Solar eclipse of May 18, 1901 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | −0.3626 |
Magnitude | 1.068 |
Maximum eclipse | |
Duration | 389 s (6 min 29 s) |
Coordinates | 1°42′S 98°24′E / 1.7°S 98.4°E |
Max. width of band | 238 km (148 mi) |
Times (UTC) | |
Greatest eclipse | 5:33:48 |
References | |
Saros | 136 (31 of 71) |
Catalog # (SE5000) | 9283 |
A total solar eclipse occurred at the Moon's descending node of orbit on Saturday, May 18, 1901,[1][2][3][4][5] with a magnitude of 1.068. 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 only about 23 hours after perigee (on May 17, 1901, at 6:50 UTC), the Moon's apparent diameter was larger.[6]
The path of totality crossed French Madagascar (the part now belonging to Madagascar), Réunion, British Mauritius (now Mauritius), Dutch East Indies (now Indonesia), and British New Guinea (now belonging to Papua New Guinea). A partial eclipse was visible for parts of East Africa, South Asia, Southeast Asia, Australia, and Western Oceania.