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：2025/11/22
Chandrasekhar limit
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(astronomy) The maximum theoretical mass of a white dwarf, approximately 1.4 solar masses.
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Chandrasekhar limit
When a white dwarf's mass approaches the Chandrasekhar limit, it becomes unstable and may collapse into a neutron star or explode as a Type Ia supernova.
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When a white dwarf's mass approaches the Chandrasekhar limit, it becomes unstable and may collapse into a neutron star or explode as a Type Ia supernova.
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