翻訳と辞書 ・ Solar eclipse of May 19, 1985 ・ Solar eclipse of May 2, 2087 ・ Solar eclipse of May 20, 1947 ・ Solar eclipse of May 20, 1966 ・ Solar eclipse of May 20, 2012 ・ Solar eclipse of May 20, 2050 ・ Solar eclipse of May 20, 2069 ・ Solar eclipse of May 21, 1993 ・ Solar eclipse of May 21, 2031 ・ Solar eclipse of May 22, 1724 ・ Solar eclipse of May 22, 2058 ・ Solar eclipse of May 22, 2077 ・ Solar eclipse of May 22, 2096 ・ Solar eclipse of May 26, 1854 ・ Solar eclipse of May 28, 1900 ・ Solar eclipse of May 29, 1919 ・ Solar eclipse of May 29, 1938 ・ Solar eclipse of May 3, 1715 ・ Solar eclipse of May 30, 1946 ・ Solar eclipse of May 30, 1965 ・ Solar eclipse of May 30, 1984 ・ Solar eclipse of May 31, 2003 ・ Solar eclipse of May 31, 2049 ・ Solar eclipse of May 31, 2068 ・ Solar eclipse of May 6, 1883 ・ Solar eclipse of May 7, 1902 ・ Solar eclipse of May 9, 1910 ・ Solar eclipse of May 9, 1929 ・ Solar eclipse of May 9, 1948 ・ Solar eclipse of May 9, 1967
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Solar eclipse of May 29, 1919 : ウィキペディア英語版 | Solar eclipse of May 29, 1919
A total solar eclipse occurred on May 29, 1919. With a maximum duration of totality of 6 minutes 51 seconds, it was one of the longest solar eclipses of the 20th century. It was visible throughout most of South America and Africa as a partial eclipse. Totality occurred through a narrow path across central Brazil after sunrise, across the Atlantic ocean and into south central Africa ending near sunset in eastern Africa. ==Observations==
This eclipse was photographed from the expedition of Sir Arthur Eddington to the island of Principe (off the west coast of Africa). Positions of star images within the field near the Sun were used to test Albert Einstein's prediction of the bending of light around the Sun from his general theory of relativity.〔(F. W. Dyson, A. S. Eddington, and C. Davidson, "A Determination of the Deflection of Light by the Sun's Gravitational Field, from Observations Made at the Total Eclipse of May 29, 1919" Philosophical Transactions of the Royal Society of London. Series A, Containing Papers of a Mathematical or Physical Character (1920): 291–333, on 332. )〕
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