Solar eclipse of December 23, 1908
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Solar eclipse of December 23, 1908 | |
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Type of eclipse | |
Nature | Hybrid |
Gamma | -0.4985 |
Magnitude | 1.0024 |
Maximum eclipse | |
Duration | 12 sec (0 m 12 s) |
Coordinates | Lua error in package.lua at line 80: module 'strict' not found. |
Max. width of band | 10 km (6.2 mi) |
Times (UTC) | |
Greatest eclipse | 11:44:28 |
References | |
Saros | 140 (23 of 71) |
Catalog # (SE5000) | 9301 |
A total solar eclipse occurred on December 23, 1908. 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.
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 |
|
125 | July 10, 1907![]() Annular |
130 | January 3, 1908![]() Total |
|
135 | June 28, 1908![]() Annular |
140 | December 23, 1908![]() Hybrid |
|
145 | June 17, 1909![]() Hybrid |
150 | December 12, 1909![]() Partial |
References
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- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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