HomeAstronomyThe Chandrasekhar limit: Facts and Observation

The Chandrasekhar limit: Facts and Observation

The Chandrasekhar limit determines if a star dies as a white dwarf, or has the mass to exceed this, launching a supernova to create a black hole or neutron star.

Stars are locked in battles against their own gravity, all of which will eventually be lost, leading to violent and radical changes that mark the end of their main sequence lifetimes.

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