Chandrasekhar Limit

The Chandrasekhar limit defines the maximum mass at which a white dwarf star remains stable.
Beyond this limit, the star collapses due to gravitational forces.
It is a core topic in astrophysics and cosmology.
Example: Studying stellar collapse in astronomy courses.

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John Smith

Harish writes about education trends, technology adoption, and school innovation. With over a decade of experience creating content for educators, he focuses on simplifying complex topics into practical insights school leaders can act on.

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