Solar eclipse of May 28, 1900 | |
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![]() Totality photographed in Wadesboro, North Carolina, by Thomas Smillie for the Smithsonian Solar Eclipse Expedition to capture photographic proof of the solar corona | |
Type of eclipse | |
Nature | Total |
Gamma | 0.3943 |
Magnitude | 1.0249 |
Maximum eclipse | |
Duration | 130 s (2 min 10 s) |
Coordinates | 44°48′N 46°30′W / 44.8°N 46.5°W |
Max. width of band | 92 km (57 mi) |
Times (UTC) | |
Greatest eclipse | 14:53:56 |
References | |
Saros | 126 (41 of 72) |
Catalog # (SE5000) | 9281 |
A total solar eclipse occurred on May 28, 1900.[1] 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.
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