Solar eclipse of January 22, 1898 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | 0.5079 |
Magnitude | 1.0244 |
Maximum eclipse | |
Duration | 141 s (2 min 21 s) |
Coordinates | 9°30′N 63°36′E / 9.5°N 63.6°E |
Max. width of band | 96 km (60 mi) |
Times (UTC) | |
Greatest eclipse | 7:19:12 |
References | |
Saros | 139 (23 of 71) |
Catalog # (SE5000) | 9275 |
A total solar eclipse occurred at the Moon's ascending node of orbit on Saturday, January 22, 1898. 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 1.8 days after perigee (on January 20, 1898, at 12:30 UTC), the Moon's apparent diameter was larger.[1]
The path of totality was visible from parts of the Royal Niger Company, Kamerun, Upper Ubanghi, British East Africa, Abyssinia, Italian Somaliland, Hindustan, Nepal, and the Chinese Empire. A partial solar eclipse was also visible for much of Africa, Europe, and Asia.