Undergrad Can a planet have multiple large moons?

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The discussion explores the feasibility of a planet having multiple large moons, particularly focusing on the implications for Earth. It notes that the visual size of moons and their tidal effects are influenced by their distance and mass, with tidal forces increasing significantly as the angular diameter of the moon increases. The concept of using less dense materials, like pumice, for moon formation is humorously suggested. The conversation also touches on the challenges of maintaining stable orbits for multiple moons, emphasizing the need for them to be outside the Roche limit and in orbital resonance. Overall, the likelihood of a planet naturally forming such a system with large moons is considered to be quite low.
Sherwood Botsford
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I thought that I'd posted this here, but perhaps not. I've had it on the OtherWorlds and the Physics stackexchange with no results.

I grew up with countless alien planet covers depicting 2-3 moons all considerably larger (telephoto lens...) than Luna's appearance from earth.

Luna from Earth subtends about 1/2 degree. If it were half the distance it would be 1 degree, and we'd have some ferocious tides. (Tidal forces go up as 1/r3, right, so 1 degree luna = 8 times present tides.)

Could Earth have two moons that subtend more than a degree?

Thoughts: visual size goes up as R2 while mass goes up as R3 So a smaller moon orbiting closer results in less orbiting mass.

But with tides as 1/r3 it appears that tides are proportional to the visual angular diameter of the moon. Yes?

Now the other way to make bigger moons would be make them out of pumice. Styrofoam moons. Or really big balloons...

Anyway, I played with a orbital simulator and spent a rainy afternoon trying to find an orbital solution that had two moons, one with 1/80 the mass of the primary, one with 1/320 the mass of the primary, but at half the distance. Usually the little guy gets ejected within a dozen orbits.

What are the conditions for a planet to have multiple moons of significant mass?
 
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I would say, as a first approximation and without having done the calculations myself, that if the moons orbit outside the Roche limit and maintain a stable orbital resonance then you may be able to construct a system with visually big moons. However, I guess that the chance of such a system forming by natural accretion would be (very) low as the system would be more likely to end up with rings and small shepherd moons.
 
UC Berkely, December 16, 2025 https://news.berkeley.edu/2025/12/16/whats-powering-these-mysterious-bright-blue-cosmic-flashes-astronomers-find-a-clue/ AT 2024wpp, a luminous fast blue optical transient, or LFBOT, is the bright blue spot at the upper right edge of its host galaxy, which is 1.1 billion light-years from Earth in (or near) a galaxy far, far away. Such objects are very bright (obiously) and very energetic. The article indicates that AT 2024wpp had a peak luminosity of 2-4 x...

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