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Arthur Eddington

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Arthur Eddington
NameArthur Eddington
CaptionSir Arthur Stanley Eddington
Birth date28 December 1882
Birth placeKendal, Westmorland, England
Death date22 November 1944
Death placeCambridge, Cambridgeshire, England
FieldsAstrophysics, Astronomy, Philosophy of science
Alma materUniversity of Manchester, Trinity College, Cambridge
Known forStellar structure, Eddington limit, Eddington number, Eddington experiment
AwardsRoyal Society Fellow (1914), Royal Medal (1928), Order of Merit (1938)

Arthur Eddington was a preeminent astrophysicist and philosopher of science whose work fundamentally shaped modern understanding of stellar structure and was instrumental in confirming Albert Einstein's general relativity. As the Plumian Professor of Astronomy and Experimental Philosophy at the University of Cambridge and director of its Cambridge Observatory, he pioneered the application of physics to astronomical problems. His leadership of the 1919 solar eclipse expedition provided the first empirical evidence for general relativity, catapulting both the theory and himself to worldwide fame.

Early life and education

Born in Kendal to a Quaker family, he was raised in Somerset after his father's death. His early academic brilliance earned him a scholarship to Owens College, which later became the University of Manchester, where he studied under renowned physicists like Arthur Schuster and Horace Lamb. In 1902, he secured a scholarship to Trinity College, Cambridge, excelling in the Mathematical Tripos and graduating as Senior Wrangler in 1905. He immediately began research at the Royal Greenwich Observatory, working under the Astronomer Royal Frank Watson Dyson on stellar parallax and the proper motions of stars.

Scientific career and research

Appointed to the Plumian Professor of Astronomy and Experimental Philosophy in 1913, he revolutionized astrophysics by elucidating the internal workings of stars. His seminal 1926 work, *The Internal Constitution of the Stars*, established the principles of hydrostatic equilibrium and radiative equilibrium, describing stars as spheres of ideal gas. He correctly hypothesized that the energy source was nuclear fusion, specifically the conversion of hydrogen to helium, and formulated the critical Eddington limit, the maximum luminosity a star can achieve before radiation pressure overcomes gravity. His research also contributed significantly to the understanding of Cepheid variable stars and the mass–luminosity relation.

Eddington and relativity

A dedicated proponent of Albert Einstein's general relativity, he masterminded the 1919 expeditions to Príncipe and Sobral to observe a solar eclipse. The goal was to measure the apparent deflection of starlight by the Sun's gravity, a key prediction of the theory. The successful results, presented to the Royal Society and the Royal Astronomical Society, were hailed as a monumental confirmation, making headlines worldwide in publications like *The Times* and *The New York Times*. He further championed the theory through his influential 1923 book, *The Mathematical Theory of Relativity*, which Einstein praised as the finest presentation of the subject in any language.

Philosophy of science

Deeply influenced by his Quaker beliefs, he pursued a synthesis of science, philosophy, and mysticism. In works like *The Nature of the Physical World* and *Science and the Unseen World*, he argued for a philosophical idealism, suggesting that the physical universe is mind-constructed. He famously distinguished between the symbolic, structural knowledge provided by physics and the direct, intimate knowledge of consciousness. His concept of selective subjectivism and his discussions on the philosophical implications of quantum mechanics and indeterminacy engaged a broad public audience, though they were sometimes critiqued by colleagues like Ernest Rutherford.

Later life and legacy

In his later years, he embarked on an ambitious but unfinished quest to derive fundamental constants like the fine-structure constant through his "Fundamental theory." He was knighted in 1930 and received the Order of Merit in 1938. He served as president of both the Royal Astronomical Society and the International Astronomical Union. He died in Cambridge in 1944 and is buried at the Ascension Parish Burial Ground. His legacy endures through concepts like the Eddington limit, the Eddington number for cycling, and his pivotal role in establishing relativity and theoretical astrophysics as cornerstones of modern science. The Eddington Medal of the Royal Astronomical Society is named in his honor.

Category:English astrophysicists Category:Fellows of the Royal Society Category:1882 births Category:1944 deaths