description Chandrasekhar limit Overview
The Chandrasekhar Limit defines the maximum mass (approximately 1.44 solar masses) a white dwarf star can have before it collapses under its own gravity, typically triggering a supernova.
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Chandrasekhar limit scores 8.57/10 (Great) on Lunoo, making it a well-rated option in the Physics Concept category.
What are the best alternatives to Chandrasekhar limit?
See our alternatives page for Chandrasekhar limit for a ranked list with scores. Top alternatives include: Stellar nucleosynthesis, Nucleosynthesis, Virial theorem.
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