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ℹ️ STELLAR FACTOID: CHANDRASEKHAR LIMIT
Named after astrophysicist Subrahmanyan Chandrasekhar, the Chandrasekhar Limit (exactly 1.44 Solar Masses) is the maximum mass threshold a stable white dwarf star can support before collapsing. Beyond this limit, electron degeneracy pressure fails, triggering a catastrophic runaway carbon-fusion reaction that explodes as a Type Ia Supernova.