| 词条 | Solar eclipse of May 9, 1910 |
| 释义 |
A total solar eclipse occurred on May 9, 1910. 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 from part of Wilkes Land in Antarctica and Tasmania in Australia. Related eclipsesSolar eclipses of 1910-1913{{Solar eclipse set 1910-1913}}References{{Solar eclipse NASA reference|1901/SE1910May09T|19101102}}{{Solar eclipses}}{{Solar-eclipse-stub}} 4 : Total solar eclipses|1910 in science|20th-century solar eclipses|May 1910 events |
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