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Solar eclipse of April 6, 1875 ：ウィキペディア英語版

Solar eclipse of April 6, 1875

A total solar eclipse occurred on April 6, 1875. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.
Totality was visible on the southern tip of Africa, across the Indian ocean, and across southeastern Asia.
== Observations ==
Astronomers J. N. Lockyer and Arthur Schuster traveled to observe the eclipse and measure spectral lines to determine the elemental contents of the solar corona.〔(Report on the Total Solar Eclipse of April 6, 1875 ) by J. N. Lockyer and Arthur Schuster, 1878, The Royal Society ()〕
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抄文引用元・出典: フリー百科事典『ウィキペディア（Wikipedia）』
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