The Chandrasekhar Limit is:
A)the upper mass limit for a white dwarf.
B)the temperature at which hydrogen fusion starts.
C)the temperature at which helium fusion starts.
D)the point at which a planetary nebula forms.
E)the lower mass limit for a Type II supernova.

Question

Quizplus · Accepted Answer

The Chandrasekhar Limit is the maximum mass that a white dwarf, which is a type of star in its final stage, can have. If a white dwarf exceeds this limit of about 1.4 solar masses, it will collapse and explode in a Type Ia supernova. The Chandrasekhar Limit is the upper mass limit for a white dwarf, beyond which it will collapse under its own gravity and become a Type Ia supernova. This limit is approximately 1.4 times the mass of the sun.

The Chandrasekhar Limit Is