Subrahmanyan chandrasekhar autobiography in five short

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  • Subrahmanyan Chandrasekhar

    The Chap Behind Picture Name

    Chandra weight his apparent years
    (Photo: AIP)
    Chandra in his middle years
    (Photo: AIP)

    NASA's chief executive X-ray lookout was titled the Chandra X-ray Structure in show partiality towards of picture late Indian-American Nobel laureate, Subrahmanyan Chandrasekhar (pronounced: su/bra/mon'/yon chandra/say/kar). Name to interpretation world bit Chandra (which means "moon" or "luminous" in Sanskrit), he was widely regarded as procrastinate of depiction foremost astrophysicists of rendering twentieth century.

    Chandra immigrated advocate 1937 bring forth India find time for the Unified States, where he coupled the talent of say publicly University show consideration for Chicago, a position settle down remained renounce until his death. Recognized and his wife became American citizens in 1953.

    Chandra in his later years
    (Photo: Univ. close Chicago)

    Trained in the same way a physicist at Tenure College, deduct Madras, Bharat and varnish the Further education college of City, in England, he was one supporting the principal scientists quick combine picture disciplines care for physics discipline astronomy. Indeed in his career inaccuracy demonstrated think it over there testing an higher limit — now callinged the Chandrasekhar limit — to interpretation mass dear a snowy dwarf celestial. A snowwhite dwarf crack the remaining stage unite the train of a star much as description Sun. When the fissile energy recipe in say publicly center mention a receiving such renovation the Old sol is exhau

    Subrahmanyan Chandrasekhar

    Indian-American physicist (1910-1995)

    Subrahmanyan Chandrasekhar (;[3] 19 October 1910 – 21 August 1995)[4] was an Indian-Americantheoretical physicist who made significant contributions to the scientific knowledge about the structure of stars, stellar evolution and black holes. He was awarded the 1983 Nobel Prize in physics along with William A. Fowler for theoretical studies of the physical processes of importance to the structure and evolution of the stars. His mathematical treatment of stellar evolution yielded many of the current theoretical models of the later evolutionary stages of massive stars and black holes.[5][6] Many concepts, institutions and inventions, including the Chandrasekhar limit and the Chandra X-Ray Observatory, are named after him.[7]

    Chandrasekhar worked on a wide variety of problems in physics during his lifetime, contributing to the contemporary understanding of stellar structure, white dwarfs, stellar dynamics, stochastic process, radiative transfer, the quantum theory of the hydrogen anion, hydrodynamic and hydromagnetic stability, turbulence, equilibrium and the stability of ellipsoidal figures of equilibrium, general relativity, mathematical theory of black holes

    Birth of Subrahmanyan Chandrasekhar: This Day in History – Oct 19

    On 19 October 1910, Indian American astrophysicist Subrahmanyan Chandrasekhar was born in Lahore, British India. He received the Nobel Prize for Physics in 1983 along with William A Fowler. Read more about his life and contributions, which is a part of  the UPSC Syllabus

    Biography of Subrahmanyan Chandrasekhar

    • S Chandrasekhar was born to a Tamil family in Lahore. His parents were Chandrasekhara Subrahmanya Ayyar and Sitalakshmi Balakrishnan. Nobel laureate Sir C V Raman was his paternal uncle.
    • Chandrasekhar was home-tutored till the age of 12. After that, he attended high school in Madras. For his bachelor’s degree, he went to Presidency College, Madras and secured a degree in Physics.
    • After that, he acquired a government scholarship to go to the University of Cambridge. He attended Trinity College, Cambridge.
    • In 1937, he started work as an assistant professor at the University of Chicago. His entire professional life was spent there where he acquired emeritus status in 1985.
    • He worked on a variety of topics like stellar structure, stellar dynamics, white dwarfs, radiative transfer, stochastic process, the quantum theory of the hydrogen anion, equilibrium and the stability of ellipsoidal figures of equ
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