Solar eclipse of April 6, 1875 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | −0.1292 |
Magnitude | 1.0547 |
Maximum eclipse | |
Duration | 277 s (4 min 37 s) |
Coordinates | 0°12′S 84°48′E / 0.2°S 84.8°E |
Max. width of band | 182 km (113 mi) |
Times (UTC) | |
Greatest eclipse | 6:37:26 |
References | |
Saros | 127 (50 of 82) |
Catalog # (SE5000) | 9222 |
A total solar eclipse occurred at the Moon's ascending node of orbit on Tuesday, April 6, 1875, with a magnitude of 1.0547. 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 1.2 days before perigee (on April 7, 1875, at 10:50 UTC), the Moon's apparent diameter was larger.[1]
The path of totality was visible from parts of the modern-day Andaman and Nicobar Islands, Myanmar, Thailand, northwestern Cambodia, Laos, Vietnam, and southern Hainan. A partial solar eclipse was also visible for parts of Southern Africa, South Asia, Southeast Asia, and East Asia.