Solar eclipse of August 10, 1915 | |
---|---|
Type of eclipse | |
Nature | Annular |
Gamma | 0.0124 |
Magnitude | 0.9853 |
Maximum eclipse | |
Duration | 93 s (1 min 33 s) |
Coordinates | 16°24′N 161°24′W / 16.4°N 161.4°W |
Max. width of band | 52 km (32 mi) |
Times (UTC) | |
Greatest eclipse | 22:52:25 |
References | |
Saros | 134 (38 of 71) |
Catalog # (SE5000) | 9316 |
An annular solar eclipse occurred at the Moon's descending node of orbit between Tuesday, August 10 and Wednesday, August 11, 1915,[1][2][3][4] with a magnitude of 0.9853. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring 5.8 days after apogee (on August 5, 1915, at 2:40 UTC), the Moon's apparent diameter was smaller.[5]
Annularity was visible from the Pacific Ocean, with the only land being Haha-jima Group in Japan, where the eclipse occurred on August 11 because it is west of International Date Line. A partial eclipse was visible for parts of Northeast Asia, northern Oceania, and Hawaii.