How A “Dwarf Planet” Gas Giant Could Challenge IAU Definition

| October 12, 2017 | 0 Comments


Ethan Siegel has just written an article, “The Science Has Spoken: Pluto Will Never Be A Planet Again” , so this is a response to it. I’ll argue that far from “story over”, actually we could make a discovery tomorrow that would turn the whole thing on its head and make their definition untenable.  This will become particularly acute if we ever find a gas giant in the outer reaches of our solar system, too far away to clear its orbit. And we could find such a planet. The WISE survey only ruled out Saturn sized planets out to 10,000 AU and Jupiter sized ones out to 26,000 au . We could have gas giants that orbit our sun over 1.5 light years away, or over 100,000 au. For consistency, we would have to call it a “Gas Giant Dwarf Planet Non Planet”. To explain why, first, here is the graph from his article which he uses to show the neat division between large planets that clear their neighbourhood and small ones that don’t. But I’ve extended it to a light year, and let’s use Alan Stern’s terminology – let’s call an orbit clearing planet an “uber planet” and one that doesn’t, an “unter planet”:

The vertical axis shows its mass in Earth masses. Full size image here .
The three lines here show three possible definitions for the IAU planet, or uber planet. As he points out, there’s a clear division between the IAU planets, or “uber planets” as I will call them in this article and the unter planets. The unter planets are all much smaller, and what’s more, there are no objects that are anywhere close to the line between the two. 
That’s kind of neat for as long as this pattern holds, that all unter planets are much smaller than uber planets. I think it’s already a bit strange to say they are not planets, when they are “dwarf planets”. But there’s more than that. 
The diagram already shows that an Earth sized object could be a dwarf planet and not a planet if it was far away as 700 au, the predicted semi-major axis for “Planet Nine” if it exists. Now, it’s true that they predict it to be Neptune sized, and at that mass, 17 times the mass of Earth, it would sneak in as a planet. But one hypothesis is that “Planet 9″ is not one planet but several planets in resonance, which according to some Spanish astronomers may explain the observations better.

Worlds Beyond Pluto –”There’s Not Just Planet 9, But Several Planets Beyond” 
In that case they could be of different sizes, and what’s to stop some of them from being too small to be IAU planets, yet larger than Earth? 
This would hardly be unprecedented. After all when Pluto was discovered, the astronomers were looking for a much larger planet, large enough to perturb the orbit of Neptune, but they just found the tiny Pluto.
I think once we have Earth sized “dwarf planets” that are not planets, if that happens, the definition will already seem a bit awkward. How can an Earth sized object out in the outer solar system be a dwarf planet, and not a planet, when Mercury, Mars and Earth are planets and not dwarf planets?
But it gets worse than that. We could have planets orbiting as far as the proposal for Nemesis, 1.5 light years away, or around 100,000 au. If you continue Ethan Siegel’s graph that far then Uranus, Neptune, Saturn, and even Jupiter would be too small to count as planets at that distance

There is plenty of space in the outer solar system to find a planet the size of Saturn which is so far from the Sun that it has no chance of “clearing its orbit”. According to the IAU definition it would be a “Gas Giant Dwarf Planet”. If we find such a planet, then surely at that point,  the definition would have to change. So it is not “Future proof”.
We could easily end up with a Saturn sized “dwarf planet gas giant”. Also according to the IAU definition, though a gas giant, it wouldn’t be a planet. At that point I think our language about planets is going to seem really messed up. That could happen. It could happen tomorrow that someone discovers a Saturn or Jupiter sized object that orbits our sun too far away to count as a planet. 
If it is as massive as Jupiter, it’s likely to have a thick hydrogen atmosphere also, like Jupiter, and what else can we call it but a “gas giant”? So then the rest of the name would follow if we use the IAU definition. It would be a “dwarf planet gas giant” and because it doesn’t clear its orbit, then also, not a planet.
And what’s the problem with having hundreds of planets? It’s not a problem with asteroids, or stars, that we have too many of them. You can have sub categories of especially interesting ones. The gas giants. The terrestrial planets that orbit close to the sun. Then – dwarf planets – Earth sized and smaller. Sub dwarf planets.
Why not use the word “dwarf” to refer to the size of the planet. The English word has nothing to do with “clearing orbits”. Then have another word for a planet that clears its orbit, and Alan Stern’s “uber planet” is as good a name for it as any.
I think language matters, that if we have clear language then we can communicate more easily and think more clearly. 
So, the IAU definition is not future proof. I’m pretty sure that if we find a Saturn sized “dwarf planet gas giant non planet” it won’t be long before the IAU definition gets changed and Pluto along with Ceres, and all the other dwarf planets are reinstated as planets. But better to do it now. 
If we don’t find such planets in our own solar system, we are just about bound to find them in other solar systems once our planet detection techniques are good enough. Gas giant sized planets that are still attached to their parent star, but are so far away from them that they can’t “clear their orbits”.
COULD WE FIND A GAS GIANT DWARF EXOPLANET IF WE APPLIED THE IAU DEFINITION TO OTHER SOLAR SYSTEMS
Let’s use Margot’s ?  - the various measures are all are in pretty good agreement in the discrimination between planets and non planets – and that’s the only one that’s easy to calculate. Very easy.
We want a heavy star with the planet far from it, so to find it I sorted the Wikipedia list of exoplanets with the most massive star first .
Here is the formula:
With the planet m measured in Earth masses, M is measured in solar masses, and a in au.. And k for those units is 833. S

The planet masses are often given in Jupiter masses. Jupiter is 317.83 Earth masses, and 833*317.83 =264752. So then the formula is
264752*m / ((M(5/2)*( D (9/8)) m= planet mass in Jupiters, M= star mass in sun masses, D= distance in AU.

One of the best candidates is Fomalhaut b . This one has actually been imaged :) . Or at least a cloud or dust around it.

Fomahaut b is in a 2,000 year highly elliptical orbit from these observations by Hubble.
It orbits at a distance of 115 au around a star that has mass at least 1.9 times the mass of the sun. It is probably a planet of mass at most twice that of Jupiter though probably much less. So putting this into the equation:
M =1.9
m =  2 
a = 177 ± 68
264752*2 / ((1.95/2*(109 9/8)  
gives a Margot PI of 543.
It is “shrouded in dust but very plausibly a planet identified from direct imaging”

Artist’s impression of Fomalhaut b (courtesy NASA) . If it is a gas giant as shown, it will have Margot’s PI > 1. However surely it is just a matter of time before we find a gas giant orbiting far enough from its host star to not be orbit clearing?

Now it could be a much smaller planet as they don’t know its size. What could its mass be to give a Margot PI less than 1? Let’s use Earth masses:
833*m / ((M(5/2)*( D (9/8))



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