Science and the Unseen World

· Pickle Partners Publishing
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Ukadiriaji na maoni hayajahakikishwa  Pata Maelezo Zaidi

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Physicist and astronomer Arthur Eddington tested Einstein's Theory of Relativity at an eclipse in 1919. A lifelong Quaker, his 1929 Swarthmore Lecture explores how science and religion define and look at reality. ‘You will understand the true spirit neither of science nor of religion unless seeking is placed in the forefront.’ ‘He puts a strong line against simplistic reductionism in relation to our minds . He emphasizes that when we ask the question, “What are we to think of it all? What is it all about?,” the answer must embrace but not be limited to the scientific answer. His lecture explores this in a delightful way, that remains fully relevant today.’ — Prof. George Ellis 'The attitude of the scientist, here so admirably explained, is the attitude, also, of the mystic. Experience, to both, is what matters most.”’- The Sufi Quarterly, 1929.

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Sir Arthur Stanley Eddington OM FRS (28 December 1882 - 22 November 1944) was an English astronomer, physicist, and mathematician of the early 20th century who did his greatest work in astrophysics. He was also a philosopher of science and a populariser of science. 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 anticipated 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. Eddington is famous for his work concerning the theory of relativity. He wrote a number of articles that announced and explained Einstein’s theory of general relativity to the English-speaking world. World War I severed many lines of scientific communication and new developments in German science were not well-known in England. He also conducted an expedition to observe the solar eclipse of 29 May 1919 that provided one of the earliest confirmations of general relativity, and he became known for his popular expositions and interpretations of the theory.

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