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symbo symbo
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Posts: 1970
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7 years ago
There is a mass limit for a star in the white-dwarf phase, the Chandrasakhar limit, beyond which the electron-degeneracy pressure can no longer support the star against its own gravity. This mass limit is
A)   0.2 solar mass.   C)   1.4 solar masses.
B)   30 solar masses.   D)   14 solar masses.
Textbook 
Discovering the Universe

Discovering the Universe


Edition: 7th
Authors:
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papachulopapachulo
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7 years ago
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symbo Author
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6 years ago
Thanks for answering, I'll share this with my classmates too
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