The Chandrasekhar mass limit is:
A).08 solar masses.
B).4 solar masses.
C)1.4 solar masses.
D)3 solar masses.
E)8 solar masses.

Question

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The Chandrasekhar mass limit is the maximum mass of a stable white dwarf star, which is approximately 1.4 times the mass of the sun. This limit is reached when the electrons inside the star become so densely packed that they merge with the protons, creating neutrons and causing a collapse that results in a supernova explosion. The Chandrasekhar mass limit is approximately 1.4 solar masses, which is the maximum mass that a white dwarf star can achieve before collapsing and potentially becoming a supernova. This limit is named after the Indian astrophysicist Subrahmanyan Chandrasekhar, who first calculated it in 1931.

The Chandrasekhar Mass Limit Is