Solar eclipse of December 23, 1908 | |
---|---|
Type of eclipse | |
Nature | Hybrid |
Gamma | −0.4985 |
Magnitude | 1.0024 |
Maximum eclipse | |
Duration | 12 s (0 min 12 s) |
Coordinates | 53°24′S 0°30′W / 53.4°S 0.5°W |
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 at the Moon's descending node of orbit on Wednesday, December 23, 1908,[1][2][3][4] with a magnitude of 1.0024. It was a hybrid event, with only a fraction of its path as total, and longer sections at the start and end as an annular eclipse. 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. Occurring about 3.1 days before perigee (on December 26, 1908, at 13:30 UTC), the Moon's apparent diameter was larger.[5]
Annularity was visible from Chile, Argentina, Uruguay and southern Brazil, while totality was visible only from southern Atlantic Ocean with no land. A partial eclipse was visible for parts of northern South America, most of North America, the Caribbean, West Africa, North Africa, and Western Europe.