This is The End
Penultimate Amazing
- Joined
- Sep 14, 2007
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No. You can classify the largest body in the co-orbiting group as the planet and the smaller ones as moons.
Unless of course it is a binary where the difference in size between the two is not statistically significant (meaning they have a mass ratio extremely close to 1; something > .9, maybe > .8, should be close enough).*
Then they should both be considered planets if they otherwise classify. Anything less and one is a moon IMO. (Some scientists have actually proposed that smaller mass ratio systems should be considered double planets. Those scientists are smelly & dumb and, most importantly, wrong.
But from what we know about the formation and evolution of solar systems they (mass ratios near 1) should be extremely rare. So improbable in fact that the term Double Planet is not even officially recognized by the IAU.
Nothing in our solar system comes even close. The closest is Pluto–Charon with a mass ratio of .11 or so (Earth-Moon being like .011, and the gas giants and there moons being like .00011). Nothing in any solar system we discover should come even close to it.
But because of the size of the universe, we should assume they do exist.**
*Not to be confused with merely being a binary system where the bodies orbit a point clearly outside of either body (their barycenter).
**A neat statistical side effect of the unfathomable size of the universe. There are some extremely low probability things that it should be basically impossible for us to find in any random solar system, or even galaxy. But yet because of the insane size of the universe, they are somewhere. (And, unfortunately, guess what is very likely one of those things? Intelligent sentient life.)