Solar eclipse of December 23, 1908 | |
---|---|
Map
|
|
Type of eclipse | |
Nature | Hybrid |
Gamma | -0.4985 |
Magnitude | 1.0024 |
Maximum eclipse | |
Duration | 0m 12s |
Coordinates | 53.4S 0.5W |
Max. width of band | 10 km |
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 partially 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, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across the surface of the Earth, while a partial solar eclipse will be visible over a region thousands of kilometres wide. This event is a hybrid, starting and ending as an annular eclipse.
This set of solar eclipses repeat approximately every 177 days and 4 hours 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 |