| 词条 | Solar eclipse of June 17, 1909 |
| 释义 |
A hybrid solar eclipse occurred on June 17, 1909. 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. This event was a hybrid, starting and ending as an annular eclipse. The path of totality crossed central Russia, the Arctic Ocean, northeastern Ellesmere Island in Canada, Greenland, , and annularity crossed southern Siberia in Russia (now in northeastern Kazakhstan and southern Russia) and southern Greenland. Related eclipsesSolar eclipses 1906-1909{{Solar eclipse set 1906-1909}}External links{{Solar eclipse NASA reference|1901/SE1909Jun17H|19090617}}{{Solar eclipses}}{{Solar-eclipse-stub}} 4 : Total solar eclipses|20th-century solar eclipses|1909 in science|June 1909 events |
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