take the open slot.

And who stepped up? A full-blown, Hollywood-grade documentary producer named Jonathan Mariande. He will make a documentary of the trip.

AND MARIANDE IS A FLAT EARTHER.

This will make it even harder for the Flerfers to tap dance around what happens.

It must be great to be a charlatan and make money off of suckers…until the truth outs. Then suddenly you see your life turning to garbage. Sorry, no sympathy from me.

It Came From Deep Space

If there’s one thing almost all of the moons of the outer solar system…and all of the TNOs…share in common it’s that they’re largely made out of water ice.

Honestly if anyone tries to sell you on the idea that space aliens are going to come here to steal our water, just laugh in their faces.

They don’t even have to come almost all the way to Earth just to filch water from our TNOs, they certainly have similar things in their own systems. Water is the most common heteronuclear molecule (i.e. composed of more than one kind of atom) in space.

Which makes sense. Half of all of the “stuff” in the universe that is not hydrogen and is not helium, is oxygen. And after being blasted out into space in a planetary nebula or supernova, the first thing an oxygen atom is likely to find (once thing settle down enough to let it hang onto eight electrons) is a hydrogen atom, or even a hydrogen molecule, because there are seventy grams of hydrogen for every gram of oxygen…which means 1100 hydrogen atoms for every oxygen atom. There’s plenty of helium around too but that’s fluff from a chemical standpoint. So the first thing that lone oxygen atom is going to find isn’t another oxygen atom to form O2, but hydrogen, to form OH then another to form H2O. Badda-bing! Water.

This notion of most solid things being made largely out of water ice is foreign to us, because Earth is almost purely rocks (which, OBTW, generally contain plenty of oxygen) and (deep, deep down) iron-nickel. If Earth actually had its share of water, it’d be Water World, with no rocks within hundreds of miles of the surface. It would look like Europa would look, if Europa melted. (Europa probably has more water in that subsurface ocean than Earth has in total, in spite of being much smaller than Earth.)

Where did our water go? It got blown away by heat. When the Earth first formed it was a molten mass; the water certainly vaporized, and at those temperatures Earth’s gravity would not hold it. Then the stream of energy and particles from the Sun would simply have whisked it away. (In fact we still lose a tiny bit of water vapor this way from our atmosphere even at our current temperatures.)

The next natural question is…OK, it’s not necessarily the next natural question, but this is my post and I’m going to go there anyway: So what would happen if one of those mostly-ice objects somehow ended up getting close to the Sun? The same thing.

You don’t have to take my word for it. This actually happens, a lot. Have a look.

Comet Hale-Bopp

Yes. Comets are basically bodies from the outer solar system that somehow end up getting into an orbit that brings them closer to the Sun. They spend billions of years “out there” just minding their own business, when some other body–perhaps another comet, or a planet, maybe even a rogue planet (one that has escaped its parent star) wanders through and perturbs its orbit, and it drops towards the Sun.

It’s now in a highly elliptical orbit. Depending on where it came from the comet may be regarded as a “short period” comet if it came from the Kuiper Belt or the scattered disk–places I talked about last time–or it may be a “long period” comet if it came from further out.

Further out?

It’s the existence of so many long-period comets that has convinced astronomers that the Kuiper Belt and scattered disk are not the outermost parts of the solar system. Instead it’s thought that these long-term comets originate from a very sparse and gigantic zone called the “Oort Cloud” (pronounced like “port” without the “p”) named after Jan Oort who first proposed it. (Note the third Dutch astronomer who has had a major role in this series on the solar system.)

These orbit anywhere from 2000 to 50,000 AU, though estimates of that upper end vary; I’ve seen numbers as high as 200,000 AU for the upper bound, and so will you by the time you finish this.

For reference, the nearest (other) star to our solar system is at a distance of 268,551 AU (or 1.3 parsecs or 4.25 light years). [Which should tell you how ridiculously far apart stars are in comparison to the sizes of solar systems…much less the sizes of the stars themselves.]

We have never, ever detected an object that is in the Oort Cloud. Too far away, and too small. We only know about it from backtracking comets. And because of these “ambassadors” from the Oort cloud, we know a fair amount about the objects in the Oort Cloud, as a class. We can’t send a probe to them, not in this lifetime, but they sometimes come most of the way to us.

History

Comets have been known, and feared, since ancient times.

The night time sky is mostly changeless. Oh, the stars shift a bit westward from one night to the next, but after a full year, you’re back where you started from; that in fact is a direct consequence of our yearly orbit about the Sun.

We see planets and the moon moving around, but they are at least somewhat predictable (even by very ancient peoples); they tend to stick being near a band about the sky called the ecliptic. In fact the Sun stays on the ecliptic though that’s a bit harder to see since you can’t see the Sun and the stars at the same time. The point being the planets were predictable and though some people tried to do “woo” with planetary positions, people in general weren’t scared of them.

There were also shooting stars, but even though those are quite unpredictable, they’re fairly frequent.

But a comet? Comets are big, spectacular, hang around for months, and completely unpredictable. There could be a big one next year. Or not. Thus they tended to be regarded as bad omens.

And then came Sir Isaac Newton and Edmond Halley.

Isaac Newton, I’ve discussed enough. He was able to show that a force that could be described mathematically (and thus, precisely) was responsible for the orbits of the planets. At that point they became viewed as essentially a clockwork. His work was published in Philosophiae Naturalis Principia Mathematica in 1687, thanks in part to Edmond Halley’s funding and encouragement.

Halley had already made observations of a comet that showed up in September of 1682. He used that data to show that that comet, too, was in an orbit fully consistent with Newton’s gravitation, but rather than a nearly circular orbit, the comet was in a highly elliptical orbit–one with an eccentricity of 0.96658, where 0 is circular and 1.0 is a parabola or line segment. And the orbit has a period of 76 years. Its semi-major axis (i.e., halfway along its length) is 17.737 AU, its nearest approach to the Sun is 0.59279 AU (inside the orbit of Venus), while its furthest distance is 35.14 AU, beyond the orbit of Neptune (which wasn’t known yet!).

Halley published this in 1705, along with data on other comets.

But here was the key implication: There’s be another comet in 1682+76=1758, but it would actually be the comet of 1682, returning.

And sure enough, sixteen years after his death in 1742 at the age of 82, a comet showed up…and it was in the right place, following the right path. That comet is now known as “Halley’s Comet.” (“Halley,” by the way, rhymes with “Valley,” at least that’s the way most people with that name pronounce it today. We’re not 100% sure that’s they way they pronounced it back then, it might have rhymed with “Holly.” Or it may actually have been Hail-ee, as it is commonly pronounced by non-astronomers.)

[Note, by the way, that the animation shows Halley’s comet orbiting clockwise. Yes, it’s retrograde just like irregular satellites are. But if you think about it other than minimum distance this looks an awful lot like an irregular satellite.]

Halley had predicted a comet. And thus, comets became something explicable. Sure, we couldn’t predict when the next long term comet would show up, but the short term ones we could predict like clockwork, and either kind, once visible, would follow predictions as to their path across the sky.

Well, mostly. The difficulty is, that an orbital calculation assumes the object isn’t under any kind of thrust. But when a comet is near the Sun, it’s constantly outgassing as it warms up…and those jets of gas act like random rocket burns. But now we knew what comets are, and that took all of the supernatural “woo” out of them.

And the terror. Well, mostly; but 1910 is a special case of panic caused by scientific illiteracy.

Once comets became an irregular but nevertheless normal phenomenon, astronomers started looking for them. Any unexpected, diffuse blob in a telescope could turn out to be a comet in the early stages of warming up and outgassing. Charles Messier (1730-1817), in fact, made it a hobby to look for comets, and made a catalog of objects–ones that were nebulous in appearance but were not comets–that had fooled him, so that he could check against it in the future to weed out false alarms. This is now known as the Messier catalog, and although it’s by no means comprehensive (it has 110 objects in it), it’s famous. Many objects in the sky are known by their Messier numbers, for example M 31 in Andromeda (the “Andromeda Galaxy”) or M 1, the Crab Nebula. Amateur astronomers even hold “Messier Marathons” during the one month of the year when they are all visible sometime, somewhere, between dusk and dawn, trying to get all of them. (On my one attempt, I got all but 15 or so of them.) Messier did discover 13 comets, and co-discovered a fourteenth.

Now that we knew what we were looking for, we have found Halley’s comet in records from 240 BCE, in Chinese chronicles. And then in 164 BCE in a couple of Babylonian tablets…actually fragments of tablets. And again in 87 BCE in more Babylonian tablets. (And it may be depicted on Armenian coins.)

The appearance of 12 BCE was recorded in China. It likely passed pretty close to Earth then. It so happened that in Rome, Marcus Vipsanius Agrippa died at that time, so the Romans took it as an omen of his death. It is also sometimes cited as a possible Star of Bethlehem (though it seems a bit early for that to me).

There is a possible record of the appearance of 66 CE, the Chinese recorded its appearance in 141. Then we apparently missed one, because the next one is 374, then 451 (heralding the defeat of Attila the Hun). Past that point, we can find every single appearance in the records. The most famous of these was in 1066, meaning someone was going to have a very bad year. Well, it was either going to be Harold (if he lost the English throne) or William (if Harold stopped him from seizing the British throne). It’s convenient that no matter what happens, the comet will turn out to have been an omen! And of course we know that Harold lost out to William the Conqueror, bringing the French language with him. (And English spelling has sucked ever since.)

The comet is depicted on the Bayeaux Tapestry, telling the history of the Battle of Hastings:

Speaking of the Star of Bethlehem, in 1305 Giotto di Bondone produced a work, the Adoration of the Magi, which depicts the star of Bethlehem as a comet. How did he know what a comet looked like? He had seen Halley’s comet in 1301, and that time, it was visually spectacular.

As it turns out, one of the probes that visited Halley’s Comet in 1986, was named Giotto after this artist.

In 1835 the comet appeared, and Mark Twain was born two weeks after its closest approach to the Sun. It was during this apparition that German astronomer Friedrich Wilhelm Bessel (who also developed the Bessel functions–very eclectic stuff) suggested that jets of evaporating material might supply enough force to alter a comet’s orbit.

In 1909 Twain stated that he “came in with Halley’s comet in 1835. It is coming again next year, and I expect to go out with it. It will be the greatest disappointment of my life if I don’t go out with Halley’s comet. The Almighty has said, no doubt: ‘Now here are these two unaccountable freaks; they came in together, they must go out together.'” And sure enough, Twain died on 21 April 1910, the day after the comet’s closest approach to the Sun.

In 1910, we had the benefit of spectroscopy and photography. We could tell from the light, what the comet was made of. One thing found was the toxic gas cyanogen. Earth was expected to pass through the tail of the comet, so a panic ensued with people afraid all life on Earth would be snuffed out, and thus buying gas masks and “anti-comet pills” that were useless (a better record than COVID “vaccines”). The fact of the matter is that a comet’s tail is so diffuse it had no effect.

Here’s the comet in 1910, taken from the Yerkes Observatory, at the time home to the largest telescope in existence. (It still is the largest refracting telescope in existence.)

Based on my grandfather’s recollection, it was a spectacular appearance. Or perhaps he was remembering a different comet; the Great Daylight Comet of [January] 1910, which could be seen even in daytime!

Speaking of comet tails…now would be a good time to discuss the structure comets. Or it may be a bad time. But this is my post, so we will.

The Anatomy of a Comet

At the very heart of a comet is the nucleus. This is the icy object that–when it’s out in the Kuiper Belt, Scattered Disk, or Oort Cloud, just minds its own business, it’s a bunch of ice, dust, and rocks, mostly water ice but also carbon dioxide, carbon monoxide, methane and ammonia. They range from 100 meters across to possibly as much as 30 km across. Often they are called “dirty snowballs.” Comets that have passed by the Sun multiple times in the past will tend to have more rock and dust at their surfaces–any ice there boiled off during a previous visit. They are very dark in color, reflecting as little as four percent of the light that reaches them.

Surrounding the nucleus is the coma, it’s basically the sum total of all of the stuff that is outgassing from the comet, and any dust that is being carried along with the outgassing. It can be thousands or even millions of kilometers across.

Here you can see the nucleus of the Hartley comet, complete with very active jets of material:

The tails form…yes, I said “tails”…when the coma material interacts with either solar radiation or the solar wind. One tail will be curved and will consist of the dust and other (relatively) heavy particles. The other is the gas tail, pure gases, and that one will always point directly away from the Sun; these are lighter things that are pushed away instantly by the pressure of the solar radiation.

The gas tail glows because the gases become ionized…in other words it actually emits light. The dust tail, on the other hand shines by reflected sunlight (like planets do).

Tails have been known to be 3.8 AU long… that’s over half a billion kilometers.

The one statistic that I clearly remember reading a lot when I was younger was how rarefied a comet’s tail is. For all of the visual appearance, it’s a near perfect vacuum (just not as close as space normally is). But I haven’t been able to nail it down on the internet. Suffice it to say it’s very, very sparse.

Here’s an animation

So, comets are huge, when they’re active.

Comets that pass by the Sun multiple times will eventually run out of ice to have vaporize. They may then resemble asteroids, or the object may have no cohesion and become swarms of small objects–dust particles, mostly. Those can eventually cause meteor showers on Earth when the Earth eventually passes through them. There are a number of these over the course of a year, generally named for the constellation the meteors seem to radiate from as seen from the ground. Typically there are good and bad years for meteor showers, depending on whether Earth is cutting through the center of the swarm or not.

Categories of Comet

As alluded to above, comets are roughly divided between short period and long period. Short period, or to many astronomers, just plain “periodic” comets are generally those whose period is less than 200 years. Usually, but by no means always, they orbit in at a low inclination, close to the ecliptic, the plane of the planets’ orbits, and in the same direction as the planets. This is an important clue. Short term comets are generally former long term comets that passed too close to one of the planets and had their orbits perturbed. Many will be sub-grouped into “families” based on the outermost extent of their orbits; that’s thought to be an indication as to which planet did the deed. In the case of Halley’s comet, since its orbit extends just a bit past Neptune’s orbit, it’s believed that Neptune perturbed its orbit. The largest of these families is (no surprise) the Jupiter family. There are also comets that orbit within the asteroid belt…they have the right composition, but very little outgassing happens that far away from the Sun.

Long Period comets can have periods of thousands or even millions of years. Those latter are our evidence for the existence of the Oort cloud. Comets C/1999 F1 and C/2017 T2 (PANSTARRS) have a semi major axis of 35,000 AU and a period of six million years. If you missed them when they first showed up, you’re basically out of luck as far as seeing them the next time. You’ll have to wait for them to reach their maximum distance from the Sun…over a light year (!), then come back.

But some comets are literally never expected to come back; those are the single-apparition comets.

If the Kuiper Belt and Oort cloud seem a bit bewildering here is another diagram for comparison…actually it’s three diagrams, one each of the asteroid belt, Kuiper Belt and Oort cloud. These are not drawn to any kind of scale; for instance in the last diagram the planet orbits and Kuiper belt are much too big; and as always the planets themselves and even the Sun are drawn much too large (they should be much less than one pixel in size).

Other Famous Comets

There are over 3,500 known comets. Most never get bright enough to be seen with the naked eye, but some become famous for one reason or another. Halley’s comet, of course, is the undisputed celebrity.

9P/Tempel was discovered in 1867 by William Tempel, and has a 5.6 year period. We lost track of it in 1898 and assumed it had disintegrated, but it was rediscovered in 1967. It turned out that its orbit had been perturbed, and that is how we lost it; it wasn’t where we expected it to be. We have sent probes to this one.

Kohoutek (C 1973 C1) in 1973 was a fizzle. Early estimates of how bright it would get made it seem as if it would be one of the brightest comets of the century, but then…big nothing! And it faded from sight by the end of January 1974. It’s hard to predict how bright a new comet will be, because we rarely have a good feel for how much ice it has, how deeply it’s buried, and so on. On a comet’s second trip, though, we will have a past history to go off of.

Kohoutek is a classic long term comet. Its measured eccentricity was between 0.9999 and 1.0. A 1.0 orbit is an escape orbit (barely), so we don’t expect to see Kohoutek again any time soon. Current estimates are that it is in a 75,000 year orbit. It passed only 0.14 AU from the Sun, meaning it went inside the orbit of Mercury.

Hyakutake in 1996 passed very near Earth (about 15 million km) over the north pole and was readily visible late at night (rather than being buried in twilight. I went outside the city away from the lights to see it as it traversed the Big Dipper and it noticeably moved in just ten or fifteen minutes. This was an unusual opportunity, comets are usually brightest (as seen from Earth) near the sun so it’s unusual to see a bright comet in a truly dark sky.

The comet came in from “below” the plane of the ecliptic (bottom center), crossed the plane of the ecliptic then over our north pole on March 22, zipped through perihelion (closest approach to the Sun, then dropped below the plane of the ecliptic and exited, lower right. Unlike with Kohoutek, this probably isn’t Hyakutake’s first visit; it’s in a 17,000 year orbit with an excentricity of “only” 0.99989.

The Ulysses spacecraft–one studying the Sun–passed through Hyakutake’s tail.

Hyakutake, however, was overshadowed by Hale Bopp, just a few months later in 1997. Hale Bopp is actually the comet I used at the beginning of this post. I unfortunately never got a good look at it. At most I saw some fuzz at twilight, and then it would set. I could never get far enough away from the city fast enough at sunset to get a good look at it. Apparently it came into its own later, after I had given up on it. So for me Hyakutake was “the” comet.

So I really missed the boat on this one, but I’ll get another crack at it in abut 2400 years. This is by no means a short-period comet but it has a significantly shorter period than Kohoutek and Hyakutake, and its orbit has a semi-major axis of a mere 177 AU.

Shoemaker-Levy 9 This one, no one would ever have cared about (other than Carolyn and Eugene Shoemaker, and David Levy, the co-discoverers of it the comet. They discovered it in 1993…and it had already broken into 21 pieces, probably sometime in 1992 when it approached Jupiter (yes…tidal forces!). But then when they plotted its orbit, the astronomers realized two things: the pieces were actually in orbit about Jupiter, not the Sun, and also that they were going to make direct hits on Jupiter in July of 1994! (Hard to believe that was thirty years ago!)

By the time it hit, Shoemaker-Levy 9 was in twenty one pieces and every one of them hit Jupiter.

The comet fragments were up to 2 km in diameter…meaning before it broke up it was actually pretty big.

How would Jupiter hold up getting pummeled like this?

The bad news is the pieces hit just into the dark side of Jupiter. That means we couldn’t see the actual moments of impact from Earth. Hubble got retasked to look; The Ulysses probe got retasked…and the Galileo orbiter was 1.6 AUs out, but it could actually see the impact site. NOTHING was more important than this.

One of the most famous pictures in astronomy is of the black holes the impacts left in Jupiter’s atmosphere.

The largest piece, G, hit with 6,000,000 megatons of of energy. It took months for the atmosphere to recover from the hits. Some of the blemishes were the size of Earth.

Perhaps we will leave such smoking holes in the Deep State, shortly.

This was particularly poignant for Eugene Shoemaker. He almost got to go to the Moon on Apollo 17 as the geologist, but for medical reasons never got to do it. He was however the head of the geology program for many years..

But one of his big “things” was warning people about the dangers of possible future asteroid and comet impacts. He spent time studying Meteor Crater in Arizona, he discovered that the Ries in Germany was an old impact crater (that wasn’t hard. It turned out that St. George’s church in Nördlingen was built out of rock that clearly had been altered by the force of an asteroid impact (it’s very distinctive; no volcano or other Earth-bound force can produce it). After that all he had to do was find the right quarry in order to bag his…er…quarry.

Geologists and astronomers had pooh-poohed his warnings, but Shoemaker-Levy 9 vindicated him completely. Now we’re quite aware of the very real danger of being hit by one of these objects. We’ve had two significant…but still very small…pieces hit since 1900, both in Russia: 1908 Tunguska and 2013 Chelyabinsk.

Exploration

When recounting the history of Halley’s comet, I stopped at 1910, not 1986. That’s because we were able to send probes…yes more than one…to the comet because we had plenty of advance notice. In fact we sent five probes. The European Space Agency sent Giotto, the Soviet Union sent Vega 1 and Vega 2, Japan sent Sakigake and Suisei.

NASA didn’t do a damned thing. However they did send a mission, ICE, to another comet the year before, and therefore the first mission to study a comet was an American probe. Another six missions have been sent to other comets since, including one lander and one deliberate impact:

Deep Space (launched 1998) used an ion drive for manuevering. It had two targets, it missed its first target and managed to reach its second target.

Stardust (launched 1999) actually captured dust from Wild, one of its target comets, and launched a capsule that returned that dust to Earth. So we got to put bits of comet into test tubes in a lab here on Earth. The other comet was…well let me hold that until later.

CONTOUR (launched 2002) was intended to study two comets but failed. Plan B was to head to yet a third comet, but the spacecraft couldn’t be contacted. Can’t win ’em all.

All missions up to that time were flybys, but we actually set up an orbiter, Rosetta, launched by the European Space Agency in 2004. It orbited 67P Churymov-Gerasimenko in 2014 and attempted to land. In the meantime, it took pictures, like this one.

Rosetta had company; ESA had launched two probes on the same day and Philae‘s purpose from the start was to land on the comet. It actually ended up bouncing multiple times, and ended up in partial shadow, limiting its useful lifetime. Philae was last heard from in 2015.

Finally there was Deep Impact, launched in 2005. Yes, one of the two big “asteroid hitting the Earth” movies from 1998 bore that name, but neither Wikipedia page references the other, so there’s not even a “name inspired by…” connection that I can find. The goal here was to study the internal composition of a comet, so the probe actually launched an impactor, and then photographed the light flash. That was comet 9P/Tempel (a fairly well known comet, though not as famous as Halley’s comet). The main craft went on to take the picture of Hartley I showed above.

Tempel is actually a fairly well known comet, it was first observed in 1867 by William Tempel, and has a 5.6 year period. We lost track of it in 1898 and assumed it had disintegrated, but it was rediscovered in 1967. It turned out that its orbit had been perturbed, and that is how we lost it; it wasn’t where we expected it to be.

Here is a composite image based on photographs taken by Deep Impact before the impact.

Here is a photograph taken by the impactor, before it became like a bug on a windshield, on July 4, 2005.

If that’s a bit boring. how about an “oh, SHIT!” GIF?

Or as seen from the main spacecraft:

The impact speed was 10.3 km/second and delivered energy equivalent to 4.7 tons of TNT. We predicted that the crater would be about 100 m across. Only in 2011 did we find out…thanks to a flyby by Stardust, that the crater was roughly 200 m across.

The Impactor bore a CD with the names of 625,000 people encoded on it.

Smack! in Popular Culture

What would happen if one of these hit the Earth?

Well, it would suck. A 1 km wide body hitting us would make every hurricane and earthquake in history put together look like nothing; the entire planet would be affected.

Consider that a long term comet will be moving at pretty close to solar escape velocity. Which when it hit the earth would be about 42 km/sec. Earth would be moving at 30 km/sec. The typical scenario is a right-angle collision, basically Earth getting T-boned by the comet; that’s a collision speed of 51.6 km/sec. Under very unusual (but not impossible) circumstances where the comet’s closest approach is 1 AU and it happens to be headed in exactly the opposite direction to Earth’s motion it could be a head-on collision at 72 km/second, but that’s so unlikely that it’s only worth contemplating if you are so tired of winning that 51.6 km/sec isn’t enough to adequately ruin your day.

An object of, say, 1km in size popping in at that speed would be catastrophic, especially if it hit the ocean. Humanity would probably survive–a death toll of 90+ percent is not 100 percent, but the survivors might find themselves blown back into the stone age…and the lasting effects would make “climate change” look like a mouse fart. Make the asteroid or comet much bigger and…we probably wouldn’t survive.

Tempel, by the way, averages about 6km across. Fortunately it doesn’t cross our orbit and if it did, it wouldn’t be at quite that high a speed.

This doesn’t mean we haven’t contemplated both comet and asteroid strikes. We know an asteroid strike either killed off the dinosaurs, or helped do so. We have those two movies from 1998, Deep Impact and Armageddon. Deep Impact was from a scientific basis a much better movie but it didn’t have Bruce Willis in it.

We also have fiction. Lucifer’s Hammer (1977) was a book by Larry Niven and Jerry Pournelle. They’re both good authors, and they are even better when they work together. It details the discovery of a comet that’s going to come very close to Earth, and follows a number of different people before, during and after the impact. The survivors fight to maintain civilization in the face of torrential rains that lasted for months, hordes of other survivors reduced to barbarism, and the incipient ice age triggered by the impact. Highly recommended.

And then it turned out that the original concept of the novel was that alien invaders had deliberately caused the impact, this time with a moonlet brought from Saturn. For whatever reason their editors had rejected that concept, but Niven and Pournelle had the last laugh; in 1985 they published Footfall, quite possibly the best alien invasion novel ever. And yes, the aliens dropped one in the Indian ocean, killing billions. Also Highly recommended.

Where Our Water Came From

Not every cometary collision is a bad one though. I mentioned at the beginning of this post that Earth lost its water back at the beginning, so the question arises, how is it we have any now? We believe that it was mostly brought in by comets, shortly after the planet cooled. There were a lot more of them back then, and Earth did its part to reduce the numbers.

Nemesis?

In 1984, it was suggested that we might be a binary star. Some very faint red dwarf could be orbiting at about 95,000 AU, outside of the Oort cloud (depending on which estimate for its outer bound is correct), and perturbing comets’ orbits, eventually leading to huge numbers of comets reaching the inner solar system. This would make sense if the red dwarf were in an elliptical orbit, and doing the perturbing only when closest to the Sun. There seemed to be a 26 million year recurring pattern of mass extinctions (not as big as the dinosaur killer or the Great Dying at the end of the Permian, but mass extinctions nonetheless).

With an effect like that, the hypothetical star has been named Nemesis.

Surely we’d know already if we were a binary star? I mean, come on. We don’t see this except on movie screens.

Not necessarily! Most stars are red dwarfs, they’re incredibly faint. None of them are visible to the naked eye at night. None of them, not even the closest one we know of now, Proxima Centauri. So one of these would not be obvious. We’d only be able to tell if we happened to look at the right one and measured its distance and speed. There is a systematic survey being made of red dwarfs, starting with the ones that appear brightest and working their way down. Conceivably, we could get a “hit.” If it’s close enough we could even conceivably send a probe, but it’d be by far the biggest space project ever, and we wouldn’t live to see the pictures.

But as of now, Nemesis is considered very unlikely. Many astronomers think we may once have had a Nemesis but it could have been lost when another star came relatively close sometime in the past.

The End?

That’s comets in a nutshell. Many are denizens of the outermost marches of the Solar System.

As usual I could only scratch the surface of the topic.

This is, I believe, the last of the series on our solar system.

2024·11·30 Joe Biden Didn’t Win (And Neither Did Kamala Harris) Daily Thread

As of desired publication time, 12:02 AM on November 29th, there are 51 days, 11 hours and 58 minutes before our Once and Future President, Donald John Trump, is restored to his rightful office.

Not that I’m counting, mind you.

What is it that feeds our battle, yet starves our victory?

Speaker Johnson
Pinging you on January 6 Tapes

Just a friendly reminder Speaker Johnson. You’re doing some good things–or at least trying in the case of the budget–but this is the most important thing out there still hanging. One initial block released with the promise of more…and?

We have American patriots being held without bail and without trial, and the tapes almost certainly contain exculpatory evidence. (And if they don’t, and we’re all just yelling in an echo chamber over here, we need to know that too. And there’s only one way to know.)

Either we have a weaponized, corrupt government or we have a lot of internet charlatans. Let’s expose whatever it is. (I’m betting it’s the corrupt weaponized government, but if I am wrong, I’d like to see proof.)

Justice Must Be Done.

The prior election must be acknowledged as fraudulent, and steps must be taken to prosecute the fraudsters and restore integrity to the system.

Nothing else matters at this point. Talking about trying again in 2022 or 2024 is hopeless otherwise. Which is not to say one must never talk about this, but rather that one must account for this in ones planning; if fixing the fraud is not part of the plan, you have no plan.

Small Government?

Many times conservatives (real and fake) speak of “small government” being the goal.

This sounds good, and mostly is good, but it misses the essential point. The important thing here isn’t the size, but rather the purpose, of government. We could have a cheap, small tyranny. After all our government spends most of its revenue on payments to individuals and foreign aid, neither of which is part of the tyrannical apparatus trying to keep us locked down and censored. What parts of the government would be necessary for a tyranny? It’d be a lot smaller than what we have now. We could shrink the government and nevertheless find it more tyrannical than it is today.

No, what we want is a limited government, limited not in size, but rather in scope. Limited, that is, in what it’s allowed to do. Under current circumstances, such a government would also be much smaller, but that’s a side effect. If we were in a World War II sort of war, an existential fight against nasty dictatorships on the brink of world conquest, that would be very expensive and would require a gargantuan government, but that would be what the government should be doing. That would be a large, but still limited government, since it’d be working to protect our rights.

World War II would have been the wrong time to squawk about “small government,” but it wasn’t (and never is) a bad time to demand limited government. Today would be a better time to ask for a small government–at least the job it should be doing is small today–but it misses the essential point; we want government to not do certain things. Many of those things we don’t want it doing are expensive but many of them are quite eminently doable by a smaller government than the one we have today. Small, but still exceeding proper limits.

So be careful what you ask for. You might get it and find you asked for the wrong thing.

Political Science In Summation

It’s really just a matter of people who can’t be happy unless they control others…versus those who want to be left alone. The oldest conflict within mankind. Government is necessary, but government attracts the assholes (a highly technical term for the control freaks).

His Truth?

Again we saw an instance of “It might be true for Billy, but it’s not true for Bob” logic this week.

I hear this often, and it’s usually harmless. As when it’s describing differing circumstances, not different facts. “Housing is unaffordable” can be true for one person, but not for another who makes ten times as much.

But sometimes the speaker means it literally. Something like 2+2=4 is asserted to be true for Billy but not for Bob. (And when it’s literal, it’s usually Bob saying it.) And in that sense, it’s nonsense, dangerous nonsense. There is ONE reality, and it exists independent of our desires and our perceptions. It would go on existing if we weren’t here. We exist in it. It does not exist in our heads. It’s not a personal construct, and it isn’t a social construct. If there were no society, reality would continue to be what it is, it wouldn’t vanish…which it would have to do, if it were a social construct.

Now what can change from person to person is the perception of reality. We see that all the time. And people will, of course, act on those perceptions. They will vote for Trump (or try to) if their perception is close to mine, and vote against Trump (and certainly succeed at doing so) if their perception is distant from mine (and therefore, if I do say so, wrong). I have heard people say “perception is reality” and usually, that’s what they’re trying to say–your perception of reality is, as far as you know, an accurate representation of reality, or you’d change it.

But I really wish they’d say it differently. And sometimes, to get back to Billy and Bob, the person who says they have different truths is really saying they have different perceptions of reality–different worldviews. I can’t argue with the latter. But I sure wish they’d say it better. That way I’d know that someone who blabbers about two different truths is delusional and not worth my time, at least not until he passes kindergarten-level metaphysics on his umpteenth attempt.

Lawyer Appeasement Section

OK now for the fine print.

This is the WQTH Daily Thread. You know the drill. There’s no Poltical correctness, but civility is a requirement. There are Important Guidelines,  here, with an addendum on 20191110.

We have a new board – called The U Tree – where people can take each other to the woodshed without fear of censorship or moderation.

And remember Wheatie’s Rules:

1. No food fights
2. No running with scissors.
3. If you bring snacks, bring enough for everyone.
4. Zeroth rule of gun safety: Don’t let the government get your guns.
5. Rule one of gun safety: The gun is always loaded.
5a. If you actually want the gun to be loaded, like because you’re checking out a bump in the night, then it’s empty.
6. Rule two of gun safety: Never point the gun at anything you’re not willing to destroy.
7. Rule three: Keep your finger off the trigger until ready to fire.
8. Rule the fourth: Be sure of your target and what is behind it.

(Hmm a few extras seem to have crept in.)

(Paper) Spot Prices

Kitco “Ask” prices. Last week:

Gold $2,716.90
Silver $31.41
Platinum $973.00
Palladium $1,034.00
Rhodium $4,950.00
FRNSI* 130.430+
Gold:Silver 86.498-

This week, 3PM Mountain Time, markets have closed for the weekend. (This time, apparently, markets closed at 12:45, not 3PM.)

Gold $2,650.10
Silver $30.69
Platinum $954.00
Palladium $1002.00
Rhodium $4,850.00
FRNSI* 127.199-
Gold:Silver 86.351-

Gold took a ninety dollar thumping on Monday, seemed to be going nowhere the rest of the week, but has recovered a little bit on Friday. The same is pretty much true of the other precious metals, though one will note rhodium actually dropped a bit. The gold:silver ratio still sucks (if you’re a silver fan).

*The SteveInCO Federal Reserve Note Suckage Index (FRNSI) is a measure of how much the dollar has inflated. It’s the ratio of the current price of gold, to the number of dollars an ounce of fine gold made up when the dollar was defined as 25.8 grains of 0.900 gold. That worked out to an ounce being $20.67+71/387 of a cent. (Note gold wasn’t worth this much back then, thus much gold was $20.67 71/387ths. It’s a subtle distinction. One ounce of gold wasn’t worth $20.67 back then, it was $20.67.) Once this ratio is computed, 1 is subtracted from it so that the number is zero when the dollar is at its proper value, indicating zero suckage.

Flat Earth Cowards

Just remember that David Weiss, Eric Dubay, Mark Sargent, Nathan Oakley, Dean Odle, and Volker Meyer, all Flat Earth proponents on the internet, are intellectual cowards at best, and knowing fraudsters (politespeak for motherfucking liars) at worst, and I am in this case inclined to believe the worst.

After years of maintaining that the Sun does indeed set in Antarctica during the southern summer, but then claiming people aren’t allowed to go look, they’ve turned down the opportunity to go look. Worse, many of them condemn Jeranism, Whitsit Gets It, and Lisbeth Acosta for going.

Any reasonable person looking at this behavior should see the hallmarks of a fraudster. The fraudster wants you to believe what he says unconditionally. The fraudster wants you to 1) ignore the lack of evidence for his position and 2) the actual evidence against his position. This is a system for protecting lies.

Would someone condemn people for going and looking, if they sincerely thought their position was true?

These people are pushing bullshit and they know they are pushing bullshit. These people are lying turds.

By contrast, eight of the globers who spend time debunking flerfers are going, one is paying for himself, one is getting the free ride offered as part of TFE, the other six are crowd funded. Globers also crowdfunded Lisbeth to go when the anonymous donor who funded a drawing for the flerfers turned out to himself be a flerfer fraud. Globers crowd funding her, not flerfers. All of the globers (and many who are not going, such as Professor Dave Explains) have vowed to remove their anti-flat earth content and post a statement that the earth is flat, if the sun actually sets for those at the Final Experiment.

On The Fringes? The Trans-Neptunian Worlds

There are nine objects that are likely “dwarf planets” (i.e. objects too small to be “real” planets, but which are nevertheless rounded by their own gravity and orbit the Sun directly). It’s difficult to confirm the roundness of many of these as all we can see of them is a fuzzy blob, even with the Hubble Space Telescope.

Here they are:

Name
Minor Planet Number
min, max distances, (mean)
(in AUs)
Eccentricity (0=circular, 1=parabola)Inclination to ecliptic
(degrees)
Period (years)Year DiscoveredPrecovery Date
Ceres
1
2.55-
2.98
(2.77)
0.078510.64.601801
Pluto
134340
29.658-
49.305 (39.482)
0.248817.16247.9419301909
Quaoar
50000
41.900-
45-488
(43.694)
0.041067.9895288.8320021954
Sedna
90377
76.19-
937
(506)
0.849611.930711,39020031990
Orcus
90482
30.281-
48.067
(39.174)
0.2270120.592245.1920041951
Haumea
136108
34.647-
51.585
(43.116)
0.1964228.2137283.1220031955
Eris
136199
38.271-
97.457
(67.864)
0.4360744.040559.0720051954
MakeMake
136472
38.104-
52.786
(45.430)
0.1612628.9835306.2120051955
Gonggong
225088
33.781-
101.190
(67.485)
0.4994330.6273554.3720071985
Orbital Parameters of the nine likely dwarf planets

A word of explanation: The “precovery” date is the oldest image found of the object, when they go back looking to see if anyone ever accidentally photographed it. This seems like a bit of trivia, but those images can be extremely useful for determining the orbit of the object (not just the semi major axis, inclination and eccentricity but also the longitude of the ascending node, argument of perihelion and time of perihelion–those three orient the orbit (along with the inclination) and put the object at a certain spot in the orbit). This is why astronomers never throw away an astrophotograph; it may be beneficial decades later.

It should be noted that the full list of possible dwarf planets is 28 objects long, based on estimated diameters, though some have no names (just minor planet numbers). For the sheer sake of self-preservation, one should probably hope that 229762 Gǃkúnǁʼhòmdímà does not make the list, as !Kung words are notoriously hard to pronounce. (No, I am not making that up.)

By the opposite token, only Ceres and Pluto are absolutely solidly confirmed to be dwarf planets; it pretty much takes a spacecraft mission to confirm it.

Ceres is an outlier, obviously, because it’s the only object in the table that isn’t a trans-Neptunian object. I’ve covered asteroids already, so from this point forward I am going to ignore the world Ceres. (Never was much into baseball anyway.) Aside from Ceres the other oddball is Sedna, with a huge eccentricity and a huge orbit; it makes all of the others pale in comparison.

What would a well behaved full-blown classical planet look like in that table? It would have a low eccentricity and a low inclination. Quaoar actually behaves more like a planet than any of the others in the table (even including Ceres).

Here is another diagram, showing relative sizes, shapes, colors and brightnesses of these and some other objects. The color is of course an average color. In some cases there’s uncertainty as to size (as with Sedna), in which case a half-arc is shown at the maximum diameter. This one might reward a right-click-and-open-in-new-tab.

So now let’s take a look at these in more detail; I’m going to save Sedna and Pluto for last (and not bother at all with Ceres).

Quaoar

Quaoar (pronounced kwah-wahr, though more strictly speaking it should be “kwa’uwar” with the ‘ representing a glottal stop as you hear in the Hawaiian pronunciation of Hawai’i) is named after a deity of the Tongva people, and for me at least that answers nothing until I go look up “Tongva people.” It turns out they were a tribe in what is now the Los Angeles basin. (They also call themselves the Kizh.) Their language is distantly related to Aztec.

Quaoar was discovered 4 June 2002 by Chadwick A. Trujillo and Michael E. Brown at the Palomar Observatory (they were not using the big 200 incher but one of the smaller (but still big) instruments, the Samuel Oschin telescope. They were running a survey looking for Kuiper belt objects (little did they know…). Once it was determined that Quaoar was not in a resonance with Neptune (making it a qubewano-class TNO), the naming convention dictated it be named after a creation deity; Brown and Trujillo consulted with some present-day Tongvas to be sure it was an appropriate name.

Quaoar is an elongated ellipsoidal shape averaging 1090 km across, making it less than half the size of Pluto (2,376.6 km). (We know it’s not perfectly spherical because its brightness varies over a span of 17.68 hours–which we infer is its day. This could just be brightness differences, like with Iapetus, but we’ve also watched Quaoar cross in front of stars and timing the length of the blackouts leads to different estimates of the diameter.) Quaoar is also a very dark object reflecting only 12% of the light it gets from the Sun (which ain’t much to begin with!) It’s somewhat reddish, like 20000 Varuna and 28978 Ixion (both objects that are on the “long list” of possible dwarf planets).

So if it’s not really round, what’s the deal with it being considered a dwarf planet? Normally any rocky body over 900km or so, or any icy body between 200-400 km across should go round. If it’s slowly rotating it should be a bit oblate (wider at the equator than through the poles). A faster rotation should resemble Haumea’s case (see below). So how can Quaoar not be round? It’s absolutely big enough. It’s possible that Quaoar used to rotate more quickly, froze into shape and then Weymot slowed its rotation down due to tidal effects. (Saturn’s moon Iapetus has a similar situation going on but is not as extreme.)

Here are the discovery images put together as a GIF. It’s easy to spot when there’s an arrow, isn’t it?

And now (drumroll) our best image, from the Hubble space telescope:

And yes, Quaoar has a moon, Weywot, discovered by Brown in February 2007; Weywot is the son of Quaoar in Tongva mythology. Weywot is about 200 km across (though some places in Wikipoo show it as smaller), which makes it too small to be rounded (the smallest rounded object known is Mimas (Saturn’s “Death Star” moon), at 396.4 km; there is at least one non-rounded objects that are larger: Neptune’s moon Proteus). Quaoar also has a ring.

Here are a couple more diagrams, the first being a picture of Quaoar’s orbit (in cyan and blue) compared to Neptune (white) and Pluto (red). The two spheres are not only about the right sizes, comparatively speaking (but not compared to the size of the orbits!), but they are correctly colored (an average color) and even the brightness (albedo) is correct.

And another, an “overhead” view with Quaoar in yellow, Pluto in magenta/pink, Neptune in blue, and a few other TNOs in a drab green.

On the whole, we know next to nothing about this one…and that’s pretty much going to be true of most of the others. They’re just too doggone far away.

Orcus

Orcus is estimated to be anywhere from 870-960 km across, thus about the size of Ceres. It’s fairly bright, neutral in color and largely made of water ice; apparently the ice is mostly crystalline so maybe sometime in the past there was cryovolcanism (i.e., water volcanoes).

Orcus was discovered by Michael Brown, Chad Trujillo and David Rabinowitz on 17 February 2004 (note that two of these astronomers also discovered Quaoar). In this case, Orcus got named after one of the Roman gods of the underworld, because it’s a plutino.

What is a plutino? Plutinos are objects that, like Pluto, are in a 2:3 orbital resonance with Neptune, orbiting twice in the time it takes Neptune to orbit three times. (Note in the chart above it has nearly the same year, and mean orbital distance, as Pluto.) But Orcus tends to be furthest away from the Sun when Pluto is closest, and vice versa.

Here we see a Hubble Space telescope image of Orcus, and its moon Vanth. Vanth is estimated to be 475 km across by some, which is easily large enough to end up in that “Medium Small” 250-500km size bucket with Mimas, Hyperion, Proteus and Nereid, but other estimates put it below that 400 km line yet still in that bucket. Considering it’s likely frozen solid, and how rigid ice is at those temperatures, it’s not expected to be a round moon. (Note that I made a point to talk about any moon in that size bucket, and above, as I went through the 8 big planets.)

Vanth was named after an Etruscan deity, a “psychopomp” who guides the deceased to the underworld.

It is, however, big enough that the center of gravity of the Orcus-Vanth system is actually outside of Orcus, making it a double object. Vanth orbits Orcus in 9.54 days, and appears to rotate in the same amount of time. The rotation of Orcus, on the other hand, has been harder to nail down, so we don’t know if both bodies are tidally locked or just Vanth.

All in all, Orcus is often thought of as an “anti Pluto” since it’s phased the opposite of Pluto and has a (proportionately) large moon like Pluto. It’s even more striking when you see the visual of the orbit (Neptune’s orbit in white, Pluto’s orbit in red, Orcus in cyan and blue–note the color changes when the object crosses the ecliptic, and note the spheres are to scale with each other, the correct colors and albedos, again):

Haumea

Haumea is named after the Hawai’ian goddess of childbirth. It was discovered by Mike Brown at Caltech, but announced by a team headed by Jose Luis Ortiz Moreno at the Sierra Nevada Observatory…not our Sierra Nevadas, but rather the ones in Spain. There’s controversy over who should get the credit for this one. It’s the third largest TNO after Pluto and Eris. Here’s a picture, again from the Hubble Space Telescope:

This one’s a bit odd. Based on watching it fluctuate in brightness, it’s a very elongated triaxial ellipsoid, meaning it has a long axis, a medium axis at right angles to that, and a short axis at right angles to the other two. Here’s an artist’s rendering of Haumea:

But this is actually the shape one would expect of a rapidly rotating object under hydrostatic equilibrium; Haumea rotates in about four hours.

So how long are the axes? Haumea is roughly 2100 by 1680 x 1074 kilometers. Or perhaps 2322 x 1704 x 1026. Depending on whose numbers you believe. Either way, it’s a sizeable object.

Haumea has moons, as you likely noticed…not just one but two of them known so far. Hi’iaka (upper right in the picture) is a medium-small moon about 310 km across, in that same “bucket” as Mimas, but probably not rounded. Namaka (lower left) is roughly 170 km across. They are named after two daughters of Haumea, the patron goddesses of the Big Island of Hawai’i, and the sea, respectively.

(That brings us, by the way, to the end of the list of medium-small moons: Mimas, Hyperion, Miranda, Proteus, Nereid, Vanth, and Hi’iaka… or does it? It turns out ttwo additional objects on the long list of possible dwarf planets, Salacia and Varda, also have moons in this size bucket. And there’s an almost perfectly-matched double body, Lempo (at 272 km) and Hiisi, with the best estimate for Hiisi being 251km (just squeaking by). If there’s one thing about TNOs, it’s that they tend to have comparatively large moons!)

Haumea is as bright as snow, with an albedo of 0.73…meaning that 73 percent of the light that hits it is reflected back. It seems to have crystalline ice on it, which is puzzling, because crystalline ice should only form above 100 K, and Haumea is at 50K, and only amorphous ice should form at that temperature. Furthermore once it forms, cosmic rays plus what’s left of the solar wind out there should degrade it to amorphous ice in about 10 million years. On top of that, old surfaces out there end up covered in tholins (“star tar”), making them appear red. So it seems that Haumea’s surface is new, but we don’t know how that could have happened. (I could spitball it, but that would be worth less than you paid for this article.)

Haumea appears to have a ring, discovered as it passed in front of a star.

Haumea turns out to be the largest member of a family of objects that have similar orbits and it appears they may all be remnants of a larger body that broke apart due to a collision. But it appears to have happened at least a billion years ago based on orbital dynamics considerations, so that won’t explain the white, crystalline ice surface of Haumea.

The New Horizons probe that went to Pluto actually took some pictures of Haumea on three different occasions…from quite a distance however. The 2007 shots were from 49 AUs away, others were in 2017 at 59 AU and in 2023 at 63 AU. Still, being able to compare the “side view” from what we see on Earth has been helpful.

Haumea’s orbit turns out to resemble Makemake’s (see below). As a bonus Quaoar is also shown:

Eris

We talked about Eris a lot last time. With a diameter of 2326 km it’s a smidge smaller than Pluto, but it’s denser (more rocks, less ice) but is considerably more massive than Pluto, 27% more in fact. As pointed out last time, if Pluto is a planet, Eris is too.

Here are Eris and Dysnomia photographed in 2006, and we’re lucky to have this, because at the moment Eris is 96.3 AUs from the Sun.

Here’s the same sort of orbital diagram I’ve showed for the others…but note in this one Neptune’s orbit is quite small.

MakeMake

Makemake (MAH-ke-MAH-ke) is comparable in size to Saturn’s moon Iapetus, or 60% the diameter of Pluto. From what little of it we see, it may actually have geothermal activity, even though it’s one of the coldest bodies in the solar system at 40K. (When you see the words “possibly nitrogen ices” in a wikipoo article, you know the place is colder than Hitlary Klinton’s lap.) It’s named after a creator god in the Rapa Nui mythology of Easter Island. Again, Michael Brown is on the list of discoverers. And again we have a fuzzy image from Hubble Space Telescope.

And yet again, we have a moon, one that hasn’t been named yet.

Makemake is bright enough–brighter than any TNO other than Pluto–that perhaps it should have been discovered much sooner (maybe even by Clyde Tombaugh). There are even claims that Tombaugh in fact should have seen it, but it was buried right in the Milky Way and with all those stars around it, it would have been hard to spot. However, it hasn’t been spotted in any of his photographs, so it’s not that he photographed it and didn’t notice. It turns out the earliest precovery date is 1955 and Tombaugh stopped looking for additional objects in 1943.

Here’s another one of those graphics of the orbits, as usual the ecliptic in white, Pluto in red. Haumea is in green and MakeMake is on the blue line. The closest and farthest approaches to the sun (the perihelia and aphelia are given. The spheres are correctly sized, the correct colors and the correct albedos.

Gonggong

Discovered by Megan Schwamb, Michael Brown and David Rabinowitz on 17 July 2007, again as part of that Palomar Distant Solar System Survey. Megan Schwamb actually was the first to spot it with the blinking technique that Tombaugh used to discover Pluto. Gonggong is a water god in Chinese mythology, usually depicted as having a copper and iron human head on a serpent’s body. Gonggong is often accompanied by Xiangliu, his minister, a nine-headed poisonous snake. Both are associated with flooding catastrophes.

But enough about the Deep State.

Gonggong is 1230 km across (give or take 50 km), about half the width of Pluto, and a fairly dark body. Here is another Hubble Space telescope image:

And yes, there’s a moon, named Xiangliu, of course.

Gonggong is very red, so almost certainly covered in tholins. There is some water ice, so maybe there was some cryovulcanism in the distant past.

It’s a lot like Eris in having a large orbit, as seen in this polar view (view from above) in which both it and Eris are shown:

And the same thing, seen from the side:

Gonggong and Eris seem to have similarly-extreme orbits (but not nearly the same orbit). Right now Gonggong is 88 AUs distant. Based on color and brightness it’s likely made of the same stuff as Quaoar.

Sedna

And now to go back to Sedna. Sedna is just…different from the rest. It’s red, it’s far, far away, and it’s going to get a lot farther away, eventually. It’s also the only one of these nine with no known moon. It’s very roughly 1000 km across. And because it has no moon whose orbit we can measure and time, we have only the vaguest notion of its mass. And now for a smashingly spectacular picture from Hubble Space Telescope:

Although I was flippant when I said that, if you think about it, it’s a huge acheivement to be able to take even this picture. Sedna is presently 83.55 AUs or 12.5 billion kilometers away. Right now Eris and Gonggong are further away, but that won’t remain true forever, since Sedna’s aphelion is 937 AU, not only busting into triple digits for the first time, but nearly reaching four digits.

Sedna is not the furthest though. There is a smaller object with and even more extreme orbit, 541132 Leleakohonua, perihelion 65.16 AU and aphelion…are you sitting down? of 2106 AU, with an orbital period of 35,760 years. However, this object is maybe 110 km across and in no way a dwarf planet. Right now it’s about 78 AUs out, getting closer to perihelion in 2078. (As a bonus the eccentricity actually busts the 0.900 mark at 0.93997.)

Neither of these objects would ever have been found if they didn’t happen to be at the near part of their orbits. Given that objects like this spend a lot less time near the sun than they do further away, there are probably a lot of them out there, simply too far away for us to detect.

Objects like this are so extreme, there’s now a new class of objects, “Sednoids” including these two plus one other (a bit less extreme than Sedna). Some have suggested that they’re really members of the inner Oort Cloud. (I haven’t talked about the Oort cloud…yet.)

There is also speculation that these crazy orbits are caused by encounters with a full planet out there somewhere, perhaps 400AU out. The fact that a lot of aphelions seem to be in very roughly the same place lends credence to this. Here are the three “Sednoid” objects (2015 TG387 is Leleakohonua’s provisional number):

Pluto (Finally)

An Ode to New Horizons

Until the Hubble space telescope, a typical photo of Pluto showed a bunch of white dots on a black background, and an arrow pointing to one of them. Pluto was only distinguishable from stars by its motion, which took days to become obvious.

Then Hubble Space Telescope took a look in 2003, and what it gave us, was used to make this animation, as Pluto did a full rotation in 6.4 days…retrograde, apparently:

Then suddenly in 2015…you could buy a fricking globe of Pluto. I saw one for sale in the observatory store at Griffith Park playing tourist one evening while on a business trip and there was no way it wasn’t coming home with me. That simple metal sphere encapsulated everything about our planetary space program…from a dot on a page to a real world, within my lifetime.

So what happened?

THIS happened:

The New Horizons probe went to Pluto.

We first had to get permission. According to Wikipedia:

In 1992 JPL scientist Robert Staehle called Clyde Tombaugh, requesting permission to visit his planet. “I told him he was welcome to it,” Tombaugh later remembered, “though he’s got to go one long, cold trip.”

Tombaugh passed away in 1997. A small portion of his ashes were on the New Horizons spacecraft. He got to go along for the ride. On the container is inscribed, “Interred herein are remains of American Clyde W. Tombaugh, discoverer of Pluto and the Solar System’s ‘third zone’ Adelle and Muron’s boy, Patricia’s husband, Annette and Alden’s father, astronomer, teacher, punster and friend: Clyde W. Tombaugh (1906-1997)”.

Could he have possibly imagined back in 1930 that in a very real sense, he’d get to go there?

By the time New Horizons launched in 2006, mere months before Pluto got “demoted” to dwarf planet, we had known (since 1978) that Pluto had a large moon, Charon, one large enough to qualify Pluto as a double planet. And we had found two others, Nix and Hydra, though they are much smaller. At the time, Pluto + Charon was the only known case of a moon that was so large in comparison to its primary that the barycenter (center of gravity) of the system was outside of the primary. As such both the planet and moon orbit a point out in space. Here is a series of pictures taken by New Horizons quite some time before closest approach.

New Horizons did something that back in the 1970s was deemed nearly impossible, a direct trip to Pluto. Back then Jupiter was just barely reachable by a probe of useful size; we could (and did: Pioneer 11, Voyager 1 and Voyager 2) get to Saturn, Uranus and Neptune by first going to Jupiter and getting a gravitational assist (a/k/a slingshot) from it.

But this time we went directly to Pluto. Actually, we did use a gravitational assist from Jupiter, but we didn’t have to. We’d have got there without it, albeit after three more years.

This involved launching the probe directly into a solar escape trajectory. How fast is that? At Earth’s distance from the Sun, it’s a bit over 42 kilometers per second. We had to break free of Earth’s gravity and then still be doing 42 km/sec with respect to the Sun, at which point, it doesn’t matter which direction you’re going, you’re never coming back to the Solar System. Of course in this case the direction did matter, we wanted to go to Pluto in particular. And also, we got 30 km/second of that 42 km/second from Earth’s speed around the sun, by launching in exactly the direction Earth was moving.

And to do this we made the probe as small as possible (the size of a desk) and put it on the biggest effing rocket we had, including special upper stages to push the thing harder once in space. It was the fastest thing we ever launched.

And now for the NASA animations. No audio in the first one (and note Pluto doesn’t look right–the animation was produced before the mission):

The second one is more “loaded” technically showing what the instruments are doing every moment, as well as spacecraft orientation. (It also has a music track.)

As you can see, Pluto’s moons were in orbits that made it look like a big target, but the object is to not hit the bullseye. New Horizons had to spend the entire time on July 14, 2015 looking at Pluto and its moons, without stopping to transmit to Earth (it would have to turn around to do that, pointing the big dish antenna basically towards the Sun and losing absolutely irreplaceable time). Only after collecting 6GB of data and with Pluto, Charon, and the other four moons in the rear view mirror, could the spacecraft contact Earth…and then spend the next eighteen months transmitting all of that data.

You can imagine the people at mission control bit their nails clean off, waiting. But then New Horizons phoned home. It had come through just fine and it had goodies to send us.

So what did we get?

1. This:

2. And this:

3. And this:

4. And this:

5. And this:

6. And this:

7. And this (ice volcanos highlighted in blue:

8. And finally (but not really, I could keep going on) this:

And that’s Pluto, yet more pictures and data were taken of its largest moon Charon:

And the other four moons; it’s probably easiest to just throw a composite image at you:

So needless to say we know a lot more about Pluto than we do about all of the other TNOs I’ve talked about, put together.

NASA does engage in CGI sometimes (in spite of the fact that the Flerfers claim it does–they’re generally completely wrong but not in this case) and they produced this video of what a flyby would look like, based on what New Horizons returned:

Pluto Itself

So…here we go.

Pluto was named after the Roman god of the Underworld, the corresponding Greek god was Hades. It’s 2,376.6 km across, give or take 1.6 km. And 0.2 percent as massive as the Earth or 17.7 percent as massive as the Moon. It orbits the Sun in 248 years, rotates once on its axis in 6.38680 days…but with an axial tilt of 122.53 degrees, it’s considered a retrograde rotation. (These numbers are awfully precise, on account of New Horizons.) At this particular time Pluto’s northern hemisphere is pointed towards the Sun, and New Horizons thus was unable to get the very southernmost part of Pluto, it was in darkness during the entire time of the encounter.

Pluto’s rotation is the same as Charon’s orbital period, which means that not only does Charon always show the same face to Pluto (as is true with every other major moon in the Solar System), but Pluto always shows the same face to Charon. Scientists will invent coordinate systems at the drop of a hat, and the line directly facing Charon is the 0 degree longitude line on any map of Pluto.

Geology and Geography

Oh, that reminds me:

Composite “Mercator” image of Pluto (it’s not really a Mercator projection when the latitude lines are equally spaced). Note that a lot of regions are named after spacecraft (Venera, Voyager, Pioneer, Viking) or astronomers (Lowell gets a Regio too). But also notice that a lot of the names come from fantasy and science fiction, like Balrogs and of all things, Cthulhu–though that one was often called “the whale” too. (Bad news on that last, it got renamed Belton Regio.)

Pluto has mountains and plains, and the first picture plainly shows the “Heart of Pluto” which simply had to be named Tombaugh Regio after Clyde Tombaugh. Tombaugh Regio is a plain, and by the way, is on the side of Pluto that faces away from Charon. The plains are mostly nitrogen ice (brrrr), with some methane and carbon monoxide, all in solid form of course.

The western and more distinct lobe of the “Heart” is Sputnik Planitia, a 1000 km wide basin of frozen ice, but as the second image shows it’s divided into polygonal cells, almost certainly convection cells that carry floating blocks of water ice crust and sublimation pits at the margins. There are signs of glacial flows both into and out of the basin. Furthermore, not one single crater was spotted, which indicates that Sputnik Planitia’s surface is less than ten million years old; in fact the latest work claims 140,000-270,000 years. There are also transverse dunes in Sputnik Planitia, which are formed by wind-blown particles, in this case of frozen methane.

What are the mountains made of? Water ice. When you order something “on the rocks” here, you mean it literally. The color ranges from charcoal black to dark orange and white; Pluto has as much contrast as Iapetus.

The fifth “This” above shows lots of 500 m high mountains from Tartarus Dorsa, the spacing reminds people of scales or tree bark. This doesn’t appear anywhere else we know of, except maybe on the unseen side of Triton…or perhaps in the Atacama desert. These are likely penitentes, icy spires that form in deserts, so named because they resemble large numbers of people at prayer.

Cutting through Tartarus Dorsa and Pluto’s heavily cratered northern terrain (and therefore younger than either) are a set of six canyons radiating from a single point; the longest is Sleipnir Fossa which is at least 580 km long.

And cryovolcanos. We’ve identified two possible cryovolcanos, Wright Mons and Piccard Mons. Piccard Mons is not named after Star Trek’s Jean Luc Picard but rather the French ballooning pioneer (two C’s, see?).

Pluto, in short shows an absolutely stunning variety of geology. Glaciological, surface-atmosphere (the dunes), impact (craters), tectonic, likely cryovolcanic, and mass-wasting (rocks falling down hill), it’s all there. This world turns out to be much more interesting than I expected back then.

Internal Structure

We know Pluto’s size. We know its mass. That means we know its average density; divide the mass by the volume. And we get 1.853 g/cm3. That means it’s a mix of rocks (things we think of as rocks) and ice, and it’s roughly 70/30 rock/ice. So we believe Pluto has a silicate (rock) core, surmounted by a mostly-water ice mantle and crust. It may even have a subsurface ocean like Europa and Enceladus. Though some think it may now be frozen, it’s just barely possible it was inhabited at one point. (This is one place where Wikipedia is a bit frustrating. The text makes it sound like no one believes there’s still liquid water down there, but the diagram indicates otherwise.)

Atmosphere

Pluto has an atmosphere as is quite evident in pictures 3 and 8 above. In fact getting New Horizons out there quickly rather than waiting a few more decades was partially motivated by this; Pluto is fairly close to the Sun right now, and that, we thought, would make the atmosphere more active. As Pluto got further from the Sun, its atmosphere might freeze out.

The atmosphere is made up of nitrogen, methane, and carbon monoxide, all sublimated from the surface ices, and in equilibrium with them (if any of them “snow” out of the atmosphere, then ices elsewhere on Pluto will sublimate to restore them). The pressure is anywhere from 1 millionth to 1/100,000th that of Earth.

Since New Horizons was launched, however, we’ve determined the atmosphere might actually thicken as it gets colder.

In any case, New Horizons‘s parting shot at Pluto was a backlit shot, used to image the atmosphere. Scientists have learned to take a “backlit shot” opportunity when it presents itself.

Moons

Pluto has five moons. And all of them are regular, orbiting in the plane of Pluto’s equator. Here’s a scale diagram…full scale, distances and diameters shown accurately (you rarely see those in astronomy!).

First up is Charon. Orbiting at 19,595.764 km from Pluto (give or take 7 or 8 meters!) and at 1212 km across, it’s a medium size moon according to the terminology I’ve been using, so now we have nine: Rhea, Iapetus, Dione and Tethys at Saturn, Ariel, Umbriel, Oberon and Titania at Uranus, and now Charon.

Pluto is 2376.6 km across. Compared to it Charon is huge. No, wait, yuge. It’s bigger than Ceres.

Charon was discovered in 1978, and named after the ferryman of the underworld in Greek mythology. (You had to pay him a coin to get ferried across. No word on what people who died in the Trojan war (centuries before coinage) had to do.) But that brings up a question. How do you pronounce “Charon”? The Greeks spell it Χάρων, and that X is like the ch in Bach. But no one in English-speaking countries says that, it’s either “Sharon” or “Karon.” The discoverer, James W. Christy (born 1938), maintains that he named it after both Χάρων and his wife Charlene, who was nichnamed “Char” (pronounced Shar), so he goes with “Sharon.” (I’m just insane enough I’d probably try to pronounce it with the ch in Bach if I ever had the chance to talk to someone about it. Y’all are both doing it wrong!)

Christy saw a bulge on the side of blobs taken of Pluto from the Naval observatory at Flagstaff. It would disappear and reappear regularly, indicating something in orbit about Pluto. In the image below (which is a photographic negative) there’s a bulge at the top on the left hand side, and no bulge on the right hand side. And so here’s an example of what Pluto looked like before HST looked at it.

Needless to say we have better pictures now.

A few years after Charon’s discovery, its orbit was edge on to us here on Earth and we could study the light curve and prove an object was transiting in front of Pluto, then behind it, even if we couldn’t resolve it as a separate fuzzy blob.

Charon is yuge compared to Pluto, and it’s the first case of a moon large enough that the center of gravity of the system is outside of the primary. Back before Pluto got demoted from planet status, many proposed that Pluto and Charon be considered a binary or double planet. And if Alan Stern succeeds in convincing people he was right, it might become one again.

In the following animation, you can see Pluto actually swinging around an imaginary point just outside of itself (and as seen above New Horizons confirmed this). There’s a black dot marking the barycenter, you’ll see it in front of Pluto when the moon is at the bottom of the image (the dot is apparently visible through Pluto in the animation). Note that Charon is closest to the viewer when it is at the top of the image. I was momentarily confused by this.

Which means that when I gave you Charon’s distance from Pluto, that was actually not the appropriate number. Its average distance from the barycenter, and thus the true size of its orbit (semimajor axis) is 17,181.0 km. It’s actually moving at a comparatively sedate 210 meters per second, and the orbit is almost perfectly circular. (The difference between the minimum and maximum distance from Pluto (not the barycenter) is a mere 6.31 kilometers.)

Charon’s density is known, 1.7 g/cm3, making it 55% rock to 45% ice (give or take 5 percent). We’re pretty sure the moon is differentiated (i.e., it has a distinct core) and may have once had a subsurface ocean. Here we have two distinct models of what Charon might look like on the inside:

…and…

And…we have a map.

Informal names given to the various canyons included Nostromo, Serenity, Argo, and so on, named after fictional ships including recent ones like from Alien and Firefly. The northern dark area was originally named Mordor. It appears to be formed from gases that escaped Pluto’s atmosphere and blew over to Charon, carried by the solar wind. The temperature here can get as low as 15K during winter, and some tholins will form. When it gets warmer, a balmy 60K, anything that’s still an ice will boil away, leaving the pole dark.

The Other Moons

The other moons, Styx, Nix, Kerberos, and Hydra, all named after creatures and features of the Underworld in Greek mythology, all have nice tidy circular orbits in Pluto’s equatorial plane. So they’re regular moons. All are less than 51 km across. The innermost, Styx, orbits 48,694 km out…considerably further from Charon. But this makes sense. It would have to be far away from the binary object Pluto/Charon or Charon would perturb Styx’s orbit as it swept by Styx on closest approach.

One more “Moon” is Pluto itself. Since it orbits the barycenter at a distance of 2035 kilometers, which puts the barycenter outside of Pluto’s 1188 km radius, Pluto, not Charon, is actually the closest orbiting body of the whole system.

Arrokoth

New Horizons was able to visit one more object beyond Pluto (blue), shown in green.

It’s 486958 Arrokoth (formerly nicknamed Ultima Thule). We didn’t know about it when New Horizons launched, but the pace of discovery of TNOs was so great we figured something would be out there we could visit with some expenditure of propellant, and Arrokoth (discovered in 2014, a bit over a year before the Pluto encounter) was chosen.

As a result, the second best known Kuiper Belt object is none of the ones I’ve mentioned so far, it’s this otherwise insignificant bit of ice and rock.

It appears to be made out of two smaller bodies, planetesimals that never became part of a planet, touching each other. The two small bodies are roughly 21 and 15 km across, for a total of 36 km along the long axis. Arrokoth orbits the Sun in 298 years. So we have our first high resolution picture of a small TNO.

We got enough data to create a geologic map:

It largely consists of a mix, a solid mix of amorphous water ice and rocky material. (It is not, unlike some objects of similar size, simply a clustering of gravel that is barely stuck together.)

It’s getting late. If you want a deeper dive on this, here’s the Wiki: https://en.wikipedia.org/wiki/486958_Arrokoth

Are We Done Yet?

The Kuiper Belt. Surely we are at the outer edges of the Solar System now. Aren’t we?

Nope. And ironically we know a lot about a region we’ve never seen. Next time.

2024·11·23 Joe Biden Didn’t Win (And Neither Did Kamala Harris) Daily Thread

58 days, 11 hours, 59 minutes until our Once and Future President, the Rightful President of the United States, is restored to his proper office.

Not that I’m counting, mind you.

[Assumes 0001 publication time. Wordpiss will be wordpiss and it’s unlikely to happen at that time.]

What is it that feeds our battle, yet starves our victory?

Speaker Johnson: A Reminder.

And MTG is there to help make it stick.

January 6 tapes. A good start…but then nothing.

Were you just hoping we’d be distracted by the first set and not notice?

Are you THAT kind of “Republican”?

Are you Kevin McCarthy lite?

What are you waiting for?

I have a personal interest in this issue.

And if you aren’t…what the hell is wrong with you?

Lawyer Appeasement Section

OK now for the fine print.

This is the WQTH Daily Thread. You know the drill. There’s no Poltical correctness, but civility is a requirement. There are Important Guidelines,  here, with an addendum on 20191110.

We have a new board – called The U Tree – where people can take each other to the woodshed without fear of censorship or moderation.

And remember Wheatie’s Rules:

1. No food fights
2. No running with scissors.
3. If you bring snacks, bring enough for everyone.
4. Zeroth rule of gun safety: Don’t let the government get your guns.
5. Rule one of gun safety: The gun is always loaded.
5a. If you actually want the gun to be loaded, like because you’re checking out a bump in the night, then it’s empty.
6. Rule two of gun safety: Never point the gun at anything you’re not willing to destroy.
7. Rule three: Keep your finger off the trigger until ready to fire.
8. Rule the fourth: Be sure of your target and what is behind it.

(Hmm a few extras seem to have crept in.)

Spot (i.e., paper) Prices

Last week:

Gold $2,563.30
Silver $30.30
Platinum $947.00
Palladium $974.00
Rhodium $4,950.00
FRNSI* 123.000-
Gold:Silver 84.597+

This week, 3PM Mountain Time, Kitco “ask” prices. Markets have closed for the weekend.

Gold $2,716.90
Silver $31.41
Platinum $973.00
Palladium $1,034.00
Rhodium $4,950.00
FRNSI* 130.430+
Gold:Silver 86.498-

The attention is on gold. It has recovered over $150 of the losses it took right after the election, just since last Friday. Alas, silver has not kept up, and the gold:silver ratio has gone up almost two points. Platinum still struggles to climb out of the gutter, while palladium seems more dynamic. Rhodium did move around a bit, but ended up where it was last Friday.

*The SteveInCO Federal Reserve Note Suckage Index (FRNSI) is a measure of how much the dollar has inflated. It’s the ratio of the current price of gold, to the number of dollars an ounce of fine gold made up when the dollar was defined as 25.8 grains of 0.900 gold. That worked out to an ounce being $20.67+71/387 of a cent. (Note gold wasn’t worth this much back then, thus much gold was $20.67 71/387ths. It’s a subtle distinction. One ounce of gold wasn’t worth $20.67 back then, it was $20.67.) Once this ratio is computed, 1 is subtracted from it so that the number is zero when the dollar is at its proper value, indicating zero suckage.

Reminder: Most Flat Earther Influencers are Liars

Most Flat Earther influencers like Flat Earth Dave and Eric Dubay have said for years that they want to go to Antarctica during southern summer and watch the Sun set…which would prove the globe model isn’t right. The globe model not only predicts the Sun will not set in Antarctica at and around the solstice, it predicts the Sun’s path through the sky will circle the observer over the course of a 24 hour day, going from north to west to south to east of the observer. (At the south pole itself, some of those directions are meaningless since every direction is north; but just move a millimeter from the pole and they mean something.)

They’ve been given the chance to go to Antarctica for free and now all of the sudden refuse to do it; they are even ostracizing the few among their number who have agreed to take the trip, accusing them of having sold out and being shills in advance of them coming back and reporting what they have seen,

That should be enough to tell any reasonable observer that they already know what the travelers to Antarctica will see…and it won’t be good for Flat Earth. Which is why I am not calling them ignorant or deluded; I am calling them liars. They know the Earth is not flat, yet they make a shitload of money claiming it is.

Lying. Sacks. Of. Shit.

However, I don’t call all of them liars. I give some praise to those few who are going; they apparently do actually believe it (which is not good on them)–negating the “liar” aspect–but more importantly they have the intellectual courage to test their beliefs, even in the face of ostracism from the knowing con-men on their side.

Beyond Neptune

Of course everyone knows what’s after Neptune.

Pluto.

But that’s not all of the story by any means.

The Discovery of Pluto

I told the story last time of the discovery of Neptune. But as astronomers observed and tracked Neptune in the last half of the 19th century, it appeared that Neptune didn’t account for all of Uranus’s unexpected motions.

The first thought, of course, is that there’s yet another planet out there. Percival Lowell decided to try to do something about it beyond thinking.

Percival Lowell had founded the Lowell observatory near Flagstaff, AZ in 1894, largely to observe Mars, but in 1906 he started searching for Planet Nine. He kept on looking with the help of William H. Pickering, using calculations by Elizabeth Williams. Nothing was found and Lowell passed away in 1916. (As it turns out his photographic plates did have “hits” on Pluto for March 19 and April 7th, 1915, but they were faint and didn’t get noticed. Planet Nine was expected to be big. There are fourteen other known instances of Pluto showing up, unrecognized, on observatories’ photographic plates from 1909 on; these are called “precovery” photographs.)

Percival Lowell’s widow, Constance, got into a ten year legal battle with the observatory, so the search stopped. But once the legal cloud had cleared, the director, Vesto Melvin Slipher (the first to see redshifts in galaxies) gave 23 year old Clyde Tombaugh the job of resuming the search. Tombaugh’s method consisted of taking photographs of the same area of the night sky a few days apart and putting the photographs (which were on glass plates) in a blink comparator, which would project one plate, then the other, and repeat. Any object that had moved in the meantime would seem to jump back and forth.

On February 18, 1930, Tombaugh spotted something on plates from the 23rd and 29th of January.

As you can see, the photographs were often not exposed to the same brightness, so anyone using a blink comparator would have to deal with the image getting brighter and dimmer, brighter and dimmer…while looking for the one object that was completely not there (not just dimmer) in one photograph or the other. (And it seems as though many things in the left photograph are not visible in the right hand photobraph. So perhaps Tombaugh simply looked for something that showed in the faint photo on the right, but not the brighter one on the left.)

A lower quality photo from the 21st helped confirm that Tombaugh wasn’t just seeing spots in front of his eyes. The observatory took more photos over the next few weeks to really nail the case down. Finally, on March 13, they telegraphed Harvard Observatory with the news.

The new planet orbits the Sun in 247.94 years, in an inclined and eccentric orbit. That period puts it into a 2:3 resonance with Neptune; it orbits twice in the amount of time it takes Neptune to orbit three times.

What to name it? They got thousands of suggestions, including Minerva, Pluto, and Cronus. Minerva had been used for an asteroid already, Cronus was being pushed by someone who was both unpopular and egocentric…so Pluto it was. (Cronus is also the Greek name for the titan who fathered Zeus and other Olympian gods…in other words it’s the Greek counterpart of the Roman Saturn.) Pluto/Hades was the god of the underworld. As a bonus, the first two letters are Percival Lowell’s initials. The name was approved by both the American Astronomical Society and the Royal Astonomical Society and the name became fixed on May 1. No jacking around with the name as had happened with Uranus for decades.

But right off the bat something didn’t add up.

One estimate from 1915 was that Planet Nine would have to be seven times as massive as the Earth. But a very early estimate after Pluto had been found, in 1931, had its mass as low as Earth’s (so, too low by a factor of 7). As more and more estimates were made over the years, Pluto’s estimated mass kept dropping; in 1948 Kuiper estimated it at 0.1 Earth masses, in 1976 it was lowered again to 0.01 Earth masses. But these were guesses based on Pluto’s size, which was estimated from how bright it was. It was never more than a dot of light on a photographic plate or film.

In 1978, we discovered Pluto had a moon, Charon…and with a moon we could determine the mass quite solidly, so the estimate dropped to 0.0015 Earth masses. And the latest number from 2006 is 0.00218 Earth masses. (I actually remember this happening. And now Pluto has five known moons.)

Charon, by the way, is the last of the medium-sized moons. Saturn has four, Uranus has four…and Pluto has one.

And we finally nailed down Pluto’s size, 2377 km in diameter. Our own moon is 3475 km across, and there are other moons larger than it. Mercury is also far larger than Pluto.

This is just way too tiny to be the planet we were looking for.

Furthermore, Voyager 2 in 1989 caused the estimates for Neptune’s mass to be dropped 0.5% and the “remaining discrepancy” in Uranus’s orbit now disappeared; Neptune accounted for it all.

So Pluto’s discovery was ultimately a stroke of luck. We were groping around in a dark room with a blindfold on, looking for a cat that wasn’t there…but we had found the mouse that was.

But now, just about everything about Pluto (and not just its size) made many wonder if it really should be considered a planet. Pluto is in a very un-planetery orbit. The other eight planets had reasonably circular orbits (Mercury being a bit of an outlier) all in nearly the same plane: the ecliptic (which is defined by the plane of Earth’s orbit). Pluto’s orbit is inclined 17 degrees to the ecliptic; no other planet came anywhere close to that. Furthermore, its orbit was very eccentric, not circular (e=.2488). In fact, with a semi-major axis of 39.482, that meant Pluto’s closest approach to the Sun was 29.658 AU.

That’s closer than Neptune. Pluto was actually at that point on September 5, 1989. For the entire twenty year period from 1979-1999 Pluto wasn’t the outermost planet, Neptune was.

[DIGRESSION: There is, by the way, little to no danger of a collision between Neptune and Pluto. If you look at the two orbits in 3D it becomes apparent that Pluto crosses the plane of Neptune’s orbit pretty far away from the actual orbit of Neptune. Here’s an animation of one Plutonian year from an oblique angle. The vertical white lines show how far below or above the plane Pluto is at any given time.

You can watch the animation and note that Neptune is at about 4 o’clock in the diagram at the start of the animation, and that’s where Pluto is furthest from the Sun. At the end of the animation, Neptune is at 10 o’clock; in other words it has orbited 1 1/2 times while Pluto orbited once (that’s a 3:2 resonance). At no point will the two planets come near each other, and since this pattern repeats, they won’t ever unless something causes an orbit to change.]

END OF DIGRESSION and back to the main thread: So Pluto didn’t look like any other planet. Nor did it act like any other planet. But if Pluto were all there was out there, most people would go ahead and consider it a planet.

But as it happens. there’s quite a lot “out there.”

The Centaurs

In 1977, Charles Kowal discovered Chiron, an asteroid, roughly 200 km across…but one with a difference. It was nowhere near the asteroid belt; it was well outside of it. That was a first, and barely a hint of things to come. Chiron is named after a centaur; and we would discover more such bodies. There’s a whole class of them now and that class is called the “centaurs.” It turned out there were “precovery” images of Chiron going clear back to 1895. And it turns out to have a ring!

There is a registry of so-called minor planets. When there is an initial observation, they’re given a “provisional designation.” (The scheme is a bit complicated: https://en.wikipedia.org/wiki/Provisional_designation_in_astronomy#Minor_planets but the first part is obviously the year of the first observation). Sometimes it gets an unofficial nickname, if it’s particularly interesting. Once we have enough data to establish an orbit, the object is given a number in the order they are discovered–and sometimes it gets a name too. (There are hundreds of thousands of objects that never got past the provisional designation stage.) Minor planets are simply numbered in order: Ceres is formally “1 Ceres”, then there is 2 Pallas, 3 Vesta, 4 Juno, and so on. It used to be just asteroids, but as we will see a lot more different kinds of things are on the list. These objects have the following in common: they orbit the sun directly, but aren’t planets, and aren’t comets.

[WARNING: Have a barf bucket handy for this one: Believe it or not there’s an object nicknamed (but not permanently named) “Biden,” provisional number 2012 VP113. And it got that name because Biden was the VP that year. However it’s been 12 years and they weren’t able to verify it so it might not be a real minor planet, in much the same way that Biden today isn’t a real president.]

When Chiron was first discovered, it got the provisional designation “1977 UB.” Once its orbit was established, it was regarded as the 2060th “minor planet” to be discovered, and now it’s formally known as 2060 Chiron. There are now over 44,000 known centaurs. And it’s speculated that Saturn’s way-out-there ninth moon, Phoebe, is a captured centaur. In general centaurs are far too likely to encounter one of the outer planets and so their orbits are not considered stable in the long term.

Buried in Planets?

Fifteen years later, things started to get crazy. We started finding more and more stuff way out there. The first was 15760 Albion (provisional designation 1992 QB1).

Here is 15760 Albion’s orbit (it’s a very slo-mo gif, so you’re not seeing things, it does move). It is in a roughly 291 year orbit. Shown in red are the orbits of Jupiter, Saturn, Uranus and Neptune.

It actually looks like a planet’s orbit; it’s even spaced about right. Unfortunately, it was only a bit over 100km across, not even remotely big enough to have forced itself into a round shape. Not a planet.

A concerted effort was made to scan the entire ecliptic for very slow moving dots of light, to see if there were other things out there.

And there sure were. Lots of small stuff. But then we started finding big ones too, ones big enough to be rounded, and many, if not most, of these objects have moons!

In 2002, we found 50000 Quaoar (named after a deity worshiped by an Indian tribe that lived in what is now the LA area), orbiting between 41.9 and 45.5 AUs, in 289 years. Its diameter is 1,090 km. OK, that’s sizeable enough to get one’s attention! And it has a moon.

Then we found 90377 Sedna, discovered in 2003, which has a gigantic 506 AU (that is not a typo, yes five hundred and six astronomical units) orbit (that is 76 billion kilometers). That’s the semi-major axis (half way across the long way). This one is a highly eccentric orbit, so it’s not that far away from us at the moment; if it was we’d never be able to see it. Right now Sedna is 83.5 AU away (still twice as far as Pluto), near its nearest approach to the Sun at 76 AU. Its furthest distance is 937 AU! But be prepared to wait a while for it to get there. Its year is 11,400 of ours, and you’ll have to wait about half that long for it to get halfway around its orbit. So far as we know, Sedna does not have a moon. We can see no detail at that ridiculous distance, but it is colored distinctly red (my guess: tholins). And Sedna is very roughly 900 km across, which is again sizeable, not dismissable as a piece of rubble. Sedna does not have a moon that we can see, which as you will see is unusual.

In 2004 we found 90482 Orcus, 900 km or so in diameter, 30.3 to 48.1 AUs out orbiting in 245.1 years (almost exactly the same as Pluto). Also, it has a moon.

OK, this is starting to get ridiculous. But we’re just getting started!

Also in 2004, there is 136108 Haumea, announced a year later and its status not fully settled even then because…well because it’s 2000km across! That’s getting close to Pluto’s size. (As a side note, Haumea is distinctly rugby-ball shaped. We think. Again we don’t see much more than blobs in our images.) And (wait for it), it has two moons.

But the absolute, oh-shit-we-have-a-problem-here discovery was announced the very next year, 2005, based on observations from late 2003 and later. 2003 UB313 was more massive than Pluto, though it appears to have a smaller diameter. The new object was “nicknamed” Xena (as in the Warrior Princess), and it took a while to settle on a permanent name. It turns out to have a moon, nicknamed Gabrielle after Xena’s sidekick. “Xena” orbits between 38.3 and 97.5 AUs, in 559 years. This object was actually announced by some YSM outlets as the tenth planet! Well, why not? If Pluto is a planet, this object certainly should be!

Because some people argued that indeed it was a planet, it took a while to get a permanent name and number. Why give it a number and have it turn out to not belong on the minor planet list? So “Xena” had to wait, for we were fully embroiled in discord.

And just for icing on the cake, on the same day that “Xena” was announced, the discovery of what would eventually be called 136472 Makemake was announced…and that was just two days after Haumea was announced. 136472 Makemake orbits between 38.1 and 52.8 AUs in 306 years.

Well. What a mess. Are they planets? We’d better figure this out because we’re getting buried here.

Rounding Up the Trans Neptunian Objects

I’m going to jump ahead here, a tiny bit. I’ll get back to the planet question soon.

I’m going to discuss the classification system we use today for these objects so (non-spoiler spoiler alert) Pluto will here be treated as one of these objects, not as a planet.

These objects all live beyond Neptune. But astronomers like to group things (you saw that with the moons of the gas and ice giants) and these objects, plus the zillions of much smaller ones in similar places that I haven’t mentioned, ultimately got “bucketed” into categories.

The Big Bucket is “trans-Neptunian object” Other than the centaurs, all of the objects I’ve discussed this time are trans-Neptunian objects (generally abbreviated “TNOs”), because they’re minor bodies outside of the orbit of Neptune.

But then we have sub-categories. The “Kuiper Belt” is those objects between 30 and 55 AUs from the Sun (as a reminder, Neptune is at roughly 30 AU). There are thousands of known Kuiper Belt objects, and the best estimate is that there are over a hundred thousand objects here over 100km in diameter. In fact there is far more “stuff” out there than in the asteroid belt. However, asteroid belt objects are typically rocks or metals, while the Kuiper Belt is mostly volatiles–iceballs, with some rocks in them.

The Kuiper Belt in turn has three classes of objects. The “classical” Kuiper Belt objects (cubewanos) are in reasonably circular, “regular” orbits, like Albion. There are a bunch in 2:3 resonance with Neptune (like Pluto), called plutinos, and others in a 1:2 resonance with Neptune, called twotinos. Orcus, Pluto, Haumea, Quaoar and Makemake are all Kuiper Belt objects. Orcus and Pluto are plutinos, the others are cubewanos.

This leaves Sedna and “Xena” unaccounted for. The other major category besides Kuiper Belt Objects is the “Scattered Disk Objects”, irregular-orbiting objects well beyond the Kuiper belt. “Xena” and Sedna fit here.

Here’s a handy-dandy chart. Or a confusing one, depending on your point of view, showing these categories, as well as the centaurs. In red across the top you will note designations like 2|3 and 1|2 for resonances with Neptune. And, oh by the way, Sedna is such an outlier it’s off the right hand edge of the diagram.

Gerard Peter Kuiper

Gerard Peter Kuiper, 1905-1973 (photo from 1964), was a Dutch-American astronomer. Americans trying to pronounce his name butcher it as “KAI-per,” rhyming with “piper.” The original Dutch pronunciation is indescribable to us except with the international phonetic alphabet: ˈɣɛrɪt ˈpitər ˈkœypər. He was the doctoral adviser for Carl Sagan, discovered Miranda (smallest moon of Uranus) and Nereid (third largest moon of Neptune), carbon dioxide in the atmosphere of Mars, and Titan’s atmosphere. He speculated that a large disk of of ices had condensed into smaller bodies, but would long since have been disrupted by Pluto (which was thought at the time to be massive). Well, he was half right; because Pluto is puny the objects are still there and the belt containing them is now named the Kuiper belt in his honor.

Discord

OK, back to “Are these planets?” The year is 2006. New Horizons launched on its mission to Pluto on 19 January of that year, and now it was time to evaluate the matter of whether it was on its way to a planet or not.

There was no formal definition of a planet. We knew them when we saw them. Except now we didn’t. Or rather everyone knew, but not the same as other people.

Alan Stern was (and still is) a principal investigator of the New Horizons probe (i.e., he is in charge of one of the instruments on that probe). Stern’s resume in the space program is as long as my arm. Time magazine even named him one of the 100 most influential people in 2007.

Stern was, and still is, an adamant defender of Pluto as a planet…and yes, he knows that means all these other objects, plus more to be discovered in the future, would be planets too.

His proposal: Divide planets into three subcategories. First, the classical planets, Mercury through Neptune, eight total. Then dwarf planets; that would include all of these big TNOs including Pluto, and Ceres, the largest object in the asteroid belt. The third category, though, is the “satellite planet.” These are the round moons orbiting other objects: our Moon, the four Galilean satellites of Jupiter, the seven round moons of Saturn, the five round moons of Uranus, Triton orbiting Neptune, and Charon orbiting Pluto.

These would all be planets, because they are massive enough for their gravity to have forced them into round shapes. (And this is one reason I’ve made a big deal about round versus not round.)

Including the moons seems a bit odd. But Stern’s position is very straightforward. He cares about the intrinsic properties of the object (it’s size and shape) first and its extrinsic circumstances, i.e. what orbit it’s in, second. If the object is round, it’s a planet, whether it dominates its orbit, or even if it orbits something else. Once it’s settled as a planet, then you decide whether it’s also a satellite, or big enough to “own” its orbit, and put it in the appropriate sub-buckets.

The IAU Makes Sausage

When the International Astronomical Union met in August of 2006 this matter was on the agenda and…well, we know the story. Alan Stern lost.

There is an aphorism that, like sausages, those that love law should not watch it being made. And that’s apparently true here as well.

The first proposal was: “A planet is a celestial body that (a) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and (b) is in orbit around a star, and is neither a star nor a satellite of a planet.”

In addition to the then-nine objects recognized as planets, this would have added Ceres, “Xena,” and Charon, the moon of Pluto. So we would immediately have twelve planets. In addition to this there were twelve candidate objects (including three asteroid-belt objects) that would likely fit once we knew more about them (including many of the ones I’ve talked about). Indeed there were claims (by Mike Brown who discovered Sedna and “Xena”) that we could have fifty three additional planets added almost immediately to this list of 12, and likely many more, perhaps 200, once we looked for more objects.

You may wonder why Charon would make the list, even though it’s fairly small as such things go. Why Charon and not Ganymede? That is because Charon and Pluto are close enough in size that the center of gravity of the Pluto-Charon system is actually outside of Pluto, unlike with every other moon in the solar system. That caused many to regard Pluto/Charon as a double planet…which of course would make Charon a planet.

Anything not spherical would be “bucketed” into Small Solar System Bodies (SSSBs). In addition, the “pluton” class (named for Pluto) would be used for things with highly eccentric or inclined objects. So this proposal drew one fairly clean line, if it’s round (and it’s not a star) it’s a planet, otherwise it’s an SSSB.

Although the relevant committee endorsed this, most of the IAU didn’t like this proposal; it was too ambiguous distinguishing between classical and dwarf planets. It failed a straw poll, 18-50 of a subgroup of the IAU.

So the second try, proposed by Gonzalo Tancredi and Julio Angel Fernandez:

(1) A planet is a celestial body that (a) is by far the largest object in its local population[1], (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape [2], and (c) does not produce energy by any nuclear fusion mechanism [3].

(2) According to point (1), the eight classical planets discovered before 1900, which move in nearly circular orbits close to the ecliptic plane, are the only planets of the Solar System. All the other objects in orbit around the Sun are smaller than Mercury. We recognize that there are objects that fulfill the criteria (b) and (c) but not criterion (a). Those objects are defined as “dwarf” planets. Ceres, as well as Pluto and several other large Trans-Neptunian objects, belongs to this category. In contrast to the planets, these objects typically have highly inclined orbits and/or large eccentricities.

(3) All the other natural objects orbiting the Sun that do not fulfill any of the previous criteria shall be referred to collectively as “Small Solar System Bodies“.[4]

Definitions and clarifications

  1. The local population is the collection of objects that cross or closely approach the orbit of the body in consideration.
  2. This generally applies to objects with sizes above several hundred kilometers, depending on the material strength.
  3. This criterion allows the distinction between gas giant planets and brown dwarfs or stars.
  4. This class currently includes most of the Solar System asteroids, Near-Earth objects (NEOs), Mars-, Jupiter- and Neptune-Trojan asteroids, most Centaurs, most Trans-Neptunian Objects (TNOs), and comets.[32]

This would have demoted Pluto to a “dwarf planet” which, despite the name including the word “planet,” was not a subcategory of planet; a difference between this and Stern’s proposal.

This went to open session, and the main point of contention was between the “static” and “dynamic” physics positions. The static position was similar to Stern’s; the emphasis would be on the intrinsic shape of the planet. “Dynamics” is a reference to the orbital properties.

There was one more draft, then the Plenary Session of the IAU met, and debated some more. And this is the result:

The IAU…resolves that planets and other bodies, except satellites, in the Solar System be defined into three distinct categories in the following way:

(1) A planet [1] is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and (c) has cleared the neighbourhood around its orbit.

(2) A “dwarf planet” is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape [2], (c) has not cleared the neighbourhood around its orbit, and (d) is not a satellite.

(3) All other objects [3], except satellites, orbiting the Sun shall be referred to collectively as “Small Solar System Bodies“.

Footnotes:

[1] The eight planets are: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune.
[2] An IAU process will be established to assign borderline objects into either dwarf planet and other categories.

[3] These currently include most of the Solar System asteroids, most Trans-Neptunian Objects (TNOs), comets, and other small bodies.

And just to be clear, a “dwarf planet” was not, despite the name, a category of planet; they passed an additional resolution to make it clear.

[I have seen clips of the actual vote, hands raised in the auditorium. I can’t find one now, or I’d include it.]

So the planets: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune.

The dwarf planets (a subgroup of the Small Solar System Bodies), most likely includes: Ceres, Pluto, Quaoar, Sedna, Orcus, Haumea, “Xena”, Makemake…and one other, Gonggong. This is a fuzzy line and there are others already known that arguably belong on this list.

The Aftermath

And so that was it for Planet Pluto. To put the nail in it, within days Pluto was given a minor planet number just like any asteroid or Kuiper Belt object: 134340 Pluto. It’s now marked as a “Small Solar System Body.”

The reaction was intense. The public of course hated this and still does.

But it’s not just the public. Many planetary scientists (not just Alan Stern) also disagree.

This issue will be revisited some day. Personally I like Stern’s suggestion better than what we got. Or perhaps the best suggestion is to just drop the word “planet” entirely since it seems to have emotional ties. Should every round object that’s not a star be a “world”?

This is NOT the first time we’ve reassessed the concept of a planet, by the way. The other times that I know of are:

  1. Any permanent wandering object in the sky was a planet; that included the Sun and the Moon, originally. Once it turned out the Moon orbited the Earth, and everything else orbited the Sun, that made the Sun “special” and the Moon a mere satellite of a planet, Earth.
  2. With the discovery of moons around other planets (the Galilean moons of Jupiter in 1610, but also the satellites of Saturn and Uranus), we started seeing the term “Planetary Satellites” (which Stern re-used) used for them; that term continued to be in use well into the 1700s if not later. It’s now often used for the big seven moons (the Moon, Io, Europa, Ganymede, Callisto, Titan and Triton); the ones I’ve been calling “large moons.”
  3. The asteroids were considered planets at first: Ceres, then we had Vesta, Juno and Pallas. They were all small and in the same general location, though so they quickly got reclassified as “minor planets” or even “asteroids.”

If you relish irony, after that flurry of discoveries in the mid 00s, only one more solid dwarf planet candidate has been discovered, and that in 2007: 225088 Gonggong, which varies from 33.8 to 101.2 AUs from the Sun, orbiting in 554 years, with a diameter of about 1230 km (give or take 50 km). It has one known moon.

…And Back to “Xena”

As for “Xena”, that same meeting settled its status, and the permanent name 136199 Eris was chosen. Eris’s moon was named Dysnomia. Eris is round. Dysnomia might be.

Eris was a Greek goddess, the personification of strife and discord. Dysnomia means “lawlessness” which (interestingly) might be a reference to Lucy Lawless, who played Xena.

What perfect names for the objects that triggered such a furor!

(Next time, we’ll look at the TNOs themselves, most especially Pluto [it’s by far the best known] in more detail.)

2024·11·16 Joe Biden Didn’t Win Daily Thread (And Neither Did Kamala Harris)

What is it that feeds our battle, yet starves our victory?

This post is scheduled to go “live” at 10:01PM MST on Friday, November 15, 2024. That’s 00:01 EST on Saturday, November 16, 2024 for those of you in that benighted timezone near the Atlantic Ocean.

As of that moment, there are 65 days, 11 hours, and 59 minutes until our rightful President of the United States is restored to office.

Not that I’m counting, mind you.

January 6 Tapes Reminder

After the first release, we were supposed to get more, every week.

As far as I know it hasn’t happened.

Speaker Johnson, please follow through!

A Caution

Just remember…we might replace the RINO candidates. (Or we might not. The record is mixed even though there is more MAGA than there used to be.) But that will make no difference in the long run if the party officials, basically the Rhonna McDaniels (or however that’s spelled–I suspect it’s RINO), don’t get replaced.

State party chairs, vice chairs, secretaries and so on, and the same at county levels, have huge influence on who ultimately gets nominated, and if these party wheelhorses are RINOs, they will work tirelessly to put their own pukey people on the ballot. In fact I’d not be surprised if some of our “MAGA” candidates are in fact, RINO plants, encouraged to run by the RINO party leadership when they realized that Lyn Cheney (and her ilk) were hopelessly compromised as effective candidates. The best way for them to deal with the opposition, of course, is to run it themselves.

Running good candidates is only HALF of the battle!

Biden Gives Us Too Much Credit

…we can move on to the next one.

Apparently Biden (or his puppeteer) has decided we’re to blame for all of the fail in the United States today.

Sorry to disappoint you Joe (or whoever), but you managed to do that all on your own; not only that, you wouldn’t let us NOT give you the chance because you insisted on cheating your way into power.

Yep, you-all are incompetent, and so proud of it you expect our applause for your sincerity. Fuck that!!

It wouldn’t be so bad, but you insist that everyone else have to share in your misery. Nope, can’t have anyone get out from under it. Somehow your grand vision only works if every single other person on earth is forced to go along. So much as ONE PERSON not going along is enough to make it all fail, apparently.

In engineering school we’re taught that a design that has seven to eight billion single points of failure…sucks.

Actually, we weren’t taught that. Because it would never have occurred to the professors to use such a ridiculous example.

Justice Must Be Done.

The prior election must be acknowledged as fraudulent, and steps must be taken to prosecute the fraudsters and restore integrity to the system.

Nothing else matters at this point. Talking about trying again in 2022 or 2024 is hopeless otherwise. Which is not to say one must never talk about this, but rather that one must account for this in ones planning; if fixing the fraud is not part of the plan, you have no plan.

Kamala Harris has a new nickname since she finally went west from DC to El Paso Texas: Westward Hoe.

Lawyer Appeasement Section

OK now for the fine print.

This is the WQTH Daily Thread. You know the drill. There’s no Poltical correctness, but civility is a requirement. There are Important Guidelines,  here, with an addendum on 20191110.

We have a new board – called The U Tree – where people can take each other to the woodshed without fear of censorship or moderation.

And remember Wheatie’s Rules:

1. No food fights
2. No running with scissors.
3. If you bring snacks, bring enough for everyone.
4. Zeroth rule of gun safety: Don’t let the government get your guns.
5. Rule one of gun safety: The gun is always loaded.
5a. If you actually want the gun to be loaded, like because you’re checking out a bump in the night, then it’s empty.
6. Rule two of gun safety: Never point the gun at anything you’re not willing to destroy.
7. Rule three: Keep your finger off the trigger until ready to fire.
8. Rule the fourth: Be sure of your target and what is behind it.

(Hmm a few extras seem to have crept in.)

Spot Prices

All prices are Kitco Ask, 3PM MT Friday (at that time the markets close for the weekend). (Note: most media quotes are for the bid…the price paid by the market makers, not the ask, which is what they will sell at. I figure the ask is more relevant to people like us who wish we could afford to buy these things. In the case of gold the difference is usually about a dollar, for the PGMs the spread is much wider.)

Last Week:

Gold $2,684.50
Silver $31.35
Platinum $979.00
Palladium $1,014.00
Rhodium $5,025.00
FRNSI* 128.863-
Gold:Silver 85.630-

This week, markets closed at 3PM Mountain Time Friday for the weekend.

Gold $2,563.30
Silver $30.30
Platinum $947.00
Palladium $974.00
Rhodium $4,950.00
FRNSI* 123.000-
Gold:Silver 84.597+

There’s no sugar coating it…the precious metals except for platinum are taking a beating. (Platinum was already on sale anyway.) Silver at least didn’t take quite as much of a beating as gold. The FRNSI, when I calculated it, turned out to be 122.9996 which rounds up to 123.000, which is why it looks suspiciously “round” at the moment. (Like the time twenty years or so ago when I bought a bunch of random things, and the total at the cash register, including sales tax, was exactly $100.00. I told the cashier to get the machine checked.)

*The SteveInCO Federal Reserve Note Suckage Index (FRNSI) is a measure of how much the dollar has inflated. It’s the ratio of the current price of gold, to the number of dollars an ounce of fine gold made up when the dollar was defined as 25.8 grains of 0.900 gold. That worked out to an ounce being $20.67+71/387 of a cent. (Note gold wasn’t worth this much back then, thus much gold was $20.67 71/387ths. It’s a subtle distinction. One ounce of gold wasn’t worth $20.67 back then, it was $20.67.) Once this ratio is computed, 1 is subtracted from it so that the number is zero when the dollar is at its proper value, indicating zero suckage.

Neptune

We now reach the last full planet. But is it the end of the road?

History

Neptune’s discovery was a triumph of Newtonian theory.

Newton in the mid-late 1600s was pondering the forces that make the planets move, as opposed to forces we see on Earth. Apparently he saw an apple fall (it did not bonk him on the noggin), and it occurred to him that the force that made the apple fall might be the same force that makes the Moon orbit the Earth. Newton knew how far away the Moon was, he knew how much it would have to accelerate to remain in its orbit about the Earth. (If there was no acceleration, it would just go in a straight line and eventually disappear from sight from becoming too faint to see.) He also knew how far he and the apple were from the center of the Earth, and already knew how fast the apple accelerated.

He was able to determine that if the acceleration induced by gravity dropped off as the square of the distance, the number for the Moon’s distance actually matched what the Moon was doing.

Twenty years later after a lot of refining and elaboration, well…For the first time we knew that the stuff “up there” follows the same rules as the stuff “down here.” It’s not a special realm, as the ancients believed.

Newton did not discover gravity. Gravity was known to Og the caveman especially after he did a faceplant tripping over something while chasing game, nor was Og the first to notice it. What Newton did do was to show that gravity is universal, it applies everywhere not just here on Earth. And he was able to write equations that described it quite accurately.

Newton, during those 20 years, had gone on to prove that such a force would cause things to orbit other things in ellipses…which matched what we already knew; Johannes Kepler had in the early 1600s proved with meticulously collected data spanning decades and years of his own skull sweat that the orbits of the planets around the Sun (and the Moon around the Earth) were ellipses. Newton also was able to show that Kepler’s other two laws of planetary motion applied. Better, one could apply his laws to the Galilean moons (as well as Titan orbiting Saturn) and show that they, too followed Newtonian mechanics and gravity.

Over the next decades astronomers refined their data on the planets and had more and more accurate data to “plug into” their equations and predicting where planets and the Moon would be became an exact science; instead of being off by five degrees (the width of you three big fingers (not the thumb and not the pinky) held at arms length), we were much less than half a degree.

Then Uranus was discovered in 1781, and that was one more thing to track on top of the other planets, known moons of planets, and so on. (Starting in 1650, we discovered binary stars orbiting each other and could track them too.) Alexis Bouvard published tables of Uranus’s ephemerides (predictions of future predctions) in 1821.

Except there was a problem, one which became apparent over the next few decades (it takes a long time, when the planet has an 84 year orbital period or “year”). Uranus was being an ass…not behaving. It was traveling too fast for a while…then too slow.

Was Newton wrong after all? In spite of his stuff having worked so well for over a century?

Bouvard didn’t think so. He speculated that some unknown body was perturbing Uranus’s orbit, pulling on it and either making it speed up or slow down, depending on where it was in relation to Uranus. In 1843 John Couch Adams began trying to figure out where this unknown body was, and by 1845-6 had generated several predictions; he was continually refining them because his method was iterative. He’d guess, run the numbers, adjust his guess, and repeat. Then repeat again.

But Adams had competition; Urbain Le Verrier was also working on the problem. He came up with similar answers. The Astronomer Royal of England, Sir George Airy, persuaded James Challis to actually look through a telescope and try to find the planet. Challis tried through August and September 1846, and failed. (However he realized much later that he had actually seen it a couple of times in July and August 1845 (a year before his search) and not recognized it for what it was, because he had poor observing techniques and old star charts. D’oh!)

Le Verrier wasn’t going to wait on the Brits to get their act together; he wrote to Johan Gottfried Galle in Berlin, and asked him to look. Galle received the lettter on the 23rd of September, 1846. Heinrich d’Arrest, a student at the observatory, pointed out that they had just made a chart of that part of the sky recently. So all Galle had to do was point his telescope and look for something that wasn’t on the chart. That would be a moving object…a planet. Galle looked that evening with a nine inch refractor telescope (one with lenses at both ends of the tube), and found it almost immediately, less than a degree away from where Le Verrier had said it would be, and twelve degrees away from Adam’s prediction. However…the old chart could just be missing the object by mistake. Galle looked at the object over the next few days and satisfied himself that it wasn’t a mistake. It was indeed a moving object.

Another planet had been found!

Newton in trouble? No way! This was actually a triumph for Newtonian mechanics because it had been used to find a planet!

(As a footnote…Galileo saw Neptune, diagrammed its position in his notes, not once but twice when it was near Jupiter on 28 December 1612 and 27 January 1613 [both dates New Style] but didn’t realize it was a moving object. So, although interesting, it isn’t enough to give him credit for the discovery. However, “In 2009, a study suggested that Galileo was at least aware that the “star” he had observed had moved relative to fixed stars.” [From Wikipedia])

Voyager 2, 25 August 1989

This is a collection of official NASA animations depicting the sole spacecraft encounter (so far) with Neptune. These videos were made before the encounter, so Neptune’s and Triton’s appearances are just guesses. They also show the rings as arcs, because that’s what they thought back then (it turns out that they’re full rings, with some thicker sections we mistook for partial arcs).

Basic Info

For a while, it was simply called “the planet exterior to Uranus” or “Le Verrier’s Planet”. Galle suggested calling it Janus, which fortunately didn’t happen or it would be confused with the Hugh Janus of the solar system. Le Verrier said, since he had discovered it, he should be able to name it and he suggested “Neptune.” And that’s the name that ultimately “stuck.” The planet had a bluish tinge and Neptune was the Roman god of the sea (corresponding to the Greek Poseidon).

Neptune orbits the Sun in 164.8 years, almost twice as long as Uranus (84.02 years). Its average distance from the sun is 30.07 AUs (30.07 times as much as Earth’s average disance). That puts it at 4.5 billion kilometers from the Sun. That means that radio signals to and from Voyager 2 took over four hours each way!

Here it is in true color, with the Earth photoshopped in for comparison.

It’s roughly the same size as Uranus…just a bit smaller, but it is considerably denser than Uranus and notably more massive (Uranus is 14.536 times the mass of the Earth, Neptune is 17.147 times.)

Neptune rotates in 16 hours, 6 minutes; that’s its day. Its axis is tilted 28.2 degrees, a bit more than Earth’s but not ridiculous like with Uranus or Venus. The temperature is 55-72 Kelvins (-218 to -201 C) depending on how deep into the atmosphere you measure it. The latter number is measured where the atmospheric pressure is the same as Earth’s at sea level. The atmosphere consists of 80 percent hydrogen, 19 percent helium and 1.5 percent methane by volume, with traces of ethane, ammonia, water ice, and ammonium hydrosulfide. The methane gives Neptune its bluish tinge.

Innards

Deeper down the methane, ammonia and water ices become more prevalent, earning Neptune its place among the ice giants. One thing I just spotted is the speculation that at a depth of 7000km, methane might decompose with the carbon forming diamond crystals that rain downwards like hailstones; this would be true on Jupiter, Saturn and Uranus as well.

Whoops, spoiler…Rings.

You’re probably used to seeing this picture of Neptune:

But if you scroll back to the earlier picture, it’s the same picture of Neptune, just rendered in different colors. This one exaggerated the colors for contrast, and in it you can see the “Great Dark Spot” which means I can now segue to discussing the weather.

Weather

The “Great Dark Spot” is similar to Jupiter’s Great Red Spot. It’s 13,000km x 6,600 km or so…which means that measured the long way it’s slightly broader than Earth! However, it wasn’t nearly as permanent as the Red Spot. By the time Hubble looked at Neptune eight years later in 1994, it was gone. But a new dark spot had appeared in Neptune’s northern hemisphere.

The white smudge is called “Scooter” because it moved more rapidly than the Great Dark Spot

Neptune has the most extreme winds in the solar system…at least, as far as we can tell. The prevailing winds on the equator are 400 m/s, dropping to a “mere” 250 m/s at the poles. In the storms the velocity can reach 600 m/s. That’s roughly 2,200 kph or 1,300 mph, well over the speed of sound. This is a stark contrast to Uranus, which had no obvious storms when Voyager 2 flew by. The concentration of methane, ethane, and acetylene at the equator is 100 times that at the poles, so it seems that at the equator the atmosphere is upwelling, bringing that stuff from down deeper where it is more common. It subsides near the poles.

Neptune, like Uranus, has a multi pole magnetic field, indicating its dynamo is probably in a relatively thin layer of the planet–much as is thought with Uranus.

Rings

Neptune has rings, but not very substantial ones. In this case it’s likely to be tiny ice particles coated with carbon-based material. And here, we came up with cool names: the most important rings are named Adams, Le Verrier, and Galle. The best way to view them is in infrared..and well guess what we just put up there that sees really, really well in infrared?

None other than the James Webb Space Telescope, of course!

Before the Voyager 2 encounter, we thought the rings were partial arcs rather than full circles; we eventually figured out those arcs were actually thicker parts of full rings.

And what a nice segue into the moons, since we can see some of them here.

Moons

You might expect the same progression of small, inner moons, nice and regular in circular orbits, then major moons (either large and planetary sized, or medium or medium-small but still round, or a mix), also in nice tidy regular orbits, then irregular satellites, that we saw with Jupiter, Saturn, and Uranus. Surely with a pattern like this three times running, we can expect more of the same here?

You might expect it, but that ain’t what you’re gonna get!

Neptune has 16 known moons, with a naming theme of water deities and one water critter out of Greek mythology.

First we have seven small regular satellites…in other words, inner moons. Some of them orbit among Neptune’s rings, as seen in the JWST photo above. Five of them were discovered by Voyager 2 in 1989, and of course the best photos we have of any of them are from that spacecraft, the only one ever to visit Neptune. Larissa was actually discovered in 1981, while Hippocamp was first spotted in 2013.

The largest of these is Proteus, with a diameter of 420 km. That puts it in the same size range as Mimas and Miranda, those smallest round moons, but it’s not round! It’s more like Hyperion in that regard, but unlike Hyperion, it’s not a gigantic sponge.

A craptastic picture like this is the best we can do when only Voyager 2 ever got close to it.
Proteus, 420 km or so in diameter, orbiting at 117,646 km in 1.12 (Earth) days.

It is remarkable Proteus was discovered well after Larissa (which is much smaller) and Nereid, which is also smaller and has been known for decades–we’ll get to that.

So far so good, right? Inner moons.

Next should be large, planetary-sized moons and/or medium moons, all nice and regular.

Well, we do get a large moon. But it’s not regular. Not even close!

Triton is 2,705 km (give or take about 5 km) orbiting at 352,759 km in 5.87 days. It’s in a nice circular equatorial orbit…but it’s not in Neptune’s equatorial plane; it’s inclined at 23 degrees. Well, no, actually, it’s inclined at 157 degrees. Yes, it’s retrograde.

Triton’s orbit in red, compared to a “normal” moon’s orbit in green. Note the opposite directions of motion.

What the Biden is going on here? We’ll come back to that. And we’ll hit Triton in more detail shortly. Meanwhile, I’ll point out that it was discovered weeks after Neptune itself, by the English astronomer William Lassell.

A black and white picture of Triton–it’s actually a mosaic pieced together from smaller pictures.
Triton looks a lot like a cantaloupe in places.

Next out is Nereid, discovered in 1949 by Gerard Peter Kuiper (you may recall I warned you that you’d be seeing his name again! And I wasn’t thinking about this when I said so). Nereid is 357 km across (give or take 13 km), and another non-round, but medium small moon. And now we see the suckage we have to deal with when only one spacecraft has ever spent any time at all near Neptune, and that only a few hours. Here is our absolute best picture of Nereid (out of 83 that Voyager took):

Nereid is another one of those “medium small” moons that didn’t quite become rounded. It got discovered before Proteus (which is larger) because it has a high albedo, reflecting most of the light that hit it.

And Nereid’s orbit is wacky. Its average distance from Neptune is 5,513,900 km–a huge jump up from Triton (it takes 360 days to orbit Neptune). But it’s at a relatively sane inclination of 5 degrees…very small for an irregular moon. But here’s the big surprise: the eccentricity is a whopping 0.75! That’s extremely elliptical. Its closest approach to Neptune is 1,381,500 km and its furthest distance is 9,626,500 km.

Next out is Halimede, about 62 km across, at 16,590,500 km, orbiting in 1879 days (almost five years), it’s retrograde and has an eccentricity of 0.521. It looks like it’s made out of the same stuff as Nereid, and there’s a 41 percent chance that at sometime in the past, it actually collided with Nereid. Or rather, that it broke off of Nereid (when you “run that tape backwards” that looks like a collision).

There are then two groups of three, the Sao group (inclined 36-50 degrees) and the Neso group (inclined 127-135 degrees), all of them 25-60km in diameter.

Halimede on out are clearly outer, irregular moons so here at least the usual pattern fits.

OK, we’ve got some crazy stuff going on here.

Triton

There are seven “large” or “planetary sized” moons in our Solar System (the Moon, Io, Europa, Ganymede, Callisto, Titan and Triton) and Triton is the smallest of them. It’s the only moon in the Solar System with a diameter in the 2,000-3,000 km range. Even so, it’s larger than all of the smaller moons in the Solar System, put together.

Before Voyager 2 flew by, we knew very little about Triton; Kuiper tried to measure its diameter in 1954 (well over a century after its discovery) and got 3,800 km. Others got values anywhere from 2500 to 6000km; that last is almost half the diameter of Earth and would have made Triton the largest moon in the solar system, beating out even Ganymede. The answer turned out to be 2706 km as measured by Voyager 2 on August 25, 1989.

Triton has a density of about 2 grams per cubic centimeter, which indicates that unlike many moons of the outer solar system, it’s more rock than ice. Its surface temperature is 38 K (-235C), slightly colder than Hitlary Klinton’s lap.

In the 1990s an atmosphere was detected (by watching stars fade as Triton passed in front of them). This is a very thin atmosphere, 0.02 millibar at most (Earth’s atmosphere is close to 1013 millibars). Nonetheless, clouds were photographed by Voyager (look at the horizon)

And also in this picture, a “parting shot” at Triton from the opposite side from the Sun (backlit pictures like this one can be very useful when studying atmospheres):

Triton also has geysers, this time of nitrogen. Triton is cold enough to have nitrogen ice on it (and remember that liquid nitrogen is stereotypically very cold stuff), but below the surface it’s warmer and you can have nitrogen geysers. The black smudges are thought to be downwind of them.

And finally we have this picture of the south polar ice cap (yes, “upside down” with south at the top):

Away from the cap we see more cantaloupe terrain. This feature is unique to Triton, so far as we know, and consists mostly of dirty water ice. They might be caused by lumps of less-dense material slowly rising to the surface, or perhaps flooding from cryovulcanism.

What’s with the red color? We’ve seen this a lot and it’s time I discussed it a bit. All of these outer moons have some amount of hydrocarbons on them (especially Titan), things like methane, ethane, and so forth. There’s zero protection from ultraviolet light on any of these moons (except maybe Titan), so the UV acts on the hydrocarbons and any sulfur that’s around and produces tholins, which are pretty much random goo formed of polymers. The term tholin was coined by Carl Sagan, who wrote:

For the past decade we have been producing in our laboratory a variety of complex organic solids from mixtures of the cosmically abundant gases CH4, C2H6, NH3, H2O, HCHO, and H2S [methane, ethane, ammonia, water, formaldehyde and hydrogen sulfide, respectively–SteveInCO]. The product, synthesized by ultraviolet (UV) light or spark discharge, is a brown, sometimes sticky, residue, which has been called, because of its resistance to conventional analytical chemistry, “intractable polymer”. […] We propose, as a model-free descriptive term, ‘tholins’ (Greek Θολός, muddy; but also Θόλος, vault or dome), although we were tempted by the phrase ‘star-tar’.[3][1]

We’ve only seen 40 percent of Triton, because that’s what Voyager photographed as it sped by. The other side might very well be a gigantic billboard reading “For a Good Time Call…” with Kamala Harris’s phone number, for all we know.

Here’s a geological map of Triton, based on what we have seen.

Triton orbits closer to Neptune than the Moon does to Earth, yet it is highly inclined and retrograde. Its orbit is nearly circular, and it has become tidally locked to Neptune (as would be expected).

Earth’s moon is slowly receding from Earth at a few centimeters per year. Triton is getting closer. In fact, in about three and a half billion years, it will probably get close enough to Neptune that tidal forces will pull it apart and we’ll have an absolutely killer set of rings to admire. (Book your travel plans now!)

But why is it getting closer to Neptune, when our Moon is getting further from Earth? Let’s look at why our Moon is getting further from Earth. It’s both raising and pulling at our tidal bulges, and our tidal bulges are pulling on the moon. The bulges precede the moon (because the rotation of the Earth shoves them ahead of where they “should” be directly under the Moon), which means the moon is pulling back on them and slowing the rotation of the Earth (which is why we keep having to add leap seconds). Conversely the bulges pull the Moon forward and cause it to speed up in its orbit. Speeding up raises the orbit. The Moon slowly recedes.

The same thing happens with Neptune and Triton…except that now the tidal bulges try to pull Triton “forward” in its orbit…but Triton is moving backward in its orbit, so pulling it forward actually cancels part of the backwards motion and slows Triton down. So, slowly but surely Triton’s orbit gets smaller and smaller.

OK So What Happened That Left This Trainwreck?

Neptune’s moon system is radically different from the others. There’s simply no way Triton could have formed where it did.

Astronomers are fairly certain that Triton is actually a captured object. And when it was captured, it wreaked havoc with the rest of Neptune’s moon system. Nereid, for instance is either also a captured object, or got put into its oddball orbit by Triton during the capture–if so it’s probably the only original Neptunian regular moon that survived, though it’s not regular any more. Any other moon that Neptune had at the time is long gone.

Adding to the pile of evidence for Triton being captured: it turns out to have a very similar chemical composition to Pluto, suggesting that they formed near each other.

Another Visit?

Will we ever visit Neptune again? Obviously the next step is an orbiter. Multiple concepts, both orbiters and more flybys, have been proposed and rejected. There’s some thought of doing things under the New Frontiers program, perhaps orbiters that would spend a lot of time on Triton, but these would be launching in 2031 or 2041 and arriving in 2047 and 2056 (note the fifteen or sixteen year travel times!). I’ll be a geezer by 2056; older than my parents lived. Failing that, the Chinese might put something at Neptune by 2058. So it looks like, not in my lifetime.

Neptune, the Mystic

Gustav Holst (1874-1934) composed an orchestral suite called The Planets in 1914-1917, with movements for Mars, Venus, Mercury, Jupiter, Saturn, Uranus and Neptune. (It’s one of the few “classical” works from the 20th century that I like.) Although he tried to evoke the mythological figures the planets are named after, I find the Neptune movement evocative of the vast distance that Neptune is, and its extreme isolation.

The slow fading out makes one think of journeying off into the stupendous void that is beyond Neptune.

The sun is 30 times further away from Neptune than it is from Earth. It’s half a degree across as seen from earth (30 minutes of arc), which means it’s one minute of arc across at Neptune. It looks the size of a quarter at 100 yards. No wonder it gives such little warmth, 1/900th of what it gives to us. And also the same tiny fraction of light. Cold and Dark, and it’s hard to imagine it getting colder and darker. Surely we are at the corner of “no” and “where.”

And yet, though we are out of planets, we are not done.

2024·11·09 Joe Biden Didn’t Win (And Neither Did Kamala Harris) Daily Thread

What is it that feeds our battle, yet starves our victory?

OK Let’s Have Some Fun

Let’s nominate people from this site for positions in the 47 administration!

E.g., Scott for Press Secretary (assuming they don’t go with Kayleigh again). Imagine the YSM Jurinalists getting the Scott treatment!

Our Turn

We’ve often seen that quote from David Plouffe: “It is not enough to simply beat Trump. He must be destroyed thoroughly. His kind must not rise again.”

This was of course a declaration of intent to annihilate not just Trump, but rather “his kind.”

You know what? I think we should flip it around. David Plouffe’s kind should be destroyed thoroughly and their kind must not rise again.

What is Plouffe’s kind? I suppose it depends on who’s talking and what they are thinking of in particular. Well, at the moment it’s me talking and I am thinking of the sort of maggot who is attracted to politics not to better his world but rather so that he can wield power over others, or line their pockets with “free” money. Often these people end up as what Ayn Rand called “pull peddlers,” receiving money in exchange for using their connections to do favors.

This type is parasitic. Utterly parasitic. And they should be destroyed thoroughly and not allowed to rise again.

The bad news is we will never eradicate them. Useless turds who can’t do anything productive will always be with us. As will the outright sociopaths.

Of course they find Trump to be their enemy. And of course they find us to be their enemy. If we won’t simply lie down and let our “betters” have their way with us, we’re a problem, we’re something to be got rid of. And of late, we haven’t lain down without a protest, as we are “supposed” to do. Dang uppity Garbage Deplorables! We don’t know our place!!!

The good news is we can provide far fewer niches for these parasites. The niches come into being when something that people formerly did of their own free will is taken over by the government; then every aspect of that activity becomes a political football.

Take for instance education. Since the government runs it, if you don’t like what’s being done, you have to form a political movement and try to work your way around the maggots embedded in the bureaucracy. If education were private, then if you didn’t like what they were doing to your child, you’d take your money and your child elsewhere. And people who didn’t even have school-age children presently would have no voice–and not have to pay money. Making it a government “thing” turned it into a political thing, and the maggots began to swarm.

So we wreck them by seriously cutting government and giving them fewer places to exist. Among all of the other benefits, the body politic would have fewer sociopaths and parasites in it.

People like Plouffe are the same type, but they are the full-on political hacks who set policy, rather than implement it. They’re just as bad if not worse; they help government grow, and steer it into serving its own ends, rather than those of the people it is supposed to be serving.

The Deep State is nothing more than a government that serves its own ends.

And we have had enough of this.

They must be destroyed thoroughly, and their kind must not rise again.

This election wasn’t the end, it was the beginning. There are millions of these malignancies in this country and we’ve just defeated two of them. Keep pushing. Now we can go after them wholesale.

It’s our turn.

Our turn.

Our turn.

OUR TURN!

You stole the 2020 election. You’ve mocked and ridiculed and put people in prison and broken people’s lives because you said this thing was stolen. This entire phony thing is getting swept out. Biden’s getting swept out. Kamala Harris is getting swept out. MSNBC is getting swept out. The Justice Department is getting swept out. The FBI is getting swept out. You people suck, okay?! And now you’re going to pay the price for trying to destroy this country.

And I’m going to tell you, we’re going to get to the bottom of where the 600,000 votes [are]. You manufactured them to steal this election from President Trump in 2020. And think what this country would be if we hadn’t gone through the last four years of your madness, okay? You don’t deserve any respect, you don’t deserve any empathy, and you don’t deserve any pity.

And if anybody gives it to you, it’s Donald J. Trump, because he’s got a big heart and he’s a good man. A good man that you’re still gonna try to put in prison on the 26th of this month. This is how much you people suck. Okay? You’ve destroyed his business thing. And he came back.

He came back in the greatest show of political courage, I think, in world history. Like, [Roman statesman] Cincinnatus coming back from the plough [returning to politics to rescue the Roman Republic]. He’s the American Cincinnatus. And what he has done is a profile in courage. We’ve had his back. But I got to tell you, he may be empathetic. He may have a kind heart. He may be a good man. But we’re not. Okay? And you deserve, as Natalie Winters says, not retribution, justice. But you deserve what we call rough Roman justice, and we’re prepared to give it to you.

Steve Bannon, on election night

OUR TURN!!

OUR TURN!!!

January 6 Tapes?

Paging Speaker Johnson…this is your conscience calling you out on broken promises.

For all your high talk about your Christian moral background…you’re looking less and less like you have any kind of moral background.

If You are a Patriot and Don’t Loathe RINOs…

Let’s talk about RINOs, and why they are the lowest form of life in politics.

Many patriots have been involved with politics, often at the grassroots, for decades. We’ve fought, and fought, and fought and won the occasional illusory small victory.

Yet we can’t seem to win the war, even when we have BIG electoral wins.

I am reminded of something. The original Star Trek had an episode titled Day of the Dove. It was one of the better episodes from the third season, but any fan of the original series will tell you that’s a very low bar. Still, it seems to get some respect; at a time when there were about 700 episodes of Star Trek in its various incarnations out there, it was voted 99th best out of the top 100.

In sum, the plot is that an alien entity has arranged for 39 Enterprise crew, and 39 Klingons, to fight each other endlessly with swords and other muscle-powered weapons. The entity lives off of hostile emotions, you see and it wants a captive food source. (The other 400 or so Enterprise crew are trapped below decks and unable to help.) Each side has its emotions played and amplified by the alien entity; one Enterprise junior officer has false memories implanted of a brother who was killed by Klingons. The brother didn’t even exist.

Even people killed in a sword fight miraculously heal so they can go do it again.

The second best line of the episode is when Kang, the Klingon captain, notes that though they have won quite a number of small victories including capturing Engineering, can’t seem to actually finally defeat the Enterprise crew. He growls, “What power is it that feeds our battle yet starves our victory?*”

Indeed. He may have been the bad guy, but his situation should sound familiar.

We are a majority in this country. We have a powerful political party in our corner. There is endless wrangling.

And yet,

What power is it that feeds our battle yet starves our victory?

In our case, that power is the RINOs in our midst. They specialize in caving when on the verge of victory. Think of Obamacare’s repeal failing…by one Republican vote. Think of the way we can never seem to get spending under control (and now our entire tax revenue goes to pay interest on the debt; anything the government actually does now is with borrowed money).

We have a party…that refuses to do what we want it to do, and that refusal is institutionalized. If you’ve been involved with GOP politics, but haven’t seen this, it’s because you refuse to see it. Or because you are part of the problem yourself. (If so, kindly gargle some red fuming nitric acid to clear the taste of shit out of your mouth, and let those not part of the problem alone so they can read this.)

We fight to elect people, who then take a dive when in office. But it’s not just the politicians in office, it’s the people behind the scenes, the leaders of the national, state and county branches of the party. Their job is to ensure that real patriots never get onto the general election ballot. They’re allowed a few failures…who can then become token conservatives who will somehow never manage to win (Jordan), or can be compromised outright (Lauren Boebert?).

That way it doesn’t actually matter who has a congressional majority. I remember my excitement when the GOP took the Senate in 1980. But all that did was empower a bunch of “moderate” puddles of dog vomit like…well for whatever reason forty years later the most memorable name is Pete Domenici. And a couple of dozen other “moderates” who simply had no interest in doing what grassroots people in their party–those same grassroots people who had worked so hard to elect them–wanted them to do.

Oh, they’ll put up a semblance of a fight…but never win. And they love it when we fight the Dems instead of fighting them. Just like that alien entity, whose motto surely was “Let’s you and him fight. It’ll be delicious!”

If you think about it, your entire political involvement has come to nothing because of these walking malignant tumors.

That should make you good and mad.

The twenty five who blocked Jordan, and the hundred people who took that opportunity to stab Jordan in the back in the secret ballot should make you good and mad.

I’ll close this with another example of RINO backstabbing, an infuriating one close to home.

In my county, the GOP chair is not a RINO. She got elected when the grassroots had had enough of the RINOs. Unfortunately the state organization is full of RINOs, and the ousted county RINOs have been trying to form a new “Republican Party” and get the state GOP to recognize them as the affiliate. I’m honestly amazed it hasn’t happened yet.

In other words those shitstains won’t just leave when they get booted out; they’ll try to destroy what they left behind. It’s an indication that they know we know how important that behind-the-scenes party power is.

So they must be destroyed. That’s the only way they’ll ever stop.

We cannot win until the leeches “on our side” get destroyed.

What power is it that feeds our battle yet starves our victory?*

We know it. What is going to be done about it?

*NOTE: The original line was actually “What power is it that supports our battle yet starves our victory.” I had mis-remembered it as feeds. When I checked it, it sure enough was “supports” and that’s what I originally quoted. On further reflection, though, I realized my memory was actually an improvement over the reality, because feeds is a perfect contrast with starves. I changed it partway through the day this originally posted, but now (since this is a re-run) it gets rendered this way from the start.

If one must do things wrong, one should do them wrong…right.

RINOs an Endangered Species?
If Only!

According to Wikipoo, et. al., the Northern White Rhinoceros (Ceratotherium simum cottoni) is a critically endangered species. Apparently two females live on a wildlife preserve in Sudan, and no males are known to be alive. So basically, this species is dead as soon as the females die of old age. Presently they are watched over by armed guards 24/7.

Biologists have been trying to cross them with the other subspecies, Southern White Rhinoceroses (Rhinoceri?) without success; and some genetic analyses suggest that perhaps they aren’t two subspecies at all, but two distinct species, which would make the whole project a lot more difficult.

I should hope if the American RINO (Parasitus rectum pseudoconservativum) is ever this endangered, there will be heroic efforts not to save the species, but rather to push the remainder off a cliff. Onto punji sticks. With feces smeared on them. Failing that a good bath in red fuming nitric acid will do.

But I’m not done ranting about RINOs.

The RINOs (if they are capable of any introspection whatsoever) probably wonder why they constantly have to deal with “populist” eruptions like the Trump-led MAGA movement. That would be because the so-called populists stand for absolutely nothing except for going along to get along. That allows the Left to drive the culture and politics.

Given the results of our most recent elections, the Left will now push harder, and the RINOs will now turn even squishier than they were before.

I well remember 1989-1990 in my state when the RINO establishment started preaching the message that a conservative simply couldn’t win in Colorado. Never mind the fact that Reagan had won the state TWICE (in 1984 bringing in a veto-proof state house and senate with him) and GHWB had won after (falsely!) assuring everyone that a vote for him was a vote for Reagan’s third term.

This is how the RINOs function. They push, push, push the line that only a “moderate” can get elected. Stomp them when they pull that shit. Tell everyone in ear shot that that’s exactly what the Left wants you to think, and oh-by-the-way-Mister-RINO if you’re in this party selling the same message as the Left…well, whythefuckexactly are you in this party, you lying piece of rancid weasel shit?

Justice

It says “Justice” on the picture.

And I’m sure someone will post the standard joke about what the fish thinks about the situation.

But what is it?

Here’s a take, from a different context: It’s about how you do justice, not the justice that must be done to our massively corrupt government and media. You must properly identify the nature of a person, before you can do him justice.

Ayn Rand, On Justice (speaking through her character John Galt, in Atlas Shrugged):

Justice is the recognition of the fact that you cannot fake the character of men as you cannot fake the character of nature, that you must judge all men as conscientiously as you judge inanimate objects, with the same respect for truth, with the same incorruptible vision, by as pure and as rational a process of identification—that every man must be judged for what he is and treated accordingly, that just as you do not pay a higher price for a rusty chunk of scrap than for a piece of shining metal, so you do not value a rotter above a hero—that your moral appraisal is the coin paying men for their virtues or vices, and this payment demands of you as scrupulous an honor as you bring to financial transactions—that to withhold your contempt from men’s vices is an act of moral counterfeiting, and to withhold your admiration from their virtues is an act of moral embezzlement—that to place any other concern higher than justice is to devaluate your moral currency and defraud the good in favor of the evil, since only the good can lose by a default of justice and only the evil can profit—and that the bottom of the pit at the end of that road, the act of moral bankruptcy, is to punish men for their virtues and reward them for their vices, that that is the collapse to full depravity, the Black Mass of the worship of death, the dedication of your consciousness to the destruction of existence.

Ayn Rand identified seven virtues, chief among them rationality. The other six, including justice, she considered subsidiary because they are essentially different aspects and applications of rationality.

—Ayn Rand Lexicon (aynrandlexicon.com)

Justice Must Be Done.

Trump, it is supposed, had some documents.

Biden and company stole the country.

I’m sure enough of this that I put my money where my mouth is.

The prior election must be acknowledged as fraudulent, and steps must be taken to prosecute the fraudsters and restore integrity to the system. (This doesn’t necessarily include deposing Joe and Hoe and putting Trump where he belongs, but it would certainly be a lot easier to fix our broken electoral system with the right people in charge.)

Nothing else matters at this point. Talking about trying again in 2024 or 2026 is pointless otherwise. Which is not to say one must never talk about this, but rather that one must account for this in ones planning; if fixing the fraud in the system is not part of the plan, you have no plan.

This will necessarily be piecemeal, state by state, which is why I am encouraged by those states working to change their laws to alleviate the fraud both via computer and via bogus voters. If enough states do that we might end up with a working majority in Congress and that would be something Trump never really had.

Lawyer Appeasement Section

OK now for the fine print.

This is the WQTH Daily Thread. You know the drill. There’s no Poltical correctness, but civility is a requirement. There are Important Guidelines,  here, with an addendum on 20191110.

We have a new board – called The U Tree – where people can take each other to the woodshed without fear of censorship or moderation.

And remember Wheatie’s Rules:

1. No food fights
2. No running with scissors.
3. If you bring snacks, bring enough for everyone.
4. Zeroth rule of gun safety: Don’t let the government get your guns.
5. Rule one of gun safety: The gun is always loaded.
5a. If you actually want the gun to be loaded, like because you’re checking out a bump in the night, then it’s empty.
6. Rule two of gun safety: Never point the gun at anything you’re not willing to destroy.
7. Rule three: Keep your finger off the trigger until ready to fire.
8. Rule the fourth: Be sure of your target and what is behind it.

(Hmm a few extras seem to have crept in.)

Spot Prices

Last week:

Gold $2,736.50
Silver $32.51
Platinum $1,002.00
Palladium $1,124.00
Rhodium $4,950.00
FRNSI* 131.378+
Gold:Silver 84.174+

This week, at Friday close:

Gold $2,684.50
Silver $31.35
Platinum $979.00
Palladium $1,014.00
Rhodium $5,025.00
FRNSI* 128.863-
Gold:Silver 85.630-

No whitewashing it, the precious metals took as big a beating as the Democrats did. Gold dropped over $75 on Wednesday and though it partially recovered Thursday, it dropped again on Friday. It’s possible the bull market is over…let’s see what happens next week.

Notably, silver did even worse than gold; the ratio is now 85.6 to 1.

For someone who took a substantial loss in net worth this week, I sure seem to be in a cheerful mood. I wonder why?

*The SteveInCO Federal Reserve Note Suckage Index (FRNSI) is a measure of how much the dollar has inflated. It’s the ratio of the current price of gold, to the number of dollars an ounce of fine gold made up when the dollar was defined as 25.8 grains of 0.900 gold. That worked out to an ounce being $20.67+71/387 of a cent. (Note gold wasn’t worth this much back then, thus much gold was $20.67 71/387ths. It’s a subtle distinction. One ounce of gold wasn’t worth $20.67 back then, it was $20.67.) Once this ratio is computed, 1 is subtracted from it so that the number is zero when the dollar is at its proper value, indicating zero suckage.

The Grand Tour

Meet Gary Flandro (1934- ):

He’s an aerospace engineer, who is currently the professor for the Boling Chair of Excellence at the University of Tennessee Space Institute. He is also the Vice President and Chief Engineer for Gloyer-Taylor Laboratories (GTL).

He has an interesting academic “ancestry”–he studied under Frank E. Marble, who studied under Hans Wolfgangg Liepmann, who studied under Bar, who studied under Emil Hilb, who studied under Karl Louis Ferdinand von Lindemann (who proved in 1882 that pi is a transcendental number), who studied under Felix Christian Klein, who studied under Rudolf Otto Sigismund Lipschitz, who studied under Johann Peter Gustav Lejeune Dirichlet, who studied under Jean-Baptiste Joseph Fourier (yes, that Fourier), who studied under Joseph-Louis Lagrange (yes, that Lagrange), who studied under Leonhard Euler (yes, that Euler). Academics sometimes like to play “academic genealogy” (as do musicians; some can show that Beethoven or Haydn taught someone who taught someone who…(eventually)…taught them). Every one of these people has a Wikipedia page, with the exception of Bar, many are famous to mathematicians.

That’s cool. But it’s not the reason I chose to mention Flandro.

Flandro is the reason we have closeup pictures of Uranus and Neptune.

In 1964, he came to the realization that we were coming up on a very rare alignment of the outer planets. No, they weren’t going to be in a tidy straight line, but it would be possible to send a spacecraft past Jupiter, get a gravity assist from Jupiter to go to Saturn, then a gravity assist from Saturn to go to Uranus, and so on, on to Neptune and Pluto (still considered a planet back then).

Or, if one sends two spacecraft, get all of that done in less time, by sending one, launched in 1977 to Jupiter, Saturn and Pluto, and the other, launched in 1979, to Jupiter, Uranus and Neptune. This concept (with one modification) was dubbed the Grand Tour program, and was proposed in 1969. That modification was to send two pairs of spacecraft.

Total cost, $1 billion or so in real money, but cheaper than sending separate spacecraft. The biggest issue was that sending a probe of any useful size past Jupiter without any assistance is difficult; it still is. (All of these fancy Jupiter and Saturn orbiters needed gravitational assists to get there with enough fuel to do an orbital insertion burn and still have enough left over to make small maneuvers for many years.) This way, if you could get to Jupiter, you could automatically get to the other planets.

What’s not to like? The money.

Instead of four spacecraft, we’d send two Mariner-type probes. And we’d blow off Uranus, Neptune and Pluto…well, sort of. Now the project was called Mariner Jupiter-Saturn, which was approved in 1972, for $360 million apiece.

Both probes would visit Jupiter, Saturn, and Titan. (Titan was included because even then it was known to have an atmosphere, which made it unusual for a moon.)

That is what was advertised, to keep cost estimates down. Here’s what actually happened. The first probe was launched on a flight plan called JST: Jupiter Saturn Titan. The second was launched on a flight plan called JSX. JSX would visit Jupiter and Saturn, but if the first mission failed either at Titan or earlier, it could be diverted to visit Titan…and that would be it. If not diverted, however, it would not do a close flyby of Titan, but instead go on to Uranus and Neptune. The reason this wasn’t advertised is that controlling those spacecraft for the additional nine years would be expensive.

These would have been Mariner 11 and Mariner 12. The earlier Mariner probes had largely explored Mars; this would have been a continuation of that legacy. But these spacecraft had a lot of new features, and so in March, 1977 NASA held a competition to rename the project. And so, just months before launch they became Voyager 1 and 2. Voyager 1 would visit Jupiter and Saturn with a close flyby of Titan. Voyager 2 would visit Jupiter and Saturn, then Uranus and Neptune, but could be diverted if Voyager 1 failed either before or during the Titan flyby, since Voyager 2 would reach Saturn nine months after Voyager 1. (There was even an option to divert Voyager 1 away from Titan and send it to Pluto, but Titan was considered the more interesting target after Pioneer 11 saw just how thick its atmosphere was.)

Voyager 2 was launched first, on August 20, 1977, then Voyager 1 on September 5th, on a faster trajectory. It would actually overtake Voyager 2 and reach Jupiter on March 5, 1979 (barely a year and a half after launch!). Voyager 2 flew by on July 9, then both were off to Saturn. Voyager 1 reached Saturn on November 12, 1980 (shortly after the election), and flew by Titan later that day. The Titan encounter actually flung it out of the plane of the ecliptic, meaning Voyager wouldn’t be visiting any more planets. Voyager 2 was not diverted, and reached Saturn on August 26, 1981. And then Uranus on January 24, 1986, and Neptune on August 25, 1989, one day shy of eight years after the Saturn flyby.

So far Voyager 2 is the only spacecraft to ever fly by Uranus and Neptune.

Voyager 1 and Voyager 2 are still ticking, believe it or not, and Voyager 1 is now in interstellar space having passed outside of the Sun’s magnetic field. It’s returning data on the almost total vacuum of interstellar space. But, in the next two years (likely next year in fact) their RTG units will have degraded enough that they will no longer be able to power any of the scientific instruments. And ultimately they will be unable to maintain radio contact with Earth sometime in the 2030s; they will be out of range of our receivers.

(The RTGs on the Voyagers are slugs of plutonium oxide; the plutonium is isotope 238 (not the 239 used in bombs) which has an 87.7 year half life. The heat generated is converted to electrical power via thermocouples using the Seebeck effect. When new they generated 160 watts electrical, 2400 watts heat.)

Old Voyagers never die, they just fade away.

Voyager 1 is still moving at 16.9 km/sec relative to the sun; it crosses 3.57 AUs per year…almost the distance between Earth and Jupiter at its closest. Voyager 2 is moving at 15.2 km/sec. Their distances are 162 and 137 AUs, or 24.5 and and 20.5 billion kilometers.

And again, it is thanks to these stalwarts that we have any closeup pictures and data for Uranus and Neptune and their moons. Hubble and JWST can take occasional ganders, but there’s no substitute for being there, however briefly; and for now, this is what we’ve got.

Uranus

Uranus was spotted by John Flamsteed in 1690 as he created his star catalog. If you’ve ever seen a star with a name something like “61 Cygni” (a number and then a Latin genitive of a constellation name), that’s a Flamsteed designation. There are 84 of his designations that are today considered to have been mistakes; in particular “34 Tauri” was actually the planet Uranus.

Uranus was identified as a planet for the first time by William Herschel in 1781, his first thought was to name it after the King…As it happens, King George III; yes, that asshole. Good taste prevailed; we couldn’t get away from assholes apparently but at least it’s more egalitarian: It’s named after everyone’s asshole.

William Herschel, 15 November 1738 – 25 August 1822

OK, more seriously it’s named after the Greek sky god, Ouranos (Οὐρανός). Ouranos was one of the primordial deities, along with Gaia (Earth), he was the father of the Titans…in particular Kronos (Saturn). Saturn in turn was the father of Zeus (Jupiter). So it’s a neat progression, one generation back every planet out from the Sun. (But with this we’re out of generations; nothing preceded Ouranos.

The usual pronunciation is “YER-in-us” rather than “your anus” but I don’t even care for that one (as it means “full of urine”) and would like to go with OO-rahn-ose which is closer to the Greek pronunciation. Not a battle I’m likely to win.

OK, some basic facts since this bit is a recap of the Hugh Janus post from several months ago.

First a picture, with Blue Marble Earth (with a non-fubared Red Sea) photoshopped in for a size comparison. This is a natural-color image of Uranus taken by Voyager 2:

Well, that’s fascinating. We could probably argue over whether that’s more green than blue, or vice versa. It’s about as detailed as any true color image of Venus. Or Titan. More can be learned from false color images.

Uranus is 19.1 AU from the Sun, on average–about twice as far out as Saturn–and takes 84.02 Earth years to make one orbit around the Sun. It rotates once (relative to the Sun) in 17 hours, 14 minutes. However, here’s the thing: its axis of rotation is tipped 98 degrees from being perpendicular to its orbit (compare to our 23.5 degrees). Since axial tilts cause seasons, and this is almost as extreme as they get, Uranus has extreme seasons; at one point in its orbit almost the entire northern hemisphere has a midnight sun while the southern hemisphere gets no sun at all. And the poles get 42 years of continuous sunlight followed by 42 years of darkness (analogous to our poles getting six months of each). Because of these extreme seasons, Uranus has the lowest minimum temperature of any planet in the Solar System coming in at 49K.

This next graphic is a simulation of what Uranus looks like from Earth (hence just about what it looks like from the Sun) from 1985 to 2030, just a bit over half a Uranian year. The rings are included to provide a reference:

Uranus’s equatorial radius is 25,559 (give or take 4) km, compare to Earth’s 6,378. It has a mass 14.5 times that of Earth.

Uranus has multiple magnetic poles, and this likely has something to do with the fact that it is an “ice giant”

We’ve not dealt with ice giants before; these are gas giants (like Jupiter and Saturn) but with a heavier concentration of the molecules that planetary scientists call “ices” (even when they’re not frozen), water, ammonia, methane, sulfur dioxide, etc; generally hydrogen combined with some fairly small atom. Deep inside the planet all sorts of interesting forms of these compounds appear. In particular, water ice has many different polymorphs (different ways of crystalizing) under great pressure. Some of these even break the water molecules apart leaving oxygen crystallized and the hydrogen ions free to move through the lattice, others under greater pressure trap the hydrogen. It is thought that Uranus (and Neptune) have layers of the conducting ice deep inside and this is where the magnetic fields originate. Since the locations are relatively thin shells, it’s likely that multiple magnetic poles would form.

In some ways Uranus and Neptune resemble what you’d get if you removed the (mostly hydrogen and helium) outer layers from Jupiter and Saturn.

Uranus has rings; these were discovered in 1977. The discoverers were planning to watch Uranus pass in front of a star to hopefully learn something about Uranus’s atmosphere. They were surprised to see the star blink out five times before and afterwards, in symmetric patterns, which is what you’d see if an otherwise invisible ring was dimming the light. Later on they detected four more rings. The rings are made out of very dark objects about the size of a basketball (similar in size to Saturn’s rings’ constituents) and thus they couldn’t be seen directly. They’re named with Greek letters, sometimes numbers, and the names are not in any kind of logical order since they were assigned in discovery order.

Moons

Uranus has 28 known moons. The naming scheme is based on characters from Shakepeare and Alexander Pope.

We’ll start with an image taken by JWST; the big ones are bright blue, nine inner moons are also shown.

I learned Uranus had five moons in school, and these “original” five are four medium-sized major moons with one medium-small major moon.

Inner Moons

But we now know of 13 “inner moons” (small, non-round moons that orbit in nice circular orbits, closer than the major moons). That’s the most of any of the four giant planets. Working outward, we have Cordelia and Ophelia, which shepherd the ε (epsilon) ring. Then we have six at very similar distances forming a group: Bianca, Cressida, Desdemona, Juliet, Portia, and Rosalind. Then another close grouping of three: Cupid, Belinda, and Perdita. Finally there are Puck and Mab, Mab is likely the source of the μ (mu) ring.

We have a fuzzy picture with some detail for one of these moons, Puck:

Puck. 162 km across, orbiting at 86,005 km in 0.761 days.

All of these moons are involved with the ring system, which (unsurprisingly) is thought to have resulted from the fragmentation of other inner moons.

Major Moons

Then we come to the major moons; the five we heard about in school if you’re anything remotely my age. They are shown in this montage at the right relative sizes and brightness, in order of distance from Uranus.

They are: Miranda (471.6 km), Ariel (1157.8), Umbriel (1169.4), Titania (1577.8) and Oberon (1522.8). Titania at 1,577.8 km is just a bit bigger than Saturn’s Rhea, and is the largest “medium” moon. Titania and Oberon were discovered by Herschel in 1787, Ariel and Umbriel in 1851 by William Lassell, and Miranda by Gerard Kuiper in 1948. (And you will be seeing the name “Kuiper” a lot in the future.)

At the time Voyager 2 flew by the southern hemisphere of Uranus and each of its moons was oriented to the Sun, and we only got 20-40% coverage in the pictures…and we still don’t know what’s on the other sides of these moons!

These moons are fairly dark, by contrast with the bright moons of Saturn.

Miranda is mostly ice, while the other four seem to have significant rocky content:

The big four seem to all have salt water layers, underlain by hydrated water, and perhaps in the case of Titania and Oberon, dry rocky cores. I get the impression that all of this is somewhat speculative.

Miranda

Miranda, 471.6 km across, orbiting at 129,858 km in 1.41 days

Miranda is likely the most interesting of these moons, with fault canyons 20 km deep, terraced layers, and a patchwork chaotic surface of different ages and features. (We can tell the different ages from the different amounts of meteor craters.) Look at that picture; it looks like a Frankenmoon. Note that the canyons and mountains are large enough to be obvious bumps and cuts in what ought to be a circular outline. There is some speculation that this moon was broken apart and reassembled at some time in the past.

Of course I cannot think of Miranda without remembering the scene from Red Heat, where Ahnuld plays a Soviet policeman in the US to arrest and bring back Georgian thugs (no, the other Georgia, the one where they really talk funny). After roughing up one suspect and then being told that here in the US there are Miranda rights, warnings, etc…

Ariel

The highest resolution image of Ariel from Voyager 2 is this one:

Ariel, 1,157,8 km across, orbiting at 190,930 km in 2.52 days.

The broad channels to the lower right stand out, they’re called grabens and may be from liquid welling to the surface…sometime in the distance past.

Umbriel

Conveniently for those wanting to memorize names, Ariel and Umbriel rhyme which might help you remember they’re adjacent to each other in the list.

Umbriel is dark and heavily cratered, and as you can see the photo is a bit blurry. At the very top is the crater Wunda.

Umbriel, 1169.4 km across, orbiting at 263,982 km in 4.14 days

Titania

As mentioned before Titania is the largest “medium” sized moon, beating out Rhea by a slim margin. Water ice and a bit of carbon dioxide as dry ice have been detected. Again we have one not-very-high-res picture, and a slightly better one.

Titania, 1576.8 km across, orbiting at 436,282 km in 8.71 days.

Oberon

Oberon, 1522.8 km across, orbiting at 583,449 km in 13.46 days.

Oberon has a lot of bright patches, these are largely craters with bright rays. The largest of these is Hamlet, almost dead center in the photograph. There is also an 11 km mountain at about 8 o’clock on the limb.

Irregular Moons

There are 10 irregular moons, ones that are lumpy and orbit in inclined or even retrograde orbits with high eccentricity. They are: Francisco, Caliban, Stephano, S/2023 U 1, Trinculo, Sycorax, Margaret, Prospero, Setebos, and Ferdinand. The largest of these irregular moons is Sycorax, a respectably-sized 120-200km. Many of these moons were discovered by the Hubble Space telescope. Caliban, Stephano and S/2023 U 1 all seem to be part of a group, six of the others are retrograde but with very dissimilar orbits, and Margaret is actually prograde at a 60 degree inclination.

Patterns

We’ve seen a definite pattern so far with giant planets’ moons. There are inner moons, small, irregularly shaped moons that nevertheless are in nice, tidy circular orbits that have almost no inclination relative to the planet’s equator. Then major moons; the trend there seems to be smaller and smaller moons on the whole, the further out you go from the Sun (Jupiter had four large moons and no medium moons, Saturn had one large moon and a bunch of medium and medium-small ones, Uranus has only medium and medium-small ones).

Since all of those moons are in nice circular orbits usually in the plane of the planet’s equator, it’s thought that the original lump of gas, volatiles, and solids that formed the planet also formed the moons. This nebular lump would collapse, spin faster (angular momentum being conserved) and form an accretion disk. The main central mass would become the planet and the rest would form the regular moons (inner and major). This is actually a miniature of the formation of the Solar System itself, where the disk around the proto-Sun would form planets, all in nearly the same orbital plane, all orbiting in the same “prograde” direction.

Outside of those major moons, we go directly to irregular moons, which come in groups suggesting some larger body was broken up. The irregular moons are never big enough to be round, and are called irregular largely because they have very eccentric, inclined orbits; most in fact are retrograde, orbiting the planet “backwards” from the normal counterclockwise as seen from over the north pole. This strongly suggests these objects did not form with the planets as the regular moons did, but rather got captured later.

Saturn is a slightly special case, some small moons are mixed in with the major moons, including four that are Trojans to a couple of the major moons, but this is an addition to the pattern, not a true breaking of it.

Onwards…

Unlike with Saturn I simply wasn’t able to bury you in pictures and information. Again, that’s a consequence of the fact that we’ve sent one spacecraft on a flyby, ever. Whereas at Saturn and Jupiter we’ve been able to park spacecraft there for years, completely map the major moons, get good reads on their masses, and so on.

So will we ever learn more? There has been some talk of sending orbiters to Uranus, and it was given a high priority during NASA’s last decadal plan, but nothing was done about it. China is talking about sending probes as well. But there’s nothing firm.

Next month, we take up Neptune!

2024·11·02 Joe Biden Didn’t Win Daily Thread

What is it that feeds our battle, yet starves our victory?

Blast from the Past

I reached voting age just after the election of 1980.

This was the time when America was humiliated by the Iranian hostage crisis. The Soviet Union was rampaging throughout the third world and was currently involved in Afghanistan despite our protests. The economy was on the ropes, with double digit unemployment and inflation that briefly reached 18 percent (and that’s the official number…no doubt it was actually worse). The then-president even used the word “malaise.”

Then we beat the Soviet Union in a hockey game.

That sounds trivial, doesn’t it? A frigging hockey game.

But the symbolic value was tremendous. It was a win after a long string of losses…and it ended up being a turning point.

We elected a new president, who didn’t have to do anything at all to resolve that damned hostage crisis. Iran released them on Inauguration Day.

And then there was this song…which expressed the sentiment very well (and doesn’t get played nearly as much as another popular song from back then by the same group does now).

America was on the move again.

Today is the 2nd. On the 5th…we will see what happens. Regardless of the result, it’s going to be rough, either because we lost and we’re done, or because we won and it’s being stolen, in which case if 2020 is any guide, we’re done, or because we won outright, and the Enemy is not going to go down without a lot of ugliness…maybe even kinetic ugliness.

Keep your powder dry. If things go well, this is the turnaround point.

January 6 Tapes?

Where are the tapes? Anyone, Anyone? Bueller? Johnson??

Paging Speaker Johnson…this is your conscience calling you out on broken promises.

News Flash

Today, it is still the case that Joe Biden didn’t Win.

I realize that to some readers, this might be a shock; surely at some point things must change and Biden will have actually won.

But the past cannot actually be changed.

It will always and forever be the case that Joe Biden didn’t win.

And if you, Leftist Lurker, want to dismiss it as dead white cis-male logic…well, you can call it what you want, but then please just go fuck off. No one here buys that bullshit–logic is logic and facts are facts regardless of skin color–and if you gave it a moment’s rational thought, you wouldn’t either. Of course your worthless education never included being able to actually reason–or detect problems with false reasoning–so I don’t imagine you’ll actually wake up as opposed to being woke.

As Ayn Rand would sometimes point out: Yes, you are free to evade reality. What you cannot do is evade the consequences of evading reality. Or to put it concretely: You can ignore the Mack truck bearing down on you as you play in the middle of the street, you won’t be able to ignore the consequences of ignoring the Mack truck.

And Ayn Rand also pointed out that existence (i.e., the sum total of everything that exists) precedes consciousness–our consciousnesses are a part of existence, not outside of it–therefore reality cannot be a “social construct” as so many of you fucked-up-in-the-head people seem to think.

So much for Leftist douchebag lurkers. For the rest of you, the regular readers and those lurkers who understand such things: I continue to carry the banner once also carried by Wheatie. His Fraudulency didn’t win.

Let’s Go, Brandon!!

His Fraudulency

Joe Biteme, properly styled His Fraudulency, continues to infest the White House, we haven’t heard much from the person who should have been declared the victor, and hopium is still being dispensed even as our military appears to have joined the political establishment in knuckling under to the fraud.

One can hope that all is not as it seems.

I’d love to feast on that crow.

(I’d like to add, I find it entirely plausible, even likely, that His Fraudulency is also His Figureheadedness. (Apparently that wasn’t a word; it got a red underline. Well it is now.) Where I differ with the hopium addicts is on the subject of who is really in charge. It ain’t anyone we like.)

Justice Must Be Done.

The prior election must be acknowledged as fraudulent, and steps must be taken to prosecute the fraudsters and restore integrity to the system.

Nothing else matters at this point. Talking about trying again in 2024 is hopeless otherwise. Which is not to say one must never talk about this, but rather that one must account for this in ones planning; if fixing the fraud is not part of the plan, you have no plan.

Lawyer Appeasement Section

OK now for the fine print.

This is the WQTH Daily Thread. You know the drill. There’s no Poltical correctness, but civility is a requirement. There are Important Guidelines,  here, with an addendum on 20191110.

We have a new board – called The U Tree – where people can take each other to the woodshed without fear of censorship or moderation.

And remember Wheatie’s Rules:

1. No food fights
2. No running with scissors.
3. If you bring snacks, bring enough for everyone.
4. Zeroth rule of gun safety: Don’t let the government get your guns.
5. Rule one of gun safety: The gun is always loaded.
5a. If you actually want the gun to be loaded, like because you’re checking out a bump in the night, then it’s empty.
6. Rule two of gun safety: Never point the gun at anything you’re not willing to destroy.
7. Rule three: Keep your finger off the trigger until ready to fire.
8. Rule the fourth: Be sure of your target and what is behind it.

(Hmm a few extras seem to have crept in.)

Spot Prices.

Kitco Ask. Last week:

Gold $2,748.70
Silver $33.77
Platinum $1033.00
Palladium $1219.00
Rhodium $4,950.00
FRNSI* 131.968+
Gold:Silver 81.395-

This week, markets closed as of 3PM MT.

Gold $2,736.50
Silver $32.51
Platinum $1,002.00
Palladium $1,124.00
Rhodium $4,950.00
FRNSI* 131.378+
Gold:Silver 84.174+

Gold touched $2790 on Wednesday, then suffered an extreme beatdown on Thursday. It looked like it might actually recover a bit on Friday but dropped at the end of the day for a net loss. Similar things happened to silver, but it was worse, it dropped much more, in percentage terms, than did gold and Gold:Silver went right back up into 84 territory. The worst beating in percentage terms was palladium…and I tend to think that’s a bad sign; it’s the metal most closely associated with catalytic converters, hence the car industry. However, palladium has a very variable supply, so it could just be it’s slightly more of a glut on the market than it was last week.

*The SteveInCO Federal Reserve Note Suckage Index (FRNSI) is a measure of how much the dollar has inflated. It’s the ratio of the current price of gold, to the number of dollars an ounce of fine gold made up when the dollar was defined as 25.8 grains of 0.900 gold. That worked out to an ounce being $20.67+71/387 of a cent. (Note gold wasn’t worth this much back then, thus much gold was $20.67 71/387ths. It’s a subtle distinction. One ounce of gold wasn’t worth $20.67 back then, it was $20.67.) Once this ratio is computed, 1 is subtracted from it so that the number is zero when the dollar is at its proper value, indicating zero suckage.

Piling On / Security Alert

OK, how can I pile onto the Flat Earthers and pass on a security alert at the same time, you ask?

Well, because Flat Earth Dave sells an app. For three bucks you get a flat earth clock and can also connect with other Flerfers.

This app has come under scrutiny. And it turns out that Flat Earth Dave doxxed all of his customers.

But before we get to that, a code analysis reveals that the app computes the distance between customers (to help them connect with other flerfers), using the “haversine formula” which is how you compute distances along great circle arcs on a sphere given the two points’ latitude and longitude. In other words Flat Earth Dave’s own code assumes a spherical Earth! (Almost as if he knows something he’s not saying…)

[If you’re curious, it’s {\displaystyle \operatorname {hav} \theta =\operatorname {hav} \left(\Delta \varphi \right)+\cos \left(\varphi _{1}\right)\cos \left(\varphi _{2}\right)\operatorname {hav} \left(\Delta \lambda \right)}where θ is the angle between the two points, φ1 and φ2 are the two points’ latitudes, Δφ is the difference between the two latitudes, and Δλ is the difference between the two longitudes. The haversine is an obscure trig function, (1-cosθ)/2; this appears in spherical trigonometry a lot so they gave it its own name. All angles are in radians, particularly since in spherical trig the sides of triangles are actually great circle arc lengths. Once you have θ, you multiply by the radius of the Earth to get the distance in miles or kilometers.]

But we already know Flat Earth Dave is a scum-sucking liar and a hypocrite, because after years of saying he’d love to go to Antarctica to show the sun sets there during Antarctic summer…he turned down the opportunity to do so…clearly knowing he’d be proven wrong but as long as he doesn’t go on the trip he can try to tapdance around the fact that he’s full of shit and knows he’s full of shit.

The bigger issue here is that it’s pretty easy for a hacker to query the app’s server database without even logging in to the app. So they can get hold of everyone’s location, name, and password. (The password is stored in the clear, which is something any computer professional knows not to do. This is the computer science equivalent of shooting yourself in the foot or poking out your own eyeball with a soup spoon.) So if you bought the app and logged in, whatever password you used on that app…which hopefully isn’t the same as a password you use anywhere else, like (say) your online banking or even worse your email…has been compromised.

So if you trusted Flat Earth Dave, you’ve been conned and doxxed. And you won’t be getting your three bucks back (nor the $11/year if you subscribed). Have a nice day.

A different treatment of the same topic, combined with some debunks. A bit long so I certainly wouldn’t expect you to watch it.

Saturn’s Other Moons

Saturn’s rings…and three moons, Tethys (the big one), Hyperion (Left and a bit up from Tethys), and Prometheus (the tiny blob in the lower left, almost touching the rings).

Titan, covered last week, is by far the largest of Saturn’s moons. The other 145 (!) moons put together–plus all of the matter in the rings–don’t have even 5 percent of the mass of Titan.

Size notwithstanding much of interest here. With Saturn we encounter our first medium-sized major moons, there are nine in the Solar System and Saturn has four of them. They are (in order from Saturn outwards): Tethys, Dione, Rhea (closer than Titan) and Iapetus (beyond Titan). All have diameters of over 1000 kilometers. All except Iapetus orbit closer to Saturn than Titan. In addition to that, there are two of the medium-small major moons as well, Mimas and Enceladus (both are closer than Tethys) and one comparably sized moon that is not major (meaning, it isn’t round), Hyperion (between Titan and Iapetus). We’ll cover each of these seven moons in detail further down.

(If nothing else, after working on this post for a few days I now have the order of the big eight moons from Saturn outwards, memorized.)

If you remember Saturn once having nine moons (possibly from school in the 1960s) the ones I just mentioned are eight of those nine, with the other one being Phoebe…which is in a totally different class, and much further away than the other eight. I’ll say a bit about that one too. (I’m not quite that old, but a lot of stuff I did see in school in the 1970s was out of date and said “nine.”)

Saturn with many of its more prominent moons,
Hyperion, Iapetus and Phoebe are not in this picture, but three of the close-in minor moons (Epimetheus, Janus and Prometheus) shown.

But Saturn has a host of other much smaller moons, too, and in many cases they’re interesting because of their interactions with the rings.

Twenty four of the moons are regular, meaning: They orbit in or near Saturn’s equatorial plane in prograde orbits–the one exception to that is Iapetus, considered regular even though it has a fairly high inclination of 7.57 degrees. Every one of the moons (except Phoebe) I just mentioned are regular moons.

The other 122 moons are all irregular, generally small and insignificant, similar to the mess we had at Jupiter. Saturn has more stuff close to the planet than Jupiter does, but fewer “big categories” overall. There’s also a major distinction here between “Inner” and “Outer” moons; inner moons are either inside the very tenuous E Ring, or actually within it. What’s the E Ring? I’ll discuss it some below, but here’s a reminder:

Saturn backlit. The E-ring is the very foggy outermost ring in the picture.

Inner Moons (Inside or Within the E Ring)

Ring Moonlets actually orbit within the Rings. They’re significantly larger than the average, run-of-the-mill ring chunk, but none are of significant size. They are interesting, though because of their interactions with the rings. All are regular, which makes sense because they actually orbit within the “big” rings. Only one has an official number (S/2009 S-1); it’s about 300 m across. Others get down as low as 40 m across, and are not part of the total count.

Ring Shepherds can either be within the rings, or just barely outside of them, and they either keep the ring particles from leaving the rings, or causing gaps to form within the rings. There are four of these, with the most famous being Pan, about 27 km across, which looks like a ravioli. The others are Daphnis, Atlas, and Prometheus.

There are four other small moons well outside the rings, but still pretty close to them in the grand scheme of things. One of these is the tenth moon I knew about as a kid, but it’s a bit confusing because one astronomer spotted the tenth moon, then another one saw it…but in totally the wrong place in its orbit, which threw doubt onto the original observation (as well as this observation). Eventually we realized that there were two moons, Epimetheus and Janus, in the same orbit but different positions in the orbit, and so they are now regarded as the tenth and eleventh moons of Saturn, respectively. So those books from my childhood were written when we didn’t realize yet that Saturn actually had 11 known moons. The other two in this group are Pandora and Aegaeon.

Then we get to the Inner major moons, the first of which is Mimas which I will discuss below.

There are three small moons orbiting between Mimas and the next major moon; again these are all regular moons, these are the Alkonyides group.

Next are more major moons, Enceladus, Tethys and Dione. I’ll discuss each one in detail below.

Tethys and Dione both have two Trojan moons (sharing the same orbit but sixty degrees away from their bigger companion); a bit more on that below too. So far the only moons anywhere in the solar system known to have Trojans are these two.

So far: four major moons (two medium size, two medium-small), one dinky moon with only a number, the four shepherds and four close-in moons, the three Alkonyides, the four Trojans, total 20. All are regular moons, which means there are four remaining regular moons and all 122 irregular moons to go.

Outer Moons (Outside the E Ring)

Outer Big: Rhea, Titan, Hyperion and Iapetus. (All of these will be covered in some detail below.) Were it not for Hyperion, which is not a major moon, just kind of big but lumpy, these could be called the outer major moons. All are regular, even Iapetus with its significant orbital inclination. [Note: Wikipedia calls these the Outer Large moons, but I don’t want to confuse that use of the word “large” with the way I’ve been using it to denote the planetary-sized moons of the solar system.]

And with the last four regular moons checked off, we have nothing left but the entire list of 122 irregular moons. They’re considered irregular because of their eccentric, inclined orbits. These can be broken down into four groups with similar orbits, the Inuit group (13) inclined at about 47 degrees, the Gallic group (7) inclined at about 35-40 degrees, the Norse group (100, including Phoebe) which are all retrograde with inclinations about 170 degrees), then two more “miscellaneous” moons that are prograde. As with Jupiter, it’s likely each of these groups has some sort of common origin (but separate from the other groups). Also the names of the groups indicate the naming convention, with the Norse group named after Norse gods…except for Phoebe which was discovered long before the others were, there was no hint until much later that there was a “group” here. (This isn’t the first, nor will it be the last, time that some body that had been known for a while turned out to be the first of a big group of similar objects.)

The overall summary is in this diagram (which you may want to right-click on to give it full-screen in another tab):

The upper stripe is a fairly conventional side view of Saturn including showing the A through E rings, and most of the Inner Moons including the four majors, Mimas, Enceladus, Tethys and Dione (two are medium sized, two are medium-small).

The middle stripe steps out ten times, and Saturn is now shown at a tilt. The four “Outer Big” moons (one actually large, two medium sized, and one medium-small (and not major) are here. Note that Iapetus is not in the same plane as the others. Here you’ll see lines drawn through each of the four moons; these actually denote the range of possible distances for those moons, meaning they’re in moderately elliptical orbits.

The last diagram zooms out ten times again, or 100 times the first, and shows all of the irregular satellites, at their orbital inclinations. The Norse group has a HUGE range of distances from Saturn, indicating they are all in highly elliptical orbits.

The Big Ones

With the big picture out of the way, let’s go back to those Major Moons (plus Hyperion). And I’ll toss in Phoebe as a bonus, because there’s some interesting things about it too. Let’s start with a table. But first, I need to explain a couple of things. The “A” Ring is the outermost readily visible ring. The “E” ring, on the other hand is very tenuous, discovered in 1907 but not confirmed until 1980…and we’ll soon see how it came to be.

MoonDistance From Saturn, 1000s of Km; and
(in terms of Titan)
Orbital Period, daysDiameter, kmDiscovery year and (order)
Outer edge of A ring136.8
Inner edge of E ring180.0
Mimas186.0 (0.152)0.942396.41789 (7)
Enceladus238.4 (0.195)1.370504.21789 (6)
Tethys295.0 (0.241)1.8881062.21684 (5)
Dione377.7 (0.309)2.7371122.81684 (4)
Outer edge of E ring480.0
Rhea527.2 (0.431)4.5181527.51672 (3)
Titan1221.9 (1.000)15.9455149.51655 (1)
Hyperion1481.5 (1.212)21.277~270.0 (not spherical)1848 (8)
Iapetus3561.7 (2.915)79.3311468.61671 (2)
Phoebe (Bonus)12929.4 (10.581)550.3 (retrorgrade)213.01898 (9)
Table of the Big 8 moons of Saturn, plus Phoebe

These moons are all consecutive, with no intervening small stuff, except for the three Alkyonides between Mimas and Enceladus, and the four Trojan moons of Tethys and Dione.

All of these moons, except Hyperion and Phoebe, are tidally locked to Saturn, displaying the same side towards Saturn at all times, like our Moon does to Earth.

Mimas

Cassini discovered Iapetus, Rhea, Dione and Tethys in the mid-late 1600s. He also discovered the Cassini Division between the A (outermost easily visible) and B (inside the A ring, wider but a bit dimmer) rings, plainly visible even in the photograph I supplied above. The Cassini division is about 4800 kilometers across, and it is actually caused by Mimas; anything orbiting in the gap is in a 2:1 resonance with Mimas (meaning: orbiting twice as fast) and the regular pulls by Mimas in the same places tend to nudge particles out of that orbit…hence the gap. However, it’s not completely empty.

Mimas is the seventh largest moon of Saturn; it just barely makes it into the “medium-small” major class. It’s most notable feature is a very large (compared to it) crater, named after Herschel (who discovered Mimas in 1789 and did not try to name it after King George the Turd), that instantly earned it the nickname “Death Star Moon” since Star Wars was a recent memory when the Voyager spacecraft first photographed it. Look, twins separated at birth:

Mimas. 396.4 km across, orbiting at 186,000 km in 0.942 days.

(I was in high school and at least one photograph from a different angle that was published looked distinctly…weapons grade to many of us. However, at roughly 64K surface temperature, it’s colder than a witch’s.)

Since we’ve sent Cassini through the system, we have seen the different moons’ gravity acting on it and can assess the masses of these moons. Sizes can be measured off the photographs (since distance is known). Dividing mass by volume, we can get a good idea of the density of these moons. It turns out that Mimas’ density is 1.15 times that of water, implying it’s mostly ice with some rocks in it. (But remember, at these temperatures, ice itself is as hard as a rock.)

Enceladus

If when you say it, Enceladus comes out something like “enchiladas” you’re doing it wrong. It’s “en-SELL-a-duss.” Like the other major moons, it’s named after a titan from Greek mythology. There was a time when the gods fought the titans (who were the previous generation), this is called the “gigantomachy.” According to the legend, Athena picked up a gigantic rock and dropped it on Enceladus. It didn’t kill him but apparently he couldn’t push it off of him and it’s still there. Every once in a while Enceladus will twitch and there is an earthquake. (To this day the Greeks will reference that in talking about earthquakes.) The rock, by the way, is now Sicily. (I told you it’s still there.)

Enceladus is one of two moons in the solar system that are in the 500-1000 km diameter range…and it just barely makes it at 504 km. (The other is Dysnomia, estimated to be about 615k km across, which orbits the dwarf planet Eris. We can’t determine if Dysnomia is rounded or not–it’s very hard to see because it is so dark but it’s got a low enough density that it might not have strong enough gravity to crush itself into a spherical shape. And I missed this one when I first did my Moon Roundup–which I have since edited to reflect the fact that Dysnomia exists.)

Enceladus is the most reflective object in the solar system, it’s blast white. Which means it’s clean, which means fresh. And in fact, Enceladus has volcanoes on it, clustered near its south pole, that regularly renew the surface. But unlike the ones on Jupiter’s inner major moon Io, these erupt water.

Enceladus. 504.2 km across, orbiting at 238,400 km in 1.370 days.

That is not a black and white photograph (nor will other moons be shown in black and white), It’s just that these moons are neutrally colored. As such people will try to punch it up a bit. So, seen almost as often as that picture is a false-color image, like this one:

The blue brings up the “tiger stripe” ridges rather well, and these are tectonic features, from the icy surface breaking into “plates”. (That implies another subsurface “ocean” like on Europa and Titan.) Some are canyons 5-10 km wide and a kilometer deep.

Enceladus has a density 1.6 times that of water, so it has a much higher percentage of rocks in it than does Mimas.

At least some volcanoes–well strictly speaking these are geysers–are still active, here’s an oblique shot of the south polar region:

This stuff is coming from the subsurface ocean. And because of that subsurface ocean and evident sources of heat, Enceladus is being thought of as yet another candidate for life to exist.

Cassini nearly didn’t get to see this. On one Enceladus flyby one of the scientists, Professor Michele Dougherty, noticed what she called a “pimple” in the magnetometer readings, caused by moving ionized water. She managed to persuade the JPL Cassini team to change the schedule of flybys to get much closer to Enceladus. (This was a huge risk–if they found nothing, a lot of irreplaceable fuel would be gone for nothing, and perhaps the magnetometer team would not be taken seriously again.) It paid off, bigly: the lead investigator for the camera, Doctor Carolyn Porco, said she nearly fell off her chair when she saw the pictures of the geysers.

This is the only confirmed liquid water in the solar system, other than on Earth.

We have talked of going ice fishing on Europa. But here, there’s no need to drill! We can send a spacecraft through the plumes and analyze the vapor, to perhaps see what’s in the water. Biomolecules? Life?

These volcanoes have been venting so prolifically, in fact, that Enceladus is the primary source of the E ring. (By happy coincidence, Enceladus starts with E, so it’s a good mnemonic.) If you need more evidence:

Near the center, the black dot buried in the E ring is Enceladus. The white blur below it is the geysers. And of course the E ring is the arc of mist you see.

Tethys

Tethys is another ball of ice, neutral colored and almost as bright as Enceladus. What sets it apart is that its density is 0.98 that of water, indicating it must be almost pure ice…and likely porous to boot.

Tethys. 1062.2 km across, orbiting at 295,000 km in 1.888 days.

Although not as obvious as Herschel is on Mimas, there is a large impact crater here too, named Odysseus.

Tethys has two other moons occupying its orbit, one 60 degrees ahead at Lagrange Point 4 (L4), named Telesto, the other 60 degrees behind at Lagrange Point 5 (L5), Calypso. This is actually a special solution to the three body problem, bodies placed at those two points are very stable. Objects like these are called “Trojans”. (Jupiter has thousands of Trojan asteroids.)

Dione

Dione is less icy than Tethys, with a density 1.48 times that of water. For some reason, its trailing hemisphere is darker than its leading hemisphere. (What is a trailing (or leading) hemisphere? Since this moon is tidally locked, it always has the same side facing Saturn; that means it also has the same side “facing” the direction it moves in it’s orbit; that’s the leading hemisphere and the other hemisphere is the trailing hemisphere.)

Dione. 1122.8 km across, orbiting at 377,700 km in 2.737 days.

The trailing hemisphere has “wispy” features seen by the Voyager probes, which turn out to be ice cliffs several hundred meters high. The cliffs are formed by tectonic forces and the bright “wisps” are actually the fresh faces of the cliffs. In fact Dione has a lot of fractures on the trailing hemisphere.

In case you’re thinking I am lying about these gray-white pictures being color images, here’s Dione with Saturn in the background. The sun is shining from below the viewer, and you can see shadows of the rings on Saturn in the upper right.

Dione and Saturn

Dione also has Trojans, Helene (leading) and Polydeuces (trailing).

Rhea

Now we leave the inner moons, and go to the outer regular moons, the ones completely outside the E ring.

Rhea is the second largest moon of Saturn and the second largest “medium size” moon in the Solar System (edged out by Uranus’s Titania), but bear in mind with Titan having 96 percent of the mass of all moons and rings in it, Rhea is a very distant second to Titan.

Rhea, second largest moon of Saturn. 1527.5 km across, orbiting at 572,200 km in 4.518 days

In many ways it’s similar to Dione, perhaps a bit less dense at 1.24 times water, it’s basically 3/4 ice. It has the same leading/trailing distinction, with wispy features that turn out to be cliffs, just like Dione.

Rhea might actually have a ring of its own, a very tenuous one–and that would be a first for a moon. Some indirect evidence (changes in the flow of electrons in Saturn’s magnetic field) points towards it, but Cassini was unable to image it or otherwise confirm it…so it may be necessary to explain that evidence in other ways.

Titan

(Covered last week, but to recap: 5149.5 km across, orbiting at 1,221,900 km in 15.945 days).

Hyperion

Now we come to an oddity. Hyperion is one of the largest objects in the solar system that is not round even though it’s not all that much smaller than Mimas.

When faced with something like this, one asks why Hyperion in particular did not collapse into a sphere. And the reason for that is it’s very light for its size…you could even joke about it being the styrofoam moon. The density is 0.54 times that of water. As such it has only 15% of the mass of Mimas, which is the smallest known body that is made spherical by gravity.

How can this be? Well, take a look:

Hyperion the Sponge Moon. Roughly 270 km across, orbiting at 1,481,500 km in 21.277 days.

It looks like a giant sponge! It has a porosity of 0.46 (which makes me wonder how one puts a number on porisity so down a Wikipedia rabbit hole I go and…ah yes, that means it’s 46 percent empty space).

Interestingly, it’s not tidally locked to Saturn. Instead it is chaotically tumbling, rotating around multiple axes at once. This is the only regular satellite in the solar system that is not tidally locked to its primary. (Remember that “regular” satellites are ones in low inclination nearly circular orbits; these tend to be close-in to the primary.) Because its rotation is actually chaotic, it’s very difficult to predict how it’s going to be oriented at some time in the future.

It may not be tidally locked to Saturn, but it is in an orbital resonance with Titan. In the time it takes Titan to orbit Saturn four times, Hyperion orbits three times.

Another thing that makes this moon a change of pace is that it’s not blast white; it seems to be covered by a thin layer of dark material, likely hydrocarbons.

Iapetus

(Pronounced EYE-app-et-us.) Much further out than the others, this is at the edge of the regular moons. This moon is another oddball, a relief after several moons that seem very much alike other than their size. First, its orbital plane is actually inclined by 15 degrees to Saturn’s equator, so from this moon you can actually see the rings tilted rather nicely. Here is an illustration of the situation:

Orbits of Saturn’s other major moons in blue, the orbit of Iapetus in red.

Iapetus is famous for having its leading hemisphere be as dark as coal while its trailing hemisphere is bright, about as bright as Europa. Thus, when its on one side of its orbit (as seen from anywhere far away from Saturn, such as Earth) it’s quite bright, on the other side, it’s quite dark (actually too dark for the telescope that discovered Iapetus), it could almost be thought of as a blinking beacon.

Iapetus. 1468.6 km across, orbiting at 3,561,700 km in 79.331 days

Or, if you’re Arthur C. Clarke, there’s no “almost” about it; it’s a blinking beacon.

We’ve all seen or at least heard of the iconic movie 2001: A Space Odyssey. It was based on Arthur C. Clarke’s (1917-2008) novel of the same name. There is, however, one very big difference between the book and the novel.

Arthur C. Clarke on the set of 2001 (the movie), 1965.
Note that the pod bay door is open. Apparently HAL is willing to open the pod bay door only if it will kill someone to do so. But Clarke seems perfectly able to breathe.

[Possible spoiler]. In the movie, an alien artifact, a “monolith” is excavated on the Moon; when the sun hits the unburied monolith for the first time, it blasts a loud radio signal. The book is the same way; the monolith is “phoning home” telling its makers that someone–presumably a new intelligent species (us!)–has found it.

[More spoiler] The difference is, in the movie the signal is aimed at Jupiter. In the book, it’s aimed at Iapetus, the blinking beacon. In the book, the already scheduled mission to Jupiter is changed…it’s now going to be a one-way trip to Saturn (with a Jupiter flyby), with the astronauts all going into cold sleep at Saturn to await retrieval by the next mission–once they’ve looked around a bit at Iapetus. It turns out that there’s a monolith waiting for them there, right smack dab in the center of a clearly artificial white oval that accounts for Iapetus’ bright side (making it look like a pupil in an eye). In the movie, of course, the Monolith is orbiting Jupiter. The result of getting close to the monolith is the same in both cases. Had they decided to go to Saturn in the movie, you’d have seen some different special effects (Saturn as a crescent, perhaps; that’s mentioned in the book–instead of Jupiter and the Galilean moons).

[Spoiler, this time for the sequel 2010]. When Arthur C. Clarke wrote 2010, the sequel, he decided to make it a sequel to the movie, reasoning more readers were likely to be familiar with it than the book. And this turned out to be lucky because he was able to leverage off the possibility that Europa has life. The 2010 movie leaves out the Chinese probe that was destroyed by Europan life. The hostility in the book was between China and everyone else, not between the US and the Soviet Union (who were fairly friendly to each other). The movie kept all the power of the book, but removed the Chinese subplot of the fatal discovery of life on Europa (it was there anyway) and added in a nasty dash of propagandizing about Reagan’s Central American policies. If you enjoyed the movie I recommend the book.

OK back to Iapetus. The coloring disparity is even more apparent when one makes a map of Iapetus. There’s little detail in the dark areas, because, frankly, we can’t sucking fee that well there:

The dark region is named Cassini Regio.

Iapetus has one other unusual feature…a raised ridge running along the equator, now named the Voyager Mountains. This was first hinted at by Voyager, which passed over Iapetus’s north polar regions. The ridge is 20 km or so wide, and 13 km tall (over 50 percent higher than Everest is above sea level). There are peaks that go up as much as 20 km. There are places where it forks, has three parallel areas. However…this ridge is in the dark zone. On the bright side, there is still a string of isolated 10km tall mountains along the equator. Given Iapetus is considerably smaller than Earth, this is a very prominent feature, as you can see here:

Maybe a snow plow drove by and left this ridge.
But this hypothesis is not tenable as there are no driveways for the ridge to block.

We aren’t clear on why this ridge formed. Nothing suggested explains why it follows the equator so well. And no suggestion explains why it only appears in the Cassini Regio (dark area).

As a final treat, here’s an enhanced picture. On my system at least, I can even see the equatorial ridge on the far right.

Phoebe

This one’s a bonus (though if you’ve made it this far, you might deem it more a case of me prolonging your suffering); it’s not a major moon, it’s not one of those five almost-major moons comparable to the medium-small major moons…it’s an irregular moon, basically trash picked up by the planet. But we’ve known about it for quite some time, and it’s pretty large for a “trash” moon.

Phoebe was actually the first object Cassini flew by. Cassini’s arrival was deliberately timed so that it would be able to encounter this irregular moon, but of course once in orbit about Saturn it never came out this far ever again. But that does make Phoebe the best-known irregular moon.

Phoebe. Way out there. 213 km across (average), orbiting retrograde at 12,929,400 km in 550.3 days.

Phoebe orbits “backwards” or retrograde (the second largest object in the Solar System to do so), so it’s thought to be a captured asteroid like object, only from the outer parts of the Solar System, the Kuiper belt (we’ll get to those). It’s also in a highly inclined orbit. Here is an animation (note the faint lines showing distance above and below Saturn’s equatorial plane). The light blue object is Titan.

Phoebe appears to be differentiated (denser stuff in the center) so it’s possible it was once spherical and got warped by repeated impacts.

It’s much too far away from Saturn to have become tidally locked, and isn’t. It rotates in nine hours and 16 minutes, rather than once every 18 months as it would if it were tidally locked.

Phoebe is the source of the “Phoebe ring,” a very tenuous ring of debris about Saturn, thought to be the result of stuff blown off of Phoebe by meteoroid impacts. The ring matches Phoebe’s orbit, so it is inclined to Saturn’s other rings. Here is an artist’s illustration (note they had to blow up Saturn).

The vast Phoebe ring in relation to Saturn, which is blown up in an inset so you can recognize it.

Phoebe has the distinction of being used as the alien weapon in the recent SF series The Expanse.

Well, that’s all. folks! Saturn has the most major moons of any of the planets or even dwarf planets…so from here on out things should get a little bit easier, at least so long as we are looking at planets. (It will also help that we’ve flown past everything from here on out exactly once and never sent an orbiter–so we know next to nothing about anything out there.)

I’ll conclude with pictures of Giovanni Domenico Cassini (8 June 1625 – 14 September 1712), discoverer of four moons and the Cassini division in the rings…

and Christiaan Huygens, 14 April 1629 – 8 July 1695, discoverer of Titan and the first to realize Saturn had rings. (The original Dutch pronunciation is [ˈkrɪstijaːn ˈɦœyɣə(n)s] [sound file of pronunciation] which just goes to prove the Dutch adage that Dutch isn’t a language it is a throat condition.)

The next planet out is Uranus, but I’ve already done the planet (the Hugh Janus of the Solar System: https://www.theqtree.com/2023/12/30/2023%C2%B712%C2%B730-joe-biden-didnt-win-daily-thread/) so after a short recap (because our wits are all dulled from listening to Kamaltoe Hairyass for the last few months), we can go directly to Uranus’s bevy of medium and medium-small moons next time.

2024·10·26 Joe Biden Didn’t Win Daily Thread

What is it that feeds our battle, yet starves our victory?

Speaker Johnson
Pinging you on January 6 Tapes

Just a friendly reminder Speaker Johnson. You’re doing some good things–or at least trying in the case of the budget–but this is the most important thing out there still hanging. One initial block released with the promise of more…and?

We have American patriots being held without bail and without trial, and the tapes almost certainly contain exculpatory evidence. (And if they don’t, and we’re all just yelling in an echo chamber over here, we need to know that too. And there’s only one way to know.)

Either we have a weaponized, corrupt government or we have a lot of internet charlatans. Let’s expose whatever it is. (I’m betting it’s the corrupt weaponized government, but if I am wrong, I’d like to see proof.)

Justice Must Be Done.

The prior election must be acknowledged as fraudulent, and steps must be taken to prosecute the fraudsters and restore integrity to the system.

Nothing else matters at this point. Talking about trying again in 2022 or 2024 is hopeless otherwise. Which is not to say one must never talk about this, but rather that one must account for this in ones planning; if fixing the fraud is not part of the plan, you have no plan.

Small Government?

Many times conservatives (real and fake) speak of “small government” being the goal.

This sounds good, and mostly is good, but it misses the essential point. The important thing here isn’t the size, but rather the purpose, of government. We could have a cheap, small tyranny. After all our government spends most of its revenue on payments to individuals and foreign aid, neither of which is part of the tyrannical apparatus trying to keep us locked down and censored. What parts of the government would be necessary for a tyranny? It’d be a lot smaller than what we have now. We could shrink the government and nevertheless find it more tyrannical than it is today.

No, what we want is a limited government, limited not in size, but rather in scope. Limited, that is, in what it’s allowed to do. Under current circumstances, such a government would also be much smaller, but that’s a side effect. If we were in a World War II sort of war, an existential fight against nasty dictatorships on the brink of world conquest, that would be very expensive and would require a gargantuan government, but that would be what the government should be doing. That would be a large, but still limited government, since it’d be working to protect our rights.

World War II would have been the wrong time to squawk about “small government,” but it wasn’t (and never is) a bad time to demand limited government. Today would be a better time to ask for a small government–at least the job it should be doing is small today–but it misses the essential point; we want government to not do certain things. Many of those things we don’t want it doing are expensive but many of them are quite eminently doable by a smaller government than the one we have today. Small, but still exceeding proper limits.

So be careful what you ask for. You might get it and find you asked for the wrong thing.

Political Science In Summation

It’s really just a matter of people who can’t be happy unless they control others…versus those who want to be left alone. The oldest conflict within mankind. Government is necessary, but government attracts the assholes (a highly technical term for the control freaks).

His Truth?

Again we saw an instance of “It might be true for Billy, but it’s not true for Bob” logic this week.

I hear this often, and it’s usually harmless. As when it’s describing differing circumstances, not different facts. “Housing is unaffordable” can be true for one person, but not for another who makes ten times as much.

But sometimes the speaker means it literally. Something like 2+2=4 is asserted to be true for Billy but not for Bob. (And when it’s literal, it’s usually Bob saying it.) And in that sense, it’s nonsense, dangerous nonsense. There is ONE reality, and it exists independent of our desires and our perceptions. It would go on existing if we weren’t here. We exist in it. It does not exist in our heads. It’s not a personal construct, and it isn’t a social construct. If there were no society, reality would continue to be what it is, it wouldn’t vanish…which it would have to do, if it were a social construct.

Now what can change from person to person is the perception of reality. We see that all the time. And people will, of course, act on those perceptions. They will vote for Trump (or try to) if their perception is close to mine, and vote against Trump (and certainly succeed at doing so) if their perception is distant from mine (and therefore, if I do say so, wrong). I have heard people say “perception is reality” and usually, that’s what they’re trying to say–your perception of reality is, as far as you know, an accurate representation of reality, or you’d change it.

But I really wish they’d say it differently. And sometimes, to get back to Billy and Bob, the person who says they have different truths is really saying they have different perceptions of reality–different worldviews. I can’t argue with the latter. But I sure wish they’d say it better. That way I’d know that someone who blabbers about two different truths is delusional and not worth my time, at least not until he passes kindergarten-level metaphysics on his umpteenth attempt.

Lawyer Appeasement Section

OK now for the fine print.

This is the WQTH Daily Thread. You know the drill. There’s no Poltical correctness, but civility is a requirement. There are Important Guidelines,  here, with an addendum on 20191110.

We have a new board – called The U Tree – where people can take each other to the woodshed without fear of censorship or moderation.

And remember Wheatie’s Rules:

1. No food fights
2. No running with scissors.
3. If you bring snacks, bring enough for everyone.
4. Zeroth rule of gun safety: Don’t let the government get your guns.
5. Rule one of gun safety: The gun is always loaded.
5a. If you actually want the gun to be loaded, like because you’re checking out a bump in the night, then it’s empty.
6. Rule two of gun safety: Never point the gun at anything you’re not willing to destroy.
7. Rule three: Keep your finger off the trigger until ready to fire.
8. Rule the fourth: Be sure of your target and what is behind it.

(Hmm a few extras seem to have crept in.)

(Paper) Spot Prices

Kitco “Ask” prices. Last week:

Gold $2,720.80
Silver $33.78
Platinum $1,023.00
Palladium $1,106.00
Rhodium $5,100.00
FRNSI* 130.618-
Gold:Silver 80.545-

This week, 3PM Mountain Time, markets have closed for the weekend.

Gold $2,748.70
Silver $33.77
Platinum $1033.00
Palladium $1219.00
Rhodium $4,950.00
FRNSI* 131.968+
Gold:Silver 81.395-

Palladium went absolutely bananas Thursday and Friday rising 96 bucks the first day and 37 bucks the second. Platinum went up a whole eight bugs then down three. (Somebody, please go wake platinum the hell up.) Silver managed to drop one cent, while gold showed a modest increase. (As such, the gold:silver ratio has gone up.)

*The SteveInCO Federal Reserve Note Suckage Index (FRNSI) is a measure of how much the dollar has inflated. It’s the ratio of the current price of gold, to the number of dollars an ounce of fine gold made up when the dollar was defined as 25.8 grains of 0.900 gold. That worked out to an ounce being $20.67+71/387 of a cent. (Note gold wasn’t worth this much back then, thus much gold was $20.67 71/387ths. It’s a subtle distinction. One ounce of gold wasn’t worth $20.67 back then, it was $20.67.) Once this ratio is computed, 1 is subtracted from it so that the number is zero when the dollar is at its proper value, indicating zero suckage.

The Moon and Flat Earth

Let us examine what we should expect to see when observing the Moon, assuming the usual flat earth model is correct.

We’ll start with this standard diagram.

It’s difficult to tie down exact distances, because the Flat Earthers have yet to come up with a map (as opposed to a diagram) complete with a scale, but apparently the Moon is claimed to be about 3000 kilometers above the plane of the Earth. There’s no official notion what the diameter of the disc is, either, but one could say that the distance from the north pole (at the center of the disc) to the outer rim (corresponding to the globe earth south pole) is 20,000 km since that is very roughly the distance on the round earth (globers have no hesitation in publishing exact figures). Alternatively since the glober circumference of the earth along the equator is ~40,000 km, we could say that that is the distance that should be measured along the circle of the equator, which means (via dividing by 2 x pi) the distance from the center to the equator is 6366.2 km. From the pole to the equator is 1/4 of the total distance across the circle, so the diameter of the entire disk is 25,465 km. (Which is actually fairly close to the globe earth circumference when that is expressed in miles, by coincidence.)

The Moon varies in declination from 28.7 S to 28.7 N, or to translate that into non-astronomese, that’s as far north or south as it gets. The Sun, by contrast, stays between 23.44 degrees S and N. (In globe earth terms, that’s the Earth’s axial tilt.) Every flat earth model I’ve seen shows the Sun going around and around on a daily basis, following a circle that grows or shrinks according to the seasons, withing these bounds on the flat earth; likely also about 3000km above the Earth. I’m going to assume the Moon behaves similarly only within the 28.7 S to 28.7 N bounds.

Here is a picture of the Moon, when it is directly over the equator, in the Flat Earth model. (Screen shot taken off a youtube video.)

The Moon is regarded by most Flat Earthers as a sphere, with some minority thinking that it, too is some sort of disk. Whichever one it is, when you look at a full moon, you see something like this:

However, it may be tilted clockwise (near moonset) or counter-clockwise (at moonrise), in other words the orientation may be different. This is lunar north pole at the top so it should be close to what you see when the moon is directly south of you, which should happen at about midnight on a full moon, provided you’re north of the moon.

And therein lies the first problem.

What if you are south of the moon at that moment? Like, for instance, living in Australia or South Africa or South America?

If the flat earth is correct, you should see a good part of the other side of the moon (if it is a sphere), since you’ll be “behind” the moon compared to the guy to its north. Not exactly behind the moon, so there will be some overlap between what the two of you see. The person south of the moon, in other words, should see some features you cannot see, and vice versa.

On the other hand, if the Moon is a disk (apparently the minority opinion in the flat earth camp), then…well, there are two sub cases. If the moon is pasted to the firmament so that it faces “down” to the Earth, than only people directly under it will see the moon as a circle; anyone else will see it as elliptical. If (on the other hand) it happens to be face-on to the viewer in the northern hemisphere, anyone not on that line of sight should see it as elliptical, and if they’re far enough away, they may even be seeing the opposite face of the disk.

Yet we’ve never seen a photograph of the back side of the Moon taken from Earth’s surface, not even a partial one. Nor have we seen pictures with the Moon distorted into an elliptical shape because the photographers are not face-on to it. Yet effects like these must happen if the Moon is as close as is claimed.

Here’s another issue. If you’re inside the circle that the Moon traces every day, you will be closest to the moon when it is directly south of you; if you’re outside of that circle, you will be closest to the moon when it is directly north of you. If you are actually very close to the moon’s latitude, it should pass by almost directly overhead, and be nearest at that time. Closer to moonrise/moon set it should be much further away.

If it’s further away, it should look smaller. Yet tracking the moon across the sky shows no change in its apparent size, no matter where you are.

Interestingly, these same issues would arise on Globe Earth, if the Moon were this close to it. If you saw the moon looking like the picture I showed, someone far away would be able to see features that you can’t, on the other side of the Moon. So the mistake here is not with the shape of the Earth, but rather, with the notion that the Moon is nearby.

All of these issues resolve if the Moon is far away, compared to our baseline (40,000 km for Flat Earth, or 13,000 km for Globe Earth). If the Moon is far enough away, two people standing 40,000 km apart will see almost exactly the same features on a spherical Moon, with the differences being seen oblique near the edges of what we see, so those differences would be hard to even tell apart.

How far away? Aristarchus of Samos who lived from 310-230 BCE (approximately) was able to do a computation, and got a value of roughly 130,000 kilometers. Others, like Hipparchus and Ptolemy, got 425,000 and 376,000 kilometers, respectively.

If numbers like these are even remotely correct–and they must be at a bare minimum, because we do not see the effects we would see (regardless of the shape of the Earth) if the Moon were closer to Earth–then there’s now a new problem.

If the Moon is that far away, two different observers on a flat Earth should see it in almost exactly the same direction, both altitude and azimuth. [Altitude: the angle above the horizon, with 0 being on the horizon and 90 being overhead. Azimuth: the compass bearing of the object. Generally 0 is considered to be due north, 90 degrees is to the east, 180 to the south, 270 to the west, and 360 is also due north.] This is because it is so far away that shifting a few thousand kilometers should make little difference, like taking two steps sideways and noting that light pole at the other end of the parking lot only seems to shift a little compared to the buildings in the distance. A 40000 km shift (from one edge to the other) against a moon 300,000 km away should lead to an angular shift of about seven and a half degrees.

Yet at the same time. different people can see the Moon low in the east, and low in the west, a difference of almost 180 degrees! OK, that one can be explained on Flat Earth. If I’m in Colorado, west is the same direction as east would be in India (check the diagram). [Also true for globe earth, in three dimensions.] But what about when the Moon is overhead for me, and low to the horizon for someone else, at the same time? There’s no way to make that work, for a distant object, on a Flat Earth. And we’ve established that the Moon must be distant.

Well, there’s only one way to solve that problem. The ground itself that you are standing on, cannot be oriented in the same direction as the ground of that other observer. To try to visualize this, it’s easiest to deal with plumb bobs; the lay of the ground (if the ground is horizontal) is perpendicular to the plumb bob. So if “horizontal’ is the same thing in two different places, the plumb bobs will be perpendicular to the same thing and thus parallel to each other. This would be the case on Flat Earth. A line of sight to a distant moon would form nearly the same angle to both plumb bobs, instead of very different angles, which is what we actually observe.

Therefore horizontal in one place, is not oriented the same as horizontal in the other place. The Earth cannot be flat. (What shape it actually is can be determined by collecting information about the orientation of the moon from various locations, all at the same time.)

As a post script, the same reasoning works for the Sun as well…though you have to have the proper equipment to see sunspots, otherwise the Sun is just a featureless sphere and you cannot tell whether two people far apart are looking at two different sides of it or not.

Oilworld

I know of a world where it rains, there are mountains, hills, streams and rivers and lakes, all under a nice thick atmosphere–thick enough you could strap on wings and fly! Not the dessicated nearly-airless rocks of the inner solar system, the roasting dry hell that is Venus, the deep-frozen (or totally volcanic) Galilean moons, the bottomless atmospheres of the gas giants.

Comparatively speaking this is nearly paradise!

Perhaps I have a second calling for writing real estate ads. Because what I haven’t told you is that this place is a frigid 93 K (-290 F)…so cold that water is a rock, a hard one, never a liquid. Those mountains are largely made of ice. The streams and rivers and lakes? Liquid methane and ethane, in some ways a lot like gasoline, but gasoline would be frozen solid here. If one could feel this stuff it would probably feel oily, not wet. The atmosphere is almost pure nitrogen; even if it weren’t at that frigid temperature you’d pass out and die breathing it. And it’s so smoggy that you’d never see the shrunken sun, nor much of anything else in the night sky.

I speak, of course, of Saturn’s moon Titan, which orbits at 1,122,870 km. (Compare to the Earth-Moon distance of 384,399 km.) Despite being almost three times further, this is still close enough to Saturn that, if you could see Saturn through the smog it would be 11 1/2 times as wide as the moon. Titan is almost precisely in Saturn’s equatorial plane, however, so the rings would be almost perfectly edge on. The orbital period is 15.95 days. Here it is, seen from an Earth-based telescope, a dot to Saturn’s upper right.

To remind people of what I said in the Moon roundup, major moons (the ones that are round) come in three sizes, large (7 of them), medium (9 of them) and small (three of them), for a total of nineteen. There are also five non-rounded minor moons about the size of those small major moons, we can call these “big” small moons, well, big small moons, or maybe medium-small.

The seven large major moons are: our own Moon, Io, Europa, Ganymede, Callisto, Titan and Triton. Titan happens to be the second largest of the Big Ones. It’s just a bit smaller than Ganymede, and it’s thus the 10th largest object in the solar system (including the Sun); it’s larger than Mercury. This is the only large major moon that Saturn has, so Jupiter has it beat. Or does it? Saturn has four of the medium major moons (out of nine total), and two of the three small ones, for a total of seven major moons. And for the cherry on top, two of the big five unrounded moons are also here. But we’ll cover the medium and small stuff later; today we focus on Titan, which is arguably the most interesting of the large (and major) moons.

Titan was thought to be larger than Ganymede until relatively recently; it turned out that astronomers were measuring the light-impenetrable atmosphere, and that was enough to make the difference and fool astronomers for decades. An understandable error; this is the only moon with a significant atmosphere; more so than ours in many ways.

And yes, there’s more than enough air pressure to allow stable liquids to form. (The only other world like that in our solar system is the one you’re sitting on.) The atmosphere is four times as dense as ours, yet the pressure is “only” 1.45 times our atmospheric pressure. The difference being largely due to Titan’s much lower surface gravity of 13.8 percent of Earths (our Moon’s gravity is higher, actually.)

After the Pioneer and Voyager missions, we realized that there could be liquids on Titan’s surface. The Hubble Space Telescope was able to add to the speculation by detecting more strong evidence.

So we decided that the next time we sent something to Saturn, we’d take a closer look at Titan.

A much closer look. As in, actually touching it.

The Cassini probe, named after one of the two scientists who first studied Saturn in depth, brought with it the Huygens lander…named after the other of those two scientists, the one who discovered Titan. From 2004-2017 Cassini was able, in its copious spare time while studying Saturn, to map Titan with its penetrating radar, and Huygens actually landed on Titan on January 14, 2005.

Radar is needed, because this is what Titan would look like to human Mark I eyeballs, in true color, no enhancements, no false color:

The color is good old smog.

With near infrared (“near” meaning it’s infrared at frequencies close to visible light), you see this:

This feature was actually first seen by the Hubble Space Telescope in 1994, though Cassini got a better look starting in 2003. The dark area is apparently a dune sea! (No, no Shai Hulud. Sorry, Coothie.)

So here is a map put together in 2016, with a lot of official names for features (open in a new tab for a much more legible rendering):

It looks like a bit of a patchwork quilt because Cassini could only do sharp imaging on those occasions where it was flying by Titan; it wasn’t dedicated to studying Titan, so many areas are just shaded polygons, or just very blurry. (In fact Cassini divided its time between studying Saturn itself and 20 different moons.)

As with any map like this, you won’t get a decent notion of the two poles, so here they are. In case you haven’t gotten my subtle hints that this isn’t very good real estate (never mind the billion mile one-way commute) you can scout out properties on the original images at over 3000 pixels width.

And now what you’ve been waiting for: Huygens’ descent to Titan’s surface. This just-under-five-minute movie is a time lapse, showing you the fish-eye image sent as the probe descended. Look to the sides, though, and you will see graphics reporting time, angles to the Sun and Cassini, which sensors are seeing what at any given time, altitude information, scale information…this thing is loaded; many of you will want to watch it a couple of times.

And in case you didn’t want to watch that, here’s the contrast-enhanced picture from the surface:

(Now go back and watch the movie.) Those rocks are almost certainly water ice.

Huygens is the only probe we’ve ever landed on a body that remains entirely in the outer solar system.

OK, so on to a bit more technical content. Here’s a cutaway of Titan, somewhat hypothetical, much like the one I found for three of the Galilean satellites a few weeks ago:

And yes…another liquid water ocean deep down! But we’re not completely certain that this is the correct model; note that the diagram specifies which model it is, which it wouldn’t have to do if we were certain of it.

The atmosphere is responsible for the fact we can have liquids on Titan; here’s a diagram of its layers:

Nearer the surface, we have this cross section, reminiscent of some notional cross sections we see for Earth:

On earth we have aquifers the top of which are the water table, and a lake is basically where the water table is above the surface. But here we have…an “alkanofer”?!? What the heck is that about?

(Dragging out the organic chemistry skis. Not a soapbox, skis. As in, getting out over my…) Alkanes are a class of molecule consisting of nothing but hydrogen and carbon. Every carbon uses all four of its bonds to connect to distinct atoms. The simplest alkane is methane, with one carbon, connected to four hydrogens, CH4. The next one up is a pair of carbons, connected to each other by one bond (carbon can double or even triple bond, but those cases wouldn’t be alkanes). The other three bonds for each carbon is connected to a hydrogen, for a total of two carbons and six hydrogens, C2H6; this is ethane. You can add a third carbon to the chain, to get propane (C3H8), a fourth to get butane (C4H10)…but now there’s an additional complication. With four carbons, they could form a chain, or a T, with one carbon in the “middle” connected directly to three other carbons. Either configuration will connect to ten hydrogen atoms. The chain is butane, the T configuration is isobutane.

And if you allow rings of carbon atoms (technically molecules with rings aren’t called alkanes, but rather cycloalkanes), you can have up to six different variations, called isomers. Four of them are shown below. Though the ones with rings don’t connect to as many hydrogen atoms, in the lower left is cyclobutane and note there are only eight hydrogen atoms.

(And yes, propane has a ring form too, but the chain is the only possible three carbon alkane.)

You can go on, and the higher you go the more isomers are possible, and this number grows rapidly. Leaving out cyclo- type isomers, you have 2 isomers for 4 carbons, three isomers for 5 carbons, five for 6 carbons, nine for 7 carbons, 18 for 8 carbons, 35 and seventy five for 9 and 10 carbons, respectively…and when you get to 32 carbons, there are over 27 billion isomers…again, no rings.

One trend is that the longer the alkane, the higher its melting point. Hence we have butane which is a liquid on earth at 0 C, and at room temperature with just a little bit of pressure (like in cigarette lighters), pentane which is liquid up to 34 C, and so on. Gasoline is largely made up of alkanes and cycloalkanes with (roughly) eight or so carbon atoms in them.

At the low temperatures on Titan, only the smallest alkanes will be liquid, but that doesn’t mean bigger ones don’t exist as sand or other forms of solid matter. Imagine a world you could scrape frozen crude off the ground.

Titan should, perhaps, be thought of as “Oilworld.”

What would it be like to swim on Titan? Pretending that the cold and lack of oxygen wouldn’t kill you within seconds, these liquids aren’t very dense, so you’d sink to the bottom of the lake or pond. Your best strategy might be to leap out of the “water,” rather than try to swim.

Life?

For those speculating about life, Titan has some advantages. It certainly has plenty of carbon, and those alkanes make good feedstock for building more complex molecules (which is why, for instance there’s so much smog there). But that life would almost certainly have to exist in that subsurface ocean…and we’re not even sure that that ocean is there, yet. Anywhere else, it’s simply too cold.

On the other hand, its atmosphere resembles the atmosphere on Earth, back before cyanobacteria and plants started producing oxygen. It’s likely Titan would have something to teach us about pre-biotic chemistry.

Future Missions

In 2028 Dragonfly will launch, and in the mid 2030s it will arrive at Titan. It will be a flying drone, powered by radioisotope thermoelectric generator, i.e., the heat from a chunk of plutonium 238 (which literally glows red, it’s so hot from radioactivity). (https://en.wikipedia.org/wiki/Radioisotope_thermoelectric_generator). This is the way we power most of our probes to the outer solar system, however Juno and Europa Clipper did (and will) use large solar arrays (they have to be large because sunlight is very weak out there). Other unfunded ideas were for a hot air balloon, a probe that would float on one of the lakes, and even a submarine drone!

Titan is going to get a lot of attention in the future, that’s for sure.

2024·10·19 Joe Biden Didn’t Win Daily Thread

What is it that feeds our battle, yet starves our victory?

Speaker Johnson: A Reminder.

And MTG is there to help make it stick.

January 6 tapes. A good start…but then nothing.

Were you just hoping we’d be distracted by the first set and not notice?

Are you THAT kind of “Republican”?

Are you Kevin McCarthy lite?

What are you waiting for?

I have a personal interest in this issue.

And if you aren’t…what the hell is wrong with you?

Lawyer Appeasement Section

OK now for the fine print.

This is the WQTH Daily Thread. You know the drill. There’s no Poltical correctness, but civility is a requirement. There are Important Guidelines,  here, with an addendum on 20191110.

We have a new board – called The U Tree – where people can take each other to the woodshed without fear of censorship or moderation.

And remember Wheatie’s Rules:

1. No food fights
2. No running with scissors.
3. If you bring snacks, bring enough for everyone.
4. Zeroth rule of gun safety: Don’t let the government get your guns.
5. Rule one of gun safety: The gun is always loaded.
5a. If you actually want the gun to be loaded, like because you’re checking out a bump in the night, then it’s empty.
6. Rule two of gun safety: Never point the gun at anything you’re not willing to destroy.
7. Rule three: Keep your finger off the trigger until ready to fire.
8. Rule the fourth: Be sure of your target and what is behind it.

(Hmm a few extras seem to have crept in.)

Spot (i.e., paper) Prices

Last week:

Gold $2,657.70
Silver $31.60
Platinum $995.00
Palladium $1,088.00
Rhodium $5,075.00
FRNSI* 127.566+
Gold:Silver 84.104+

This week, 3PM Mountain Time, Kitco “ask” prices. Markets have closed for the weekend.

Gold $2,720.80
Silver $33.78
Platinum $1,023.00
Palladium $1,106.00
Rhodium $5,100.00
FRNSI* 130.618-
Gold:Silver 80.545-

The attention is on gold for bursting through the $2700 line. And the FRNSI is now over 130. At what point does it become worthwhile to simply wipe your butt with dollar bills rather than lugging them around in your wallet? (Honestly, though, they aren’t absorbent enough…so probably, never.)

As I said the attention is on gold…but silver should not be neglected! It has gone up over two dollars over the past week, and (net) almost all of that was on Friday after four days of almost no net movement. It went up $2.03 on Friday or 6.4 percent. (Versus gold going up 1.05 percent on Friday) And you can see the effect in the Gold:Silver ratio. In terms of silver, gold dropped over three and a half ounces.

Even platinum went up more on a percentage basis Friday than did gold.

*The SteveInCO Federal Reserve Note Suckage Index (FRNSI) is a measure of how much the dollar has inflated. It’s the ratio of the current price of gold, to the number of dollars an ounce of fine gold made up when the dollar was defined as 25.8 grains of 0.900 gold. That worked out to an ounce being $20.67+71/387 of a cent. (Note gold wasn’t worth this much back then, thus much gold was $20.67 71/387ths. It’s a subtle distinction. One ounce of gold wasn’t worth $20.67 back then, it was $20.67.) Once this ratio is computed, 1 is subtracted from it so that the number is zero when the dollar is at its proper value, indicating zero suckage.

Flat Earther Influencers are Mostly Lying Sacks of Shit

The Final Experiment continues to make waves in the Flat Earth Community.

I will link a relevant video below, but I’ll summarize here.

After years of happily saying that a 24 hour sun in Antarctica during southern summer (with it doing a 360 around the viewer over the course of a day) would disprove the Flat Earth viewpoint, but then saying “yeah but you can’t go to Antarctica” or flatly asserting that the sun does set in Antarctica, and furthermore that they’d love to go to Antarctica and see…

They’re for the most part refusing to go take a look. Everything from whining about how they’d have to deal with globe-earth “trolls” on the trip to…well, I don’t know what other rationales they have. There are three, maybe four going. (Four is if you count Candace Owens’ producer.)

Plenty of globe earthers are going, and at least a couple of them have vowed to take down their content and replace it with a video stating that the Earth is flat…if the sun sets during the five days they are at 79+ degrees south latitude.

Meanwhile other flerfers have begged the three that are going, not to go, or have already accused them of being shills. (Interesting. Before they even report back what they have seen, they are already bought off shills. Almost as if the accusers already know they will be reporting back that the Sun did not set!

One would think that if the flerfers are so confident of their position, they would positively relish the prospect of their final victory over the globers, as they point to the twighlight and say “So, Dave, where’s the sun?!?!” as they film McKeegan’s humiliation for their own channels!

That is how they would behave if they were really thinking of themselves as people with some special insight who have had their viewpoint put down and suppressed; they would love to have their day in the court of the brute fact that the sun went down in Antarctica during Antarctic summer.

Instead, with the exception of those who are actually going on the trip, they are acting like knowing con-men whose jig is about to be up.

Those reading this who have accepted the flerfer claims might just want to think about that. That should speak louder to you than all their shitty geometry, bogus astronomy, and physics claims which (let’s face it) should not have fooled any educated adult. The sad, blunt truth of the matter is that you have been suckered.

Flat Earthers are Desperately Dodging a Free Trip to Antarctica

No Science Post This Week (Sorry)

A lot of distractions this week.

2024·10·12 Joe Biden Didn’t Win Daily Thread

What is it that feeds our battle, yet starves our victory?

January 6 Tapes Reminder

After the first release, we were supposed to get more, every week.

As far as I know it hasn’t happened.

Speaker Johnson, please follow through!

A Caution

Just remember…we might replace the RINO candidates. (Or we might not. The record is mixed even though there is more MAGA than there used to be.) But that will make no difference in the long run if the party officials, basically the Rhonna McDaniels (or however that’s spelled–I suspect it’s RINO), don’t get replaced.

State party chairs, vice chairs, secretaries and so on, and the same at county levels, have huge influence on who ultimately gets nominated, and if these party wheelhorses are RINOs, they will work tirelessly to put their own pukey people on the ballot. In fact I’d not be surprised if some of our “MAGA” candidates are in fact, RINO plants, encouraged to run by the RINO party leadership when they realized that Lyn Cheney (and her ilk) were hopelessly compromised as effective candidates. The best way for them to deal with the opposition, of course, is to run it themselves.

Running good candidates is only HALF of the battle!

Biden Gives Us Too Much Credit

…we can move on to the next one.

Apparently Biden (or his puppeteer) has decided we’re to blame for all of the fail in the United States today.

Sorry to disappoint you Joe (or whoever), but you managed to do that all on your own; not only that, you wouldn’t let us NOT give you the chance because you insisted on cheating your way into power.

Yep, you-all are incompetent, and so proud of it you expect our applause for your sincerity. Fuck that!!

It wouldn’t be so bad, but you insist that everyone else have to share in your misery. Nope, can’t have anyone get out from under it. Somehow your grand vision only works if every single other person on earth is forced to go along. So much as ONE PERSON not going along is enough to make it all fail, apparently.

In engineering school we’re taught that a design that has seven to eight billion single points of failure…sucks.

Actually, we weren’t taught that. Because it would never have occurred to the professors to use such a ridiculous example.

Justice Must Be Done.

The prior election must be acknowledged as fraudulent, and steps must be taken to prosecute the fraudsters and restore integrity to the system.

Nothing else matters at this point. Talking about trying again in 2022 or 2024 is hopeless otherwise. Which is not to say one must never talk about this, but rather that one must account for this in ones planning; if fixing the fraud is not part of the plan, you have no plan.

Kamala Harris has a new nickname since she finally went west from DC to El Paso Texas: Westward Hoe.

Lawyer Appeasement Section

OK now for the fine print.

This is the WQTH Daily Thread. You know the drill. There’s no Poltical correctness, but civility is a requirement. There are Important Guidelines,  here, with an addendum on 20191110.

We have a new board – called The U Tree – where people can take each other to the woodshed without fear of censorship or moderation.

And remember Wheatie’s Rules:

1. No food fights
2. No running with scissors.
3. If you bring snacks, bring enough for everyone.
4. Zeroth rule of gun safety: Don’t let the government get your guns.
5. Rule one of gun safety: The gun is always loaded.
5a. If you actually want the gun to be loaded, like because you’re checking out a bump in the night, then it’s empty.
6. Rule two of gun safety: Never point the gun at anything you’re not willing to destroy.
7. Rule three: Keep your finger off the trigger until ready to fire.
8. Rule the fourth: Be sure of your target and what is behind it.

(Hmm a few extras seem to have crept in.)

Spot Prices

All prices are Kitco Ask, 3PM MT Friday (at that time the markets close for the weekend). (Note: most media quotes are for the bid…the price paid by the market makers, not the ask, which is what they will sell at. I figure the ask is more relevant to people like us who wish we could afford to buy these things. In the case of gold the difference is usually about a dollar, for the PGMs the spread is much wider.)

Last Week:

Gold $2,654.30
Silver $32.26
Platinum $999.00
Palladium $1,038.00
Rhodium $5,025.00
FRNSI* 127.402-
Gold:Silver 82.278+

This week, markets closed at 3PM Mountain Time Friday for the weekend.

Gold $2,657.70
Silver $31.60
Platinum $995.00
Palladium $1,088.00
Rhodium $5,075.00
FRNSI* 127.566+
Gold:Silver 84.104+

Gold see-sawed, getting closer to 2700, almost dipping below 2600 on Wednesday and Thursday but recovered nicely on Friday, even to the point of closing up for the week, barely. Silver, however, has definitely slipped, and you would need almost two more ounces of silver this week to buy an ounce of gold, than last week. Platinum a bit down, palladium might be starting another run.

*The SteveInCO Federal Reserve Note Suckage Index (FRNSI) is a measure of how much the dollar has inflated. It’s the ratio of the current price of gold, to the number of dollars an ounce of fine gold made up when the dollar was defined as 25.8 grains of 0.900 gold. That worked out to an ounce being $20.67+71/387 of a cent. (Note gold wasn’t worth this much back then, thus much gold was $20.67 71/387ths. It’s a subtle distinction. One ounce of gold wasn’t worth $20.67 back then, it was $20.67.) Once this ratio is computed, 1 is subtracted from it so that the number is zero when the dollar is at its proper value, indicating zero suckage.

Moon Roundup

Before 1610, there was one Moon, and it wasn’t a class of objects. Actually at one time the Moon and Sun (!) were lumped in with Mercury, Venus, Mars, Jupiter and Saturn as planets. They were, after all, all objects that moved with respect to the background stars (that includes the Sun but it takes a little bit of extra work to show this since it’s rather difficult to see the stars and Sun at the same time). And planet derives from a Greek word for wanderer.

Note by the way that Earth was not considered a planet. Planets were things up there in the sky, not down here, and certainly not as “down here” as you can get, the dirt beneath your feet.

This was back in the old “Earth is the center of everything” days, but late in the 1500s some people started suggesting that perhaps it was the Sun at the center. (This was actually a revival of an ancient Greek idea.) Now this is difficult to settle with naked eye observations, but a telescope will show you that not everything goes around the Earth. Venus and Mercury exhibit phases that show they orbit the Sun. And Jupiter, of course, has those Galilean moons.

Galileo actually considered them planets at first, because, after all, they moved against the background stars, just like Jupiter did. He didn’t realize we needed a new category of thing, with the Moon being the first known member. And it took a while; for a couple of centuries the larger moons of the outer planets were called “satellite planets” instead of “moons” or just plain “satellites.”

So if you think Pluto being demoted from planet status was a kerfuffle, imagine what was going on then, when they still couldn’t figure out which buckets even existed that they could put things into (figuratively speaking of course).

Eventually anything that orbited the Sun was a planet, including Earth, and anything that orbited a planet was a satellite or moon, including “the” Moon. We know of no cases of a moon itself having a natural satellite of any significant size.

And yes, “satellite” used to be synonymous with “moon,” but then we started putting things in orbit, and we started talking about natural and artificial satellites. Some people still do so, but most people use “moon” (with a lower case M) for the natural case and just plain “satellite” for the artificial case.

[And yes, we’ve no idea how to classify Stacy Abram’s hindquarters. It’s a moon…sort of…and is of similar size to the major moons, but it’s not a heavenly body by any stretch of the imagination.]

Since those days, of course, we’ve found objects out there of all kinds of different sizes orbiting both planets and the Sun, so we had to sit down and reassess definitions again and Pluto got the boot from the “planet” clique. (And, IMHO, rightly so; the other alternative would have been to promote about half a dozen Kuiper belt objects.) There’s no minimum size, as yet, for moons, so technically any planet with a ring has countless moons: all the constituent rocks that make up the ring.

Anyhow, we’re not even halfway through the moons that are in our solar system. But I thought I’d do a quick roundup, to set up the Big Picture. Let’s start out with a picture from Wikipedia showing planets and large (or famous) moons, all to scale by size. Notably, Mercury and Mars look roughly the size of some of the bigger moons, and Pluto is outclassed by at least seven moons.

Let’s consider them in order of size. If you ignore the planets and Pluto, there seem to be seven “big ones,” and a bunch of medium sized ones.

The big ones are The Moon, Io, Europa, Ganymede, Callisto (all orbiting Jupiter), Titan (Saturn), and Triton (Neptune). They are all 2500 km across or larger. There seems to be a big gap between Triton and any of the moons smaller than it, and when you look at masses, that is confirmed. Triton, the smallest of these seven, is more massive than all of the other moons put together. So you could actually make a list with eight entries, the eighth being “everything else that’s a moon, put together” and that would be the last item on the list.

That makes it seem like a nice, natural dividing line between “large” and “medium.”

The large moons verge on being planet sized, with Ganymede more voluminous than Mercury (though made of much lighter stuff). So much so that at least some astronomers call these seven the “satellite planets.” (I.e., things that would be planets, if only they weren’t orbiting a planet!) [As an aside I suspect we’ll be looking, again, at reclassifying things soon. And I would not be entirely unsympathetic.]

Now just eyeballing that diagram again, there are nine moons in the “medium” bracket (with S for Saturn, U for Uranus, and P for Pluto): Titania (U), Oberon (U), Rhea (S), Iapetus (S), Charon (P), Ariel (U), Umbriel (U), Dione (S), and Tethys (S). And again, it turns out that Tethys, the smallest of the nine, is bigger than all of the remaining “small” moons, put together. So, another natural dividing line, between medium and small. These medium moons are all 1000-2500 kilometers in diameter.

Up to here, moons seem to be named after mythical figures, however for some reason the moons of Uranus got named after Shakespearean characters.

So that’s sixteen medium and large size moons. Everything else is “small.”

But there’s another criterion we could use…and that’s “hydrostatic equilibrium” which when you dumb it down means “is it spherical”?

If you don’t dumb it down, there are nuances. For instance, if a moon is orbiting fairly close to a planet when it’s still largely molten, it’s going to take on an oblate shape, first because it’s rotating once per orbit, and second because the planet’s going to tend to make it egg shaped (tidal forces). If it then solidifies and its orbit gets larger, it’s technically not quite in hydrostatic equilibrium any more; because if it were liquid it would flow into a slightly different shape. Our own moon is actually an example. But in general, for classification purposes, this is a nuance that is ignored; the sucker is round or it isn’t.

[Edited to add:] A moon in hydrostatic equilibrium is considered to be a “major moon,” no matter how small it might be.

[Edited:] All of the large and medium moons are major moons. But as happens, three (maybe four) of the biggest “small” moons, those below 1000km across but greater than 250 km across, are round too and also qualify as major moons. There are two moons in the 500-1000 km range, and seven in the 250-500 km range. I’m going to call the 250-1000 km range the “medium small” range.

[Edited:] In the 500-1000 km range, we have Enceladus (S) barely making it at 504 km, and definitely a major moon. There is also Dysnomia, a satellite of the dwarf planet Eris, which is the “maybe” case. It’s 615 km across, apparently, but it’s very dark and we cannot get a read on its shape though its density appears to be low enough that we don’t expect its gravity will have crushed it into a sphere.

[Edited:] in the 250-500 km range we have Mimas (S), and Miranda (U), 400 and 470 km in diameter respectively, both major moons. And we also have five objects that are not major moons, and they are Hyperion (S), Proteus (N), Nereid (N), Vanth (satellite of dwarf planet Orcus) and Hi’iaka (satellite of dwarf planet Haumea). Proteus is actually bigger than Mimas, so there’s clearly not a hard line, above which a moon will be round (and therefore major). As I alluded to above, a low density can make a moon less massive, which can be enough that it does not “go round.”

[Edited:] So there’s your roundup. Expect to see talk of Large, Medium and Medium-small moons, as well as major moons and minor moons; “major” encompassing large and medium moons as well as three of the scores of small moons.

Saturn

History

Saturn, to the ancients, was a star-like object that took 29.5 years to make one trip around the ecliptic. Dimmer and slower than Jupiter, which was associated with the king of the gods, it got associated with the prior generation.

You see, in Greek and Roman mythology the Olympian gods were the third generation. The first was Uranus (Οὐρανός), the sky, and Gaia, the Earth. He was both her son and her husband. Their children were the titans, twelve of them: Oceanus, Coeus, Crius, Hyperion, Iapetus, Theia, Rhea, Themis, Mnemosyne, Phoebe, Tethys, and Cronus. (You will see some of those names again…in fact if you read the previous section, you already have.) Cronus (or Kronos) was the father of Zeus, Hera, Poseidon, Hades, Hestia, Demeter and Chiron. These are all the Greek names. The one called Kronos was known to the Romans as Saturn.

In 1610 Galileo turned that telescope towards Saturn, and saw…well, a couple of lumps one on each side of Saturn that each looked like it might be a moon a third the size of Saturn. (Let’s face it, it wasn’t a very good telescope, even if it was one of the best in the world at the time.)

A couple of years later, he looked again, and the moons were gone. He predicted that they would be back later, and indeed they showed up. And got bigger to the point where Saturn seemed oval-shaped. Christiaan Huygens finally saw this as rings in 1655, publishing his results in 1659. Huygens spotted one moon, which he named Titan. Shortly thereafter (1675) Giovanni Domenico Cassini discovered a gap in the rings, and also four more moons, Iapetus, Rhea, Tethys and Dione–all named after titans. (Dione is either another daughter of Uranus and Gaia, or the daughter of Oceanus and Tethys, depending on whose rendering of the mythology you’re reading.) In 1789 William Herschel (discoverer of Uranus) discovered two more moons, Mimas and Enceladus–these are two of the three “small” moons in our solar system that are nevertheless big enough to be round, from the previous section. Hyperion was discovered in 1848. It’s comparable to Mimas and Enceladus, but not round…far from it, as we’ll see.

Saturn ends up having seven major moons, one large, the other six medium. Add in Hyperion, and that’s eight. When I was a kid, the count was ten (with most books still saying nine). The missing two were Phoebe (1898) and..well..number ten, first spotted in 1966, was a bit confusing. It was first spotted on December 15, 1966. But then another astronomer spotted it again…but in a different place in the same orbit…on December 18, 1966. Here was a moon that appeared to be jumping around in its orbit, but it was there (well, maybe not) and it was number 10. Finally in 1978, a couple of astronomers realized what was really going on. There were two moons sharing the same orbit, Janus and Epimetheus, a situation which had been assumed to be unstable up until then. So elementary school Steve didn’t realize Saturn’s tenth moon was really the tenth and eleventh moons. Today’s count is (drumroll) one hundred and forty six, with the most recent discovery being in 2020. But I am going to save detailed discussion of the moons until next time.

Pioneer 11 flew by in 1979. Voyager 1 zipped by in 1980, and Voyager 2 followed it in 1981. What a nice little barrage, especially since the cameras on the Voyagers were so much better. After that nothing until 2004, when Cassini went into orbit around Saturn. It not only stayed there for 13 years (until we deliberately deorbited it into Saturn’s atmosphere, since it was about to die anyway), it even put a lander on Titan! The ONLY landing ever made beyond the asteroid belt.

The Planet Proper

Saturn itself orbits at an average distance of 1,434 million kilometers, nearly a billion and a half. That’s 9.58 AUs. It has an axial tilt of about 28 degrees, a bit more than Earth’s 23 degrees, so Saturn definitely has seasons, unlike Jupiter (whose axial tilt is about 2 degrees). This will turn out to be important when we finally quit fiddling around and talk about the rings.

Saturn has a magnetosphere, like Jupiter, Ganymede, and Earth. Unlike Jupiter and Earth, the Saturn “magnet” is aligned with the axis of rotation pretty well. This magnetosphere isn’t as strong as Jupiter’s, but still significant.

Measured across the equator, Saturn is as wide as 9 earths. Measured through the poles, on the other hand, it’s only 8 earths tall. That’s because it is spinning very rapidly, once in about 10 1/2 hours, and it’s fluid clear down to a solid core that’s about 16,000 km across. We were able to learn a LOT about Saturn’s interior just from monitoring its gravity’s effect on both the Cassini probe and the rings.

Saturn has a banded atmosphere much like Jupiter’s though not nearly as colorful. It doesn’t have a long-standing storm like the Great Red Spot, but from time to time white spots will appear. Great white spots tend to appear once every Saturnian year, during its northern hemisphere summer, the last one in 1990. Cassini got to see one form, stretch out along its band, and eventually dissipate, after the head of the thing caught up and passed its tail. And then in 2010, ten years early, we got another white spot.

Voyager 1 spotted something very peculiar around Saturn’s north pole. For some reason we don’t fully understand, the clouds there form a hexagon, which appears to rotate with the planet, in time with Saturn’s radio emissions.

The south pole, by contrast, shows something like a hurricane eyewall. (No word yet on whether this is where all the FEMA hurricane money goes.)

OK, with that out of the way…

The Rings

They have been called “Gravity’s Masterpiece.”

And that is an understatement.

Gravity created them, gravity maintains their structure, and gravity is slowly destroying them.

Galileo noticed change when looking at Saturn, but could not resolve the rings; his telescope was simply too small. That change is caused by Saturn’s seasons. When it’s northern hemisphere summer, the north surface of the rings is tilted toward the Sun, at autumn they are edge on, at northern winter, the south surface is tipped toward the Sun, and finally at northern spring, they are edge on again. And since, comparatively speaking, we’re quite close to the Sun, we see the same thing. Here is a twenty nine year time lapse:

The rings are thin. At the time the earth crosses through the plane of the rings, we can’t see anything, not even a thin line. It has been likened to looking at a sheet of paper edge on, but relatively speaking the sheet of paper is much too thick! The next “disapperance” is next year, right now it looks something like this:

The rings are skinny but definitely there.

The rings are themselves subdivided into seven sections, imaginitively named A, B, C, D, E, F, and G.

What we see through our telescopes are basically A, B, and C. This is typically what you’ll see…only it’s much smaller in the telescope field of view than this:

This picture (from Cassini) shows the rings from well above the plane, with Saturn itself casting a shadow on them.

Going form the outside in, there’s a medium-bright ring (A), a wide gap–the one noted by Cassini, a brighter ring (B), and a much fainter ring (C). There are other, smaller gaps as well. Where do they come from? The Cassini gap happens to be at that spot where, if something were orbiting there, it’d do so in a 2:1 resonance with Mimas. That causes enough instability to force objects into smaller or larger orbits. In other cases, small moons within the rings help clear things out.

That’s just the beginning of the crazy stuff that happens in the rings. Ripples one to two kilometers high raised by embedded moons, spokes on the B ring we can’t figure out (yet)…some scientists are spending their entire careers on this stuff!

To see the D through G rings readily, we must look at Saturn backlit…something we couldn’t do until we sent spacecraft there.

By the way, if you right click and open in new tab, between the two “gray” fuzzy rings (a narrow one and a broad one) at about 4 oclock…that dot there is Earth.

The rings appear to be made of chunks of ice, averaging about a foot across. And they’re pretty bright; they haven’t been covered with dark space dust. That leads most scientists to think that they aren’t that old…150 million years at the most. It’s possible that they weren’t there when the non-avian dinosaurs were killed 66 million years ago.

The most common thought is that a medium-sized moon got too close to Saturn somehow, perhaps thanks to perturbations from the other moons, and tidal forces (yes tidal forces again) did the rest.

Picture this: a spherical body maybe 200 kilometers across in orbit. It will orbit as if the entire mass of the moon were concentrated at the center. But a rock at the far side of the moon is 100 kilometers further away, and one at the near side is 100 kilometers closer. An object 100 km further out, in order to stay in orbit, wants to move slower than this moon is orbiting, yet that rock is being forced to move faster than that, since it’s stuck to the moon. If the moon were to suddenly disappear and leave the rock behind, it would actually go into a new, elliptical orbit, with the closest part where the rock was, sitting on the moon, and the furthest part, oh, some distance away. And so, this is what the rock “wants” to do. It actually feels a slight tug pulling at it, off the surface of the moon. If the moon is close enough to the planet, and its gravity weak enough, the rock will actually feel no net attraction to the moon, and drift off. As will its neighboring rocks. And similar things happen on the side of the moon closest to the planet, they want to go into smaller orbits and feel a net tug toward the planet and off the moon.

That’s how loose rocks might peel off, but moons are generally solid, aren’t they? Sure. But, if you think about that orbit where things on the far side will just barely want to drift away, but put the moon closer, then something deep underground at the far side would (if it weren’t buried) drift away. Now bury it again. Everything above it wants to drift away too. Those miles of stuff are effectively “hanging” wanting to fall off the moon. Enough of that, and even a solid rock will fracture. Rocks don’t do too well under tension, a fact which has had a profound effect on architecture here on Earth.

So, basically, we think a mostly-icy moon got too close and shattered. And the tidal forces have kept it from reforming. However some suggest that instead, two moons collided and this is the debris from the collision.

The rings are dying, though. The ice is slowly sublimating with help from cosmic rays, and that ice ends up in Saturn’s magnetic field and eventually forms auroras in its atmosphere. There are also other forces causing ring material to rain down onto Saturn’s equator (this was discovered by the Cassini spacecraft). The rings have 10-100 million years to live at the rate they are losing mass.

I’ll close this with another picture:

..or two, just to see the aurora…

..or three (you can see the hexagon in this one).

Obviously I could go on. But some of the coolest stuff is on the moons. So…until next time!