Arthur Eddington

Also known as Sir Arthur Stanley Eddington, Sir Arthur Eddington

British astrophysicist (1882-1944)

OverviewAI-generated

Arthur Stanley Eddington was a male person from the United Kingdom. He was born on December 28, 1882, and died on November 22, 1944. His works include The Nature Of The Physical World, New Pathway In Science, Space Time and Gravitation, and Theory of Relativity and Its Influence on Scientific Thought.

Eddington is recognized in the Royal Society collection and the American Academy Arts Sciences collection. He is referenced by 518 other encyclopedia articles. Regarding his writing, he stated that physics has in the main contented itself with studying the abridged edition of the book of nature.

Synthesized by Vinony from 19 facts across 8 sources: Wikidata, Last.fm, Crossref, Wikiquote, MusicBrainz, Open Library, Vinony collections, Vinony graph. Generated from structured data (not the Wikipedia text) and checked against those facts — may still contain errors.

Wikidata facts

Instance of: human
Given name: Arthur
Gender: male
Citizenship: United Kingdom
Place of birth: Kendal
Place of death: Cambridge
Occupation: mathematician
Position held: professor
Educated at: University of Cambridge
Employer: Royal Observatory
Languages spoken: English language
Notable work: radiative transfer
Noble title: Knight Bachelor
Doctoral advisor: Ernest Barnes
Field of work: astrophysics
Image: Arthur Stanley Eddington.jpg

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member of: Academy of Sciences of Turin
Commons category: Arthur Stanley Eddington
date of birth: 1882-12-28
date of death: 1944-11-22
Commons Creator page: Arthur Stanley Eddington
nominated for: Nobel Prize in Physics
name in native language: sir Arthur Stanley Eddington
writing language: English language
influenced by: Horace Lamb
maintained by WikiProject: WikiProject Mathematics

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Encyclopedic overview

Sir Arthur Stanley Eddington (28 December 1882 – 22 November 1944) was an English astrophysicist and mathematician. The Eddington limit, the natural limit to the luminosity of stars, or the radiation generated by accretion onto a compact object, is named in his honour.

Around 1920, he foreshadowed the discovery and mechanism of nuclear fusion processes in stars in his paper "The Internal Constitution of the Stars". At that time, the source of stellar energy was a complete mystery; Eddington was the first to correctly speculate that the source was fusion of hydrogen into helium.

Excerpted from Wikipedia’s “Arthur Eddington” article, available under the CC BY-SA 4.0 licence.