Signs of Planet X... um, IX

Here's the paper:
Abstract

Recent analyses have shown that distant orbits within the scattered disk population of the Kuiper Belt exhibit an unexpected clustering in their respective arguments of perihelion. While several hypotheses have been put forward to explain this alignment, to date, a theoretical model that can successfully account for the observations remains elusive. In this work we show that the orbits of distant Kuiper Belt objects (KBOs) cluster not only in argument of perihelion, but also in physical space. We demonstrate that the perihelion positions and orbital planes of the objects are tightly confined and that such a clustering has only a probability of 0.007% to be due to chance, thus requiring a dynamical origin. We find that the observed orbital alignment can be maintained by a distant eccentric planet with mass gsim10 m⊕ whose orbit lies in approximately the same plane as those of the distant KBOs, but whose perihelion is 180° away from the perihelia of the minor bodies. In addition to accounting for the observed orbital alignment, the existence of such a planet naturally explains the presence of high-perihelion Sedna-like objects, as well as the known collection of high semimajor axis objects with inclinations between 60° and 150° whose origin was previously unclear. Continued analysis of both distant and highly inclined outer solar system objects provides the opportunity for testing our hypothesis as well as further constraining the orbital elements and mass of the distant planet.



New York Times: Ninth Planet May Exist in Solar System Beyond Pluto, Scientists Report

[...]

"We are pretty sure there's one out there," said Michael E. Brown, a professor of planetary astronomy at the California Institute of Technology.

What Dr. Brown and a fellow Caltech professor, Konstantin Batygin, have not done is actually find that planet, so it would be premature to revise mnemonics of the planets just yet.

Rather, in a paper published Wednesday in The Astronomical Journal, Dr. Brown and Dr. Batygin lay out a detailed circumstantial argument for the planet's existence in what astronomers have observed — a half-dozen small bodies in distant, highly elliptical orbits.

What is striking, the scientists said, is that the orbits of all six loop outward in the same quadrant of the solar system and are tilted at about the same angle. The odds of that happening by chance are about 1 in 14,000, Dr. Batygin said.

[...]

First, they focused on the six objects in stable orbits and disregarded objects that had been recently flung out by Neptune to eventually depart the solar system.

That made the picture clearer.

"What we realized is the story is much more simple and more fundamental," Dr. Batygin said. "They all point into the same overall direction. All in same quadrant. This is in stark contrast with the rest of the Kuiper belt."

Besides the long odds of this alignment being coincidental, Dr. Batygin said, this pattern would not last indefinitely, dispersing over a few hundred million years — a short time compared to the 4.5 billion-year age of the solar system.

"We're not observing a relic of a perturbation of the past," he said.

That argued for something else, something bigger, that is currently guiding Sedna and the others.

Dr. Batygin, a theorist, tried placing a planet among the six objects. That did scatter some of the Kuiper belt objects, but the orbits were not sufficiently eccentric.

Then he examined what would happen if a ninth planet were looping outward in a direction opposite to Sedna and the others. That, Dr. Batygin said, gave "a beautiful match to the real data."

The computer simulations showed that the planet swept up the Kuiper belt objects and placed them only temporarily in the elliptical orbits. Come back in half a billion years, Dr. Brown said, and Sedna will be back in the Kuiper belt, while other Kuiper belt objects will have been swept into similar elliptical orbits.

Another strange result in the simulations: A few Kuiper belt objects were knocked into orbits perpendicular to the plane of planetary orbits. Dr. Brown remembered that five objects had been found in perpendicular orbits.

"They're exactly where we predicted them to be," Dr. Brown said. "That's when my jaw hit my floor. I think this is actually right."

Dr. Trujillo said the new paper made a much more convincing argument for another planet than his own did. "We're pleasantly surprised that someone has really done a much better job than we did," he said.
 
More planet! Whatever the mass is meant to be for it, I can't tell. "gsim10 m⊕", anyone?
 
Yaaaaaay. Finally, nine planets again!

Once we find the damn thing, since it's a body slightly bigger than earth out in the outer kupiter belt to inner oort cloud.

Um, if they can calculate where the planet is, why don't they point a telescope at it?

Pics or it didn't happen.

There's this concept we like to call 'Space is Big'. We're hunting for what is probably an earth to super-earth sized object in an area the size of the entire solar system within Neptune's orbit, with little reflective radiation at that distance to make it shine, and cold enough to be able to hide from WISE. We'll find it, but that doesn't make it EASY to find. Hell, for all we know New Horizons will run right into it.
 
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So I skipped most of this because I maybe understood 1 in 5 of these words. Math has never been my strong suit.

What exactly is the edge of our solar system anyway? I was under the vague impression that a little ways past Pluto was the boundary line.
 
So I skipped most of this because I maybe understood 1 in 5 of these words. Math has never been my strong suit.

What exactly is the edge of our solar system anyway? I was under the vague impression that a little ways past Pluto was the boundary line.

Ahhahahahahaahahaha--no.

Pluto is the innermost major object of what is known as the 'Kupiter Belt'. A giant disk collection of bigass iceballs the same size as it that never quite formed into gas giants. This extends about another 50-ish AU out (say, the same distance as from the sun to Pluto) before a sudden dropoff from the resonace from the gas giants and this potential new planet.

Beyond that is the oort cloud, which is basically a 2 lightyear across cloud of comets in orbit around the sun. Eris and Sedna are members of this that migrated closer in. This is the absolute edge of the sun's influence. Though there is also the heliopause, where the solar wind gets blown away by the interstellar wind, and that's a whole other kettle of 'what in the hell'.
 
Ahhahahahahaahahaha--no.

Pluto is the innermost major object of what is known as the 'Kupiter Belt'. A giant disk collection of bigass iceballs the same size as it that never quite formed into gas giants. This extends about another 50-ish AU out (say, the same distance as from the sun to Pluto) before a sudden dropoff from the resonace from the gas giants and this potential new planet.

Beyond that is the oort cloud, which is basically a 2 lightyear across cloud of comets in orbit around the sun. Eris and Sedna are members of this that migrated closer in. This is the absolute edge of the sun's influence. Though there is also the heliopause, where the solar wind gets blown away by the interstellar wind, and that's a whole other kettle of 'what in the hell'.

You didn't have to laugh. My fragile internet feelings are hurt. :(

...I should have realized. It's called solar system for a reason. The boundary is past the edge of the sun's influence on the celestial bodies surrounding it?
 
You didn't have to laugh. My fragile internet feelings are hurt. :(

...I should have realized. It's called solar system for a reason. The boundary is past the edge of the sun's influence on the celestial bodies surrounding it?

'That depends' is honestly the most solid answer you'll get on where the Solar System ends. There's a lot of factors involved.
 
The boundary is past the edge of the sun's influence on the celestial bodies surrounding it?
...No? If the Sun weren't influencing them by way of gravity, those bodies couldn't well orbit around the sun, no? The heliopause is where the heliosphere ends, basically the region where the solar winds dominate against interstellar matter. But the Sun's gravity reaches further out. However, there is no clearly set border to that influence. Even nearby stars influence each other with gravity. I suppose the most pragmatical boundary for the extent of the solar system would be the orbit of the most distant object still consistently orbiting the Sun.... i.e., so far we absolutely can't tell :p As Richardson says, the estimate is that there is that Oort Cloud extending 0.9-1.9ly (50k-100k AU) out... which yes, is a very imprecise estimation.
 
Many machines on Ix. New Machines.


Better than those on Richese.
 
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That sign is the sign for Earth. So I think they mean... around 10 Earth masses? At least 10 Earth masses? I have no idea what gsim means to be honest.
The actual theory is that the planet is between five and fifteen Earth masses, so they went with ten because it's right between them.
6 whole data points? Good luck with those numbers. Hopefully, the telescope finds something.
Yeah, they apparently whittled down to six objects from twelve, so...
 
Um, if they can calculate where the planet is, why don't they point a telescope at it?
They can't do that. It's just as they say in the abstract: the evidence is that orbits of the Kuiper belt objects are (based on their modelling) unlikely to have come about by chance, but could have been a result of some massive body perturbing the orbits.

That sign is the sign for Earth. So I think they mean... around 10 Earth masses? At least 10 Earth masses? I have no idea what gsim means to be honest.
The usual LaTeX code for a ≳ symbol defined by AMS math packages is \gtrsim, from 'greater' and ∼ being \sim. It's safe to assume that this is just a shortened variant, esp. since that's what it looks like in the original abstract.


The actual theory is that the planet is between five and fifteen Earth masses, so they went with ten because it's right between them.

No; the reason is that it's just an order of magnitude. They also modelled 0.1 M⊕​ and 1.0 M⊕​ masses as well to see how they did in explaining the clustering of the Kuiper belt objects, for example. The results aren't anywhere near as precise as to claim 5-15.
 
Um, if they can calculate where the planet is, why don't they point a telescope at it?

Pics or it didn't happen.
Well, if you wanna take a shot at getting your name in the history books, here's a map on where to look.

The biggest unexplored territory is where, statistically, it is most likely to be: near aphelion. Sadly, aphelion is also very close to the Milky Way galaxy. Ugh.

So where is it? Probably distant. 500 AU+. Probably fainter than 22nd magnitude. Very possibly in the middle of the Milky Way galaxy.

Now go find planet nine.
 
More planet! Whatever the mass is meant to be for it, I can't tell. "gsim10 m⊕", anyone?

Greater than approximately 10 Earth masses (i.e. ice giant range, a triplet with Uranus/Neptune).

Um, if they can calculate where the planet is, why don't they point a telescope at it?

Pics or it didn't happen.

They can't. They said in the paper that they don't have enough data to fix the parameters.

So I skipped most of this because I maybe understood 1 in 5 of these words. Math has never been my strong suit.

What exactly is the edge of our solar system anyway? I was under the vague impression that a little ways past Pluto was the boundary line.

It doesn't really have a well-defined "edge". Beyond Neptune's orbit at 30 AU (1 AU is the distance from the Earth to the Sun) there's the Kuiper belt at 30-50 AU, which is sort of like the main asteroid belt except colder (so there's more icy bodies) and dominated by interactions with Neptune rather than Jupiter like the main belt. Then you have the scattered disk, which is composed of objects with significant inclinations (their orbits are tilted relative to the plane of the Solar System) and eccentricities (their orbits are highly elliptical), so that while their perihelia (closest approaches to the Sun) overlap the Kuiper belt in physical space their aphelia (far end of their orbits) are much further out at 100 AU or so. Sedna, a body that's puzzled astronomers for a while and one of the six bodies this paper is trying to explain, loops between 76 and about 900 AU, which is considered beyond the scattered disc.

The Sun's stellar wind starts to slow down around 80-90 AU (the termination shock, defined as the transition from supersonic to subsonic motion) and completely runs out of puff (because it's pushing against the interstellar medium) around 120 AU or so.

Of course, as stars are a LONG way from each other, Sol's actual gravitational influence extends far beyond that. The Oort cloud (the debris only vaguely bound to the Sun that's thought to be the origin of long-period comets) is thought to extend out to about a light-year, which is 63,000 AU.
 
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Scientists Find Hints Of A Giant, Hidden Planet In Our Solar System

The first suggestion that something big might be affecting the orbits of distant, icy bodies came in 2014. An international team of astronomers announced that they'd discovered a new dwarf planet, nicknamed Biden, that stays even farther out than Sedna. They also noted a strange clustering in the orbits of these objects, and in the orbits of about a dozen others. Perhaps, they hypothesized, the gravity of some unseen planet was acting as a shepherd.

"They were pointing out that there was something funny going on in the outer solar system, but nobody could really understand what it was," says Brown. "Ever since they pointed it out we've been scratching our heads."

The idea of a huge, hidden planet seemed kind of crazy. "No one really took it very seriously," says Brown. "It was ignored more than you might guess."

But he walked a few doors down to meet with Batygin and suggested they take this on. As they studied the freaky way that these objects lined up in space, Brown says, they realized that "the only way to get these objects to line up in one direction is to have a massive planet lined up in the other direction."

What's more, this planet naturally explains why the dwarf planets Sedna and Biden have weird orbits that never let them come in close to the solar system. "This wasn't something we were setting out to explain," says Brown. "This is something that just popped out of the theory."

But there was one moment that turned Brown into a believer. Their computer simulations predicted that if this hypothetical planet existed, it would twist the orbits of other small bodies in a certain way. So Brown looked through some old data to see if any icy bodies had been discovered with those kinds of orbits — and, lo and behold, he found five of them.

"They're objects that nobody has really explained or tried to explain before," says Brown. "My jaw hit the floor. That just came out of the blue. Being able to make a prediction and having it come true in five minutes is about as fun as it gets in science."

Their work suggests how big the planet must be, and more or less where it could be found. Brown has already started looking. He hopes other scientists will too.

"I want to know what it's like. I want to see that it's really there," says Brown. "It will hurt when somebody finds it and it's not me — but I assume it's going to happen, and I'm willing to feel that pain."

Caltech astronomers Mike Brown (left) and Konstantin Batygin are "willing to take bets" that a giant ninth planet is lurking in our solar system — way, way out, beyond Neptune.
Lance Hayashida/Courtesy of Caltech

It may be hard to believe that something so big would not have been seen before now. But Scott Sheppard of the Carnegie Institution for Science explains that for us to see it, sunlight has to travel all the way out there, bounce off the object, then travel all the way back.

"Objects get very faint very fast," says Sheppard. "If you do the math, if you move something twice as far away from the sun, it gets 16 times fainter."
Sheppard is one of the researchers who, after discovering Biden and the strange orbits, suggested a large planet might be the culprit.

"What we published was a very basic analysis of this clustering of objects in the outer solar system," he says. "We just did some basic stuff."

The new analysis, he says, has gone much deeper and has more rigor. "It leaves me thinking that the possibility of there being this super-Earth or mini-Neptune out there is more and more real now," says Sheppard.

Still, he's not completely convinced. "We really need to find more of these objects — more of these small objects that can lead us to the bigger object," Sheppard says. "I think it's still a tossup if it's really out there or not. I think we just need more data. Hopefully within the next few years we'll really be able to nail this down."

Dwarf planets like Sedna and Biden are not exactly household names. But Sheppard says if the solar system indeed has an honest-to-goodness ninth planet — a distant, giant planet that's bigger than Earth — "that, I think, is something that would blow the mind of anyone here on Earth."
That's cool.
 
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