Moons with Moons: Solar System Possiblities

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Discussion Overview

The discussion revolves around the possibility of moons having their own moons within our solar system, exploring the theoretical and practical implications of such systems. Participants examine the stability of orbits, the concept of Hill spheres, and the conditions under which a moon could potentially host another moon.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants assert that no moons in our solar system have moons, citing stability issues and the small size of moons relative to their parent planets.
  • Others propose that while the existence of moons with moons is theoretically possible, it is unlikely in our solar system due to the limited size of Hill spheres and gravitational dynamics.
  • A participant mentions that Earth's Moon was formed closer to Earth, which would have affected its Hill sphere and potential for hosting a moon.
  • Concerns are raised about the Kozai effect and its impact on the stability of such systems over time.
  • Some participants suggest that the absence of moons orbiting moons in our solar system may not be mere coincidence, but rather a reflection of the dynamics involved.
  • One participant references the discovery of Polydeuces, a moon of Dione, as a potential example of a moon having a companion moon, though others clarify its orbital characteristics do not fit the traditional definition of a moon of a moon.
  • There is discussion about the possibility of finding moons with moons in other solar systems as exploration continues.

Areas of Agreement / Disagreement

Participants generally agree that the concept of moons having moons is theoretically interesting but remains largely unresolved in the context of our solar system. Multiple competing views exist regarding the stability and dynamics of such systems.

Contextual Notes

Participants note limitations related to the definitions of "moon" and "Hill sphere," as well as the complexities of gravitational interactions over time, which remain unresolved in the discussion.

Who May Find This Useful

Readers interested in celestial mechanics, orbital dynamics, and the exploration of planetary systems may find this discussion relevant.

JV
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Are there any moons in our solar system that have moons?
Or is this not possible, due to instability?
 
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There are no such systems. I don't believe such a situation is theoretically impossible in an arbitrary planetary system, though it would probably be impossible in our own solar system. Most of the moons in the solar system are quite small compared to their parent planets, and are also quite close. For example, the first Lagrange point between the Earth and Earth's Moon is about 9/10 of the way from the Earth to the Moon. This is the point where the Earth's and Moon's gravity are equal in magnitude, and it's only 38,400 km from the Moon's center. Any satellite of the Moon that got further away than that would get tugged into an orbit around the Earth instead.

- Warren
 
JV said:
Are there any moons in our solar system that have moons?
Or is this not possible, due to instability?

In the short-term you'll find many stable zones where moons can orbit moons, but in the long-term its a different story. And the solar system is old, so anything that once temporairly existed is long gone now.

Earth's Moon was formed much closer to the Earth than it is now. This would dramatically reduce its Hill Sphere and any chance it had of forming with its own moon. Even now, its Hill Sphere is not that large, and things such as the Kozai effect would work to destroy such an alignment.

Mars' moons can't have moons, not even artificial ones. Their Hill Spheres (sphere where something can be gravitationally bound to an object) are below their surfaces. Probably many of the solar system's moons share this feature.

But as we get better and better at finding solar systems beyond our, I would bet that its only a matter of time before we find something that orbits something that orbits something else (not counting galaxies)!
 
JV said:
Are there any moons in our solar system that have moons?
Or is this not possible, due to instability?
I guess it depends on our definition of "Moon". There are two asteroids that have their own small moons which I think was considered unlikely until discovery. Ida is a biggie with its own moon. See: http://www.windows.ucar.edu/tour/link=/headline_universe/Eugenia_moon.html
Asteroids aren't moons of planets, they aren't planets, so maybe they can be considered "moons" of the sun. (?)
 
So it is no problem for a satellite to orbit the moon (stable), as long as it is close enough in the "Hill Sphere".
Apparently it is just a coincidence that there is no example of a moon orbitting a moon in our solar system. At least the chance of it happening was just small, but it is their. Am I right?
 
JV said:
So it is no problem for a satellite to orbit the moon (stable), as long as it is close enough in the "Hill Sphere".
Apparently it is just a coincidence that there is no example of a moon orbitting a moon in our solar system. At least the chance of it happening was just small, but it is their. Am I right?
Yes, if an object were in a moon's Hill sphere, it could orbit stabally. But the Hill spheres for moons are very small because of their close proximity to a planet. And Hill spheres can change size as moons' orbits change size and shape over long time periods. So over a long time period moons will likely lose their moons. So I don't think it's just a coincidence that our solar system's moons are moonless. Also, its unlikely that a moon of a moon could even form in such a small Hill sphere.

I'd bet that in a hundred years from now, when we have millions of other solar systems mapped out, that we will find a few examples.

Just my guesses...
 
tony873004 said:
Yes, if an object were in a moon's Hill sphere, it could orbit stabally. But the Hill spheres for moons are very small because of their close proximity to a planet. And Hill spheres can change size as moons' orbits change size and shape over long time periods. So over a long time period moons will likely lose their moons. So I don't think it's just a coincidence that our solar system's moons are moonless. Also, its unlikely that a moon of a moon could even form in such a small Hill sphere.

I'd bet that in a hundred years from now, when we have millions of other solar systems mapped out, that we will find a few examples.

Just my guesses...
From a JPL news release today it seems that moons do have moons:
Another discovery was a tiny moon, about 5 kilometers (3 miles) across, recently named Polydeuces. Polydeuces is a companion, or “Trojan” moon of Dione. Trojan moons are found near gravitationally stable points ahead or behind a larger moon. Saturn is the only planet known to have moons with companion Trojan moons.

EDIT: Site here:
http://saturn.jpl.nasa.gov/news/press-release-details.cfm?newsID=547
 
Last edited by a moderator:
No. Polydeuces is orbiting Saturn roughly in Dione's orbit, in a 'teardrop orbit' (seen in the co-rotating frame) around the L4 or L5 Langrangian positions 600 ahead or behind Dione, or even in a 'horse-shoe orbit' (seen in the co-rotating frame) around both and centred on the L1 position 1800 from Dione.

Garth
 
Last edited:
Garth said:
No. Polydeuces is orbiting Saturn roughly in Dione's orbit, in a 'teardrop orbit' (seen in the co-rotating frame) around the L4 or L5 Langrangian positions 600 ahead or behind Dione, or even in a 'horse-shoe orbit' (seen in the co-rotating frame) around both and centred on the L1 position 1800 from Dione.

Garth
But at least it qualifies as a "companion" moon to a moon.
 
  • #10
Well yes - all trojans are companions in orbits with the same period.
 

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