Solar eclipse of October 10, 1912
| Total eclipse | |
| Gamma | −0.4149 |
|---|---|
| Magnitude | 1.0229 |
| Maximum eclipse | |
| Duration | 115 s (1 min 55 s) |
| Coordinates | 28°06′S 40°06′W / 28.1°S 40.1°W |
| Max. width of band | 85 km (53 mi) |
| Times (UTC) | |
| Greatest eclipse | 13:36:14 |
| References | |
| Saros | 142 (17 of 72) |
| Catalog # (SE5000) | 9309 |
A total solar eclipse occurred at the Moon's descending node of orbit on Thursday, October 10, 1912, with a magnitude of 1.0229. 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 2.8 days after perigee (on October 7, 1912, at 18:50 UTC), the Moon's apparent diameter was larger.
Totality was visible from Ecuador, Colombia, northern tip of Peru and Brazil. A partial eclipse was visible for parts of Central America, the Caribbean, South America, Antarctica, and Southern Africa.