Chandrasekhar limit is now taken as aprox. approximately 1.4 times the mass of the sun. Any white dwarf with less than this mass will star a white dwarf forever, while a star that exceeds this mass is destined to end its life in that most violent of explosions: "a supernova".
hope this much is enough if u need for information ask me frankly
Sneha3123
sry i don't know why ita name is chandrasekhar
Sneha3123
but white dwarf is a small but very dence star nearly its size is as the size of planets A white dwarf is formed when a low-mass star has exhausted all its central nuclear fuel and lost its outer layers as a planetary nebula.
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Chandrasekhar limit is now taken as aprox. approximately 1.4 times the mass of the sun. Any white dwarf with less than this mass will star a white dwarf forever, while a star that exceeds this mass is destined to end its life in that most violent of explosions: "a supernova".
hope this much is enough
if u need for information ask me frankly
thank you
#Sneha