GENERAL KNOWLEDGE

Detailed explanation-1: -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.

Detailed explanation-2: -In 1930, 19-year-old Subrahmanyan Chandrasekhar discovered that stars were destined to collapse into nothingness and become black holes.

Detailed explanation-3: -Beginning in the 1930s, Subramanyan Chandrasekhar formulated theories for the development that stars subsequently undergo. He showed that when the hydrogen fuel of stars of a certain size begins to run out, it collapses into a compact, brilliant star known as a white dwarf.

Detailed explanation-4: -Subrahmanyan Chandrasekhar was one of the foremost astrophysicists of the twentieth century. He was one of the first scientists to couple the study of physics with the study of astronomy. Chandra proved that there was an upper limit to the mass of a white dwarf.