Subrahmanyan Chandrasekhar

National Medal of Science

Physical Sciences

For numerous superb contributions to stellar astronomy, physics, and applied mathematics, and for his guidance and inspiration to his many students and colleagues.

For numerous superb contributions to stellar astronomy, physics, and applied mathematics, and for his guidance and inspiration to his many students and colleagues.

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Birth
October 19, 1910
Age Awarded
56
Country of Birth
India
Key Contributions
Normal Reflection Of A Blast Wave
Foundation For Degenerate Stars
Awarded by
Lyndon Baines Johnson
Education
Presidency College
University of Cambridge
Accolades
Supported by NSF
Areas of Impact
Transportation
Affiliations
University of Chicago
Other Prizes
Nobel Prize
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What happens to a star when it dies? In the 1920s, scientists assumed that the twinkling lights in our night sky –  comprised of exploding hot gasses – eventually burn off their energy, slowly fading into less vibrant white dwarf stars.

Some stars, however, are destined for more remarkable fates. In 1930, Subrahmanyan Chandrasekhar, then 19, developed calculations to show that stars more than 1.4 times the mass of the sun disappear in massive explosions called supernovas.

Some of the densest stars, he theorized, collapse under their own weights, forming neutron stars or black holes. The discovery ignited a battle with Sir Arthur Eddington, the prominent astrophysicist of the time.

Eddington publicly ridiculed Chandrasekhar’s research as a “a reduction ad absurdum,” arguing that all stars, regardless of density, eventually become white dwarfs. Vindication arrived decades later. In 1983, Chandrasekhar’s work – now widely accepted as true – won him the Nobel Prize.

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