General Knowledge - World Geography - Discussion

Discussion Forum : World Geography - Section 1 (Q.No. 56)
56.

The limit beyond which the stars suffer internal collapse is called the

Raman Effect
Chandrasekhar limit
Aurora Borealis
Quasan Zone
Answer: Option
Explanation:
No answer description is available. Let's discuss.
Discussion:
3 comments Page 1 of 1.

Venkat said:   7 years ago
Chandrasekhar Limit is 1.4 times the mass of our Sun, meaning that any star got to have a minimum mass of the above-mentioned number to go supernova. If not, the collapse won't be strong enough and the star would become a White Dwarf.

Varas said:   8 years ago
Chandrasekhar limit in astrophysics, maximum mass theoretically possible for a stable white dwarf star.

Lokesh said:   8 years ago
Explain the remaining three options?

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