Solar eclipse of December 12, 1871 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | 0.1836 |
Magnitude | 1.0465 |
Maximum eclipse | |
Duration | 263 s (4 min 23 s) |
Coordinates | 12°42′S 119°24′E / 12.7°S 119.4°E |
Max. width of band | 157 km (98 mi) |
Times (UTC) | |
Greatest eclipse | 4:03:38 |
References | |
Saros | 130 (44 of 73) |
Catalog # (SE5000) | 9215 |
A total solar eclipse occurred at the Moon's descending node of orbit on Tuesday, December 12, 1871, with a magnitude of 1.0465. 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 10.5 hours before perigee (on December 12, 1871, at 14:40 UTC), the Moon's apparent diameter was larger.[1]
The path of totality was visible from parts of modern-day India, Indonesia, Australia, and the Solomon Islands. A partial solar eclipse was also visible for parts of the Middle East, Central Asia, South Asia, Southeast Asia, Australia, and Oceania.