翻訳と辞書 ・ Solar eclipse of September 2, 1997 ・ Solar eclipse of September 2, 2035 ・ Solar eclipse of September 2, 2054 ・ Solar eclipse of September 20, 1960 ・ Solar eclipse of September 21, 1903 ・ Solar eclipse of September 21, 1922 ・ Solar eclipse of March 7, 1951 ・ Solar eclipse of March 7, 1970 ・ Solar eclipse of March 7, 1989 ・ Solar eclipse of March 9, 1997 ・ Solar eclipse of March 9, 2016 ・ Solar eclipse of March 9, 2035 ・ Solar eclipse of March 9, 2054 ・ Solar eclipse of May 1, 2079 ・ Solar eclipse of May 10, 1994 ・ Solar eclipse of May 10, 2013 ・ Solar eclipse of May 11, 1975 ・ Solar eclipse of May 11, 2040 ・ Solar eclipse of May 11, 2059 ・ Solar eclipse of May 11, 2078 ・ Solar eclipse of May 11, 2097 ・ Solar eclipse of May 17, 1882 ・ Solar eclipse of May 18, 1901 ・ Solar eclipse of May 18, 1920 ・ Solar eclipse of May 19, 1928 ・ 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
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Solar eclipse of May 10, 2013 : ウィキペディア英語版 | Solar eclipse of May 10, 2013
An annular solar eclipse took place on May 9–10 (UTC), 2013, with a magnitude of 0.9544. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. == Visibility == Annularity was visible from a 171 to 225 kilometre-wide track that traversed Australia, eastern Papua New Guinea, the Solomon Islands, and the Gilbert Islands, with the maximum of 6 minutes 3 seconds visible from the Pacific Ocean east of French Polynesia.
抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)』 ■ウィキペディアで「Solar eclipse of May 10, 2013」の詳細全文を読む
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