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Mass is what causes an object to have gravity. Above a certain mass and radius, the self-gravity of the object overcomes the yield strength of even the strongest solid materials. The surface may still be irregular, but overburden pressure causes the rocks deep inside to deform until the planet has a stable spherical shape. For solid bodies, that occurs between 200km and 300km radius, depending on the density and strength of the materials. Dwarf planets, moons and asteroids with radii less than 200km may be more potato-shaped, but larger objects will always be round.

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11y ago

There is no specific limit; simply speaking, the more mass a planet has, the more gravity it will have. And the larger it is, the more insignificant will any elevation (such as a mountain) seem in comparison. But of course, there is no definite point at which you can say "this one is round, and the other one isn't"; technically, no planet will ever be perfectly round.

A good rough estimate would be Ceres, the least massive object we know of that's definitely "round". The mass of Ceres is about 1021 kg. However, much less massive bodies could be round if they're liquid; any liquid body should be "round".

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Q: How you determine how much mass is needed to make a planet round?
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