Solar eclipse of August 9, 1896
Solar eclipse of August 9, 1896 | |
---|---|
Map | |
Type of eclipse | |
Nature | Total |
Gamma | 0.6964 |
Magnitude | 1.0392 |
Maximum eclipse | |
Duration | 163 sec (2 m 43 s) |
Coordinates | 54°24′N 132°12′E / 54.4°N 132.2°E |
Max. width of band | 182 km (113 mi) |
Times (UTC) | |
Greatest eclipse | 5:09:00 |
References | |
Saros | 124 (48 of 73) |
Catalog # (SE5000) | 9272 |
A total solar eclipse occurred on August 9, 1896. 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. It was visible across Europe, Asia, and Japan.
Observations
Related eclipses
It is a part of solar Saros 124.
References
- NASA graphics
- Corona and Coronet: Being a narrative of the Amherst Eclipse Expedition to Japan, in Mr. James's Schooner-Yacht Coronet, to Observe the Sun's Total Obscuration, 9th August, 1896, by Mabel Loomis Todd, Houghton, Mifflin and Company, publishers, 1898
- Total Eclipses of the Sun, By Mabel Loomis Todd, 1894, new and revised edition by David P. Todd, 1900.
- Solar eclipse of August 9, 1896 in Russia
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