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Subrahmanyan Chandrasekhar

Astronomy

Subrahmanyan Chandrasekhar calculated, as a young man on the ship from India to England in 1930, the maximum mass a white dwarf star can have before its own gravity overwhelms the pressure holding it up, about 1.44 times the mass of the Sun. Beyond that limit a collapsing star cannot settle into a white dwarf and instead becomes a neutron star or black hole. He shared the 1983 Nobel Prize in Physics for this and later work on stellar structure. This description is adapted from Wikipedia contributors under CC BY-SA 4.0; changes were made. https://creativecommons.org/licenses/by-sa/4.0/

Facts
Birth YearSourced to the subject's own account
1910 1
Death DateSourced to the subject's own account
1995-08-21 1
Death YearSourced to the subject's own account
1995 1
FieldSourced to the subject's own account
Astrophysics 1
Connections

Works In

Astronomy, Disciplines
Source Astrophysics (Britannica)
Sources
1. Subrahmanyan Chandrasekhar (Wikipedia)
WikipediaLead section
Quote, Lead section
Subrahmanyan Chandrasekhar (19 October 1910-21 August 1995) was an Indian-American theoretical physicist.
View the Source
Astrophysics (Britannica)
Encyclopaedia BritannicaWorks In: AstrophysicsView the Source
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