Why is there an upper limit to the mass of a white dwarf?
A)The upper limit to the masses of white dwarfs was determined through observations of white dwarfs in binary systems, but no one knows why the limit exists.
B)The more massive the white dwarf, the greater the degeneracy pressure and the faster the speeds of its electrons. Near 1.4 solar masses, the speeds of the electrons approach the speed of light, and no more mass can be supported.
C)White dwarfs come only from stars with masses less than 1.4 solar masses.
D)The more massive the white dwarf, the higher its temperature and hence the greater its degeneracy pressure. Near 1.4 solar masses, the temperature becomes so high that all matter effectively melts into subatomic particles.

Question

Quizplus · Accepted Answer

As a white dwarf becomes more massive, the electrons within it must move faster in order to support the increasing gravitational force. Once the electrons begin moving close to the speed of light, their relativistic effects prevent further increase in mass. This upper limit is known as the Chandrasekhar limit, which is approximately 1.4 solar masses.

Why Is There an Upper Limit to the Mass of a White