Chandrasekhar Limit

Output: Press calculate

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Formula:Chandrasekhar Limit

About Chandrasekhar Limit

The Chandrasekhar Limit is the maximum mass of a stable white dwarf star. It is approximately 1.4 solar masses. When the mass of a white dwarf exceeds this limit, it cannot withstand gravitational collapse and undergoes a violent collapse into a neutron star or a black hole.

Parameter usage:


Data Validation

The mass should be a positive number.


The Chandrasekhar Limit plays a significant role in the understanding of the life cycles of stars and the formation of various celestial bodies such as neutron stars and black holes.

Tags: Astronomy, Stellar Evolution, White Dwarf, Chandrasekhar Limit