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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

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Subrahmanyan Chandrasekhar

Very Interesting!

Subrahmanyan Chandrasekhar was known to the world as Chandra. The word chandra means "moon" or "luminous" in Sanskrit.

Subrahmanyan Chandrasekhar was born in 1910 in Lahore, which at the time was in British India. He was one of ten children born to Sita Balakrishnan and Chandrasekhara Subrahmanya Ayyar. His father was a government officer while his mother was a highly intellectual woman that translated literary works into Tamil, an Indian dialect. His parents and private tutors schooled Chandra at home until the age of twelve. He attended Hindu High School where he graduated in 1925 at the age of fifteen. He earned a bachelors degree in physics from Presidency College. Chandra received a scholarship to pursue graduate studies at Cambridge University in England. He also studied for one year in Copenhagen at the Institut for Teoretisk Fysik prior to receiving his Ph.D. from Cambridge in 1933. In 1936 Chandra was joined with Lalitha Doriswamy in a marriage that lasted for over fifty years. In 1937 Chandra joined the faculty

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Subrahmanyan Chandrasekhar—child prodigy, predictor of black holes, Nobelist, and UChicago professor for nearly 60 years—often distilled his life into two sentences: “I left India and went to England in 1930. I returned to India in 1936 and married a girl who had been waiting for six years, came to Chicago, and lived happily thereafter.”

Chandrasekhar is best known for the earliest part of his career, when he determined the fate of massive stars and was betrayed by a mentor. Yet he spent the next six decades making equally influential breakthroughs in stellar structure and dynamics, and training a new generation of astrophysicists. He also faced discrimination and alienation, elided from the fairy-tale ending he liked to recount.

Chandra, as he was known, was born in 1910 in Lahore—then British India, now Pakistan—the third of 10 children. In Chandra: A Biography of S. Chandrasekhar (University of Chicago Press, 1990) his biographer Kameshwar C. Wali, a UChicago physicist in the late ’60s, describes him as a mischievous child with an early aptitude for math.

Chandra didn