In 1935, 24-year-old Subrahmanyan Chandrasekhar discovered that stars exceeding approximately 1.4 times the Sun's mass cannot end as calm white dwarfs; instead, gravity overcomes electron degeneracy pressure, causing the core to collapse into an unimaginably dense state. Despite being dismissed by influential astronomer Arthur Eddington as 'stellar buffoonery' at the Royal Astronomical Society, this discovery became foundational to understanding white dwarfs, supernovae, and neutron stars, ultimately earning Chandrasekhar the Nobel Prize in Physics 53 years later.
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They Laughed at His Theory for 50 Years. Then Gave Him the Nobel Prize.Added:
In 1935, [music] a single speech nearly erased a discovery that explains how stars die.
A 24-year-old Subramanyan [music] Chandrasekhar had already run the numbers years earlier during a voyage from India to [music] England. He found a hard cutoff.
Above about 1.4 times the sun's [music] mass, a star cannot end as a calm, fading ember.
Gravity wins. The core must collapse into something unimaginably dense.
Then Arthur Eddington, the most influential [music] astronomer alive, stood up at the Royal Astronomical Society and dismissed it as stellar buffoonery.
With his reputation, that was enough.
The room followed his lead. [music] The idea was pushed aside for years. But the sky did not cooperate with Eddington.
Chandrasekhar's limit became essential science, a cornerstone for [music] understanding white dwarfs, supernovae, and the birth of the most extreme remnants.
53 years after that [music] shipboard calculation, Chandrasekhar received the Nobel Prize. Eddington never publicly [music] withdrew his attack, but the universe had already delivered its verdict.
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