# Who developed the theory of Chandrasekhar limit?

## Who developed the theory of Chandrasekhar limit?

astrophysicist Subrahmanyan Chandrasekhar
Chandrasekhar limit, in astrophysics, maximum mass theoretically possible for a stable white dwarf star. This limiting value was named for the Indian-born astrophysicist Subrahmanyan Chandrasekhar, who formulated it in 1930.

## What is the size of the Chandrasekhar limit?

1.4 solar masses
The Chandrasekhar Limit of 1.4 solar masses, is the theoretical maximum mass a white dwarf star can have and still remain a white dwarf (though this limit does vary slightly depending on the metallicity).

The Chandrasekhar limit (/tʃʌndrəˈseɪkər/) is the maximum mass of a stable white dwarf star. The currently accepted value of the Chandrasekhar limit is about 1.4 M ☉ (2.765×1030 kg).

### What do you mean by Chandrashekhar limit?

Definition of Chandrasekhar limit : the maximum mass at which a star near the end of its life cycle can become a white dwarf and above which the star will collapse to form a neutron star or black hole : a stellar mass equal to about 1.4 solar masses.

### What is Chandrasekhar unit?

What is meant by Chandrasekhar limit explain its significance?

#### Who is famous Indian astrophysicist?

Jayant Vishnu Narlikar is an Indian astrophysicist. Narlikar is a proponent of steady state cosmology. He developed with Sir Fred Hoyle the conformal gravity theory, commonly known as Hoyle–Narlikar theory. It synthesises Albert Einstein’s Theory of Relativity and Mach’s Principle.

#### What is Chandrasekhar limit Quora?

Chandrashekar limit is the most stable mass of a white dwarf. In case of white dwarfs, their mass increases as their radius decreases. It is accepted as 1.4M(2.765 × 1030 kg) times the mass of the Sun. Any white dwarf lesser than 1.4 shall remain a white dwarf forever while anything more Woll result in a Supernova.

How black holes are formed?

Stellar black holes form when the center of a very massive star collapses in upon itself. This collapse also causes a supernova, or an exploding star, that blasts part of the star into space. Scientists think supermassive black holes formed at the same time as the galaxy they are in.

## What is Chandrasekhar limit Upsc?

Chandrasekhar Limit is the maximum mass theoretically possible for a stable white dwarf star. A limit which mandates that no white dwarf (a collapsed, degenerate star) can be more massive than about 1.4 times the mass of the Sun.