Search results
Subrahmanyan Chandrasekhar FRS ( / ˌtʃəndrəˈʃeɪkər /; [3] 19 October 1910 – 21 August 1995) [4] was an Indian-American theoretical physicist who made significant contributions to the scientific knowledge about the structure of stars, stellar evolution and black holes.
Chandra Shekhar (17 April 1927 – 8 July 2007), known as Jananayak, was an Indian politician who served as the 8th Prime Minister of India, between 10 November 1990 and 21 June 1991. He headed a minority government of a breakaway faction of the Janata Dal with outside support from the Indian National Congress. [1]
Biographical. I was born in Lahore (then a part of British India) on the 19th of October 1910, as the first son and the third child of a family of four sons and six daughters. My father, Chandrasekhara Subrahmanya Ayyar, an officer in Government Service in the Indian Audits and Accounts Department, was then in Lahore as the Deputy Auditor ...
Jun 17, 2024 · S. Chandrasekhar, Indian-born American astrophysicist who, with William A. Fowler, won the 1983 Nobel Prize for Physics for key discoveries that led to the currently accepted theory on the later evolutionary stages of massive stars.
Aug 21, 1995 · 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.
NASA's premier X-ray observatory was named the Chandra X-ray Observatory in honor of the late Indian-American Nobel laureate, Subrahmanyan Chandrasekhar (pronounced: su/bra/mon'/yon chandra/say/kar). Known to the world as Chandra (which means "moon" or "luminous" in Sanskrit), he was widely regarded as one of the foremost astrophysicists of the ...
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.
Subrahmanyan Chandrasekhar was an astrophysicist. He discovered that massive stars can collapse under their own gravity to reach enormous or even infinite densities. Today we call these collapsed stars neutron stars and black holes.
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.
Oct 19, 2017 · This figure — 1.4 times the mass of our sun — is now known as the “Chandrasekhar limit,” and it’s key to understanding the evolution of stars in our universe. Beyond this limit, stars at ...
