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Solar eclipse of April 17, 1912 ：ウィキペディア英語版

Solar eclipse of April 17, 1912

A total solar eclipse occurred on April 17, 1912. It is a hybrid event, starting and ending as an annular eclipse, with only a small portion of totality. 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 over the sea between Spain and France, with annularity continued northeast across Europe and Asia.
This eclipse occurred two days after the RMS ''Titanic'' sank in the northwestern Atlantic ocean under the darkness of new moon.〔(www.astronomeer.com: The "Titanic" eclipse of 17 April 1912 ) ''The last annular eclipse in the Netherlands was 17 April 1912, just two days after the Titanic hit an iceberg and sank.''〕
== Observations ==

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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