The limit beyond which the stars suffer internal collapse is called the

Raman Effect
Chandrasekhar limit
Aurora Borealis
Quasan Zone

The correct answer is: B. Chandrasekhar limit

The Chandrasekhar limit is the maximum mass of a stable white dwarf star. Beyond this limit, electron degeneracy pressure cannot support the star against gravitational collapse.

The Raman effect is the inelastic scattering of light by a substance, resulting in a change in frequency of the light.

The Aurora Borealis, also known as the Northern Lights, is a natural light display in the sky, predominantly seen in the high-latitude regions (around the Arctic and Antarctic).

The Quasan Zone is a region of space that is thought to be the source of quasars. Quasars are extremely bright objects that are powered by supermassive black holes.

The Chandrasekhar limit is named after Indian astrophysicist Subrahmanyan Chandrasekhar, who first calculated it in 1931. The limit is approximately 1.4 solar masses, which is the mass of the Sun.

If a white dwarf star has a mass greater than the Chandrasekhar limit, it will collapse under its own gravity. This collapse can lead to a supernova explosion, or the formation of a neutron star or black hole.

Exit mobile version