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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.
SCORE
0
DENSITY LEVEL: 1
STELLAR MASSDEGENERACY PRESSURE
0.60 M☉
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×1.0
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ANOMALIES ACTIVE
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STABILIZE
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SHARDS
0