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The Chandrasekhar limit is about 1.4 solar masses

The Chandrasekhar limit is about 1.4 solar masses

The Chandrasekhar limit is about 1.4 solar masses

White dwarfs above this mass cannot support themselves with electron degeneracy pressure and collapse — often as Type Ia supernovae.

Shahzad Mahota Shahzad Mahota @shahzad-mahota

The Chandrasekhar limit is about 1.4 solar masses