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Solar eclipse of March 4, 1802 ：ウィキペディア英語版

Solar eclipse of March 4, 1802

A total solar eclipse occurred on March 4, 1802. 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.
The eclipse was visible in Indonesia, Papua New Guinea, Australia, New Zealand and Antarctica, while the totality was seen in Australia and Antarctica.〔(【引用サイトリンク】url=http://eclipse.gsfc.nasa.gov/5MCSEmap/1801-1900/1802-03-04.gif )〕
== See also ==

* List of solar eclipses in the 19th century

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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