Solar eclipse of June 17, 1909
Lua error in Module:Infobox at line 235: malformed pattern (missing ']'). A total 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 is a hybrid, starting and ending as an annular eclipse.
The path of totality crossed Arctic ocean, Canada, Greenland, central Russia, central Asia.
Related eclipses
Solar eclipses 1906-1909
Each member in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.
| Ascending node | Descending node | |||
|---|---|---|---|---|
| 115 | July 21, 1906 Partial |
120 | January 14, 1907 Total |
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| 125 | July 10, 1907 Annular |
130 | January 3, 1908 Total |
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| 135 | June 28, 1908 Annular |
140 | December 23, 1908 Hybrid |
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| 145 | June 17, 1909 Hybrid |
150 | December 12, 1909 Partial |
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External links
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<references />, or <references group="..." />- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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