k 1919 solar eclipse 1919 solar eclipse. Image 1 of 3. This set of images, taken by the British astronomer Arthur Eddington 18821944, confirmed Einsteins theory of general relativity. The stars near the Sun appear slightly shifted because their light is curved by its gravitational field. This shift is only noticeable during a solar eclipse as at other times the Suns brightness obscures the stars. This is a total solar eclipse, when the moon fits over the Sun so only its corona atmosphere is visible. Image taken from Principe Island, Gulf of Guinea, on 29 May 1919. For a sequence of the eclipse see R506416R506418. Stock Photo - Afloimages
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1919 solar eclipse 1919 solar eclipse. Image 1 of 3. This set of images, taken by the British astronomer Arthur Eddington  1882 1944 , confirmed Einstein s theory of general relativity. The stars near the Sun appear slightly shifted because their light is curved by its gravitational field. This shift is only noticeable during a solar eclipse as at other times the Sun s brightness obscures the stars. This is a total solar eclipse, when the moon fits over the Sun so only its corona  atmosphere  is visible. Image taken from Principe Island, Gulf of Guinea, on 29 May 1919. For a sequence of the eclipse see R506 416 R506 418.
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1919 solar eclipse

1919 solar eclipse. Image 1 of 3. This set of images, taken by the British astronomer Arthur Eddington (1882-1944), confirmed Einstein's theory of general relativity. The stars near the Sun appear slightly shifted because their light is curved by its gravitational field. This shift is only noticeable during a solar eclipse as at other times the Sun's brightness obscures the stars. This is a total solar eclipse, when the moon fits over the Sun so only its corona (atmosphere) is visible. Image taken from Principe Island, Gulf of Guinea, on 29 May 1919. For a sequence of the eclipse see R506/416-R506/418.

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