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Stars are formed when clouds of gas and dust collapse into themselves. Either the cloud is big and dense enough to collapse into a star, or it will remain as a cloud. Our Jupiter was created when, during the collapse, other forces pulled part of the collapsing cloud away from the sun, into a stable orbit. > Stars form when the dust and gas clouds in a nebula cool, progressively fragment and eventually collapse under their own gravity. The smallest stars are about 80 Jupiter masses, below which the core is not dense enough to fuse hydrogen, but smaller objects can coalesce through the same process, including dimly glowing brown dwarfs – sometimes called failed stars – and, below about 13 Jupiter masses, planetary-mass objects. But theoretical predications suggest that the lower boundary for an object forming through a star-like gravitational collapse is about three to seven Jupiter masses. https://www.theguardian.com/science/2023/oct/02/jumbos-jupit... |
Why is this? Why can’t a small molecular cloud coalesce into small objects?