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Solar eclipse of August 21, 1560 | |
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Type of eclipse | |
Nature | Total |
Gamma | 0.405 |
Magnitude | 1.0469 |
Maximum eclipse | |
Duration | 225 s (3 min 45 s) |
Coordinates | 29°42′N 5°18′E / 29.7°N 5.3°E |
Max. width of band | 170 km (110 mi) |
Times (UTC) | |
Greatest eclipse | 12:30:55 |
References | |
Saros | 118 (43 of 72) |
Catalog # (SE5000) | 8451 |
A total solar eclipse occurred on August 21, 1560. 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. It's an astronomical phenomenon where, during the moon's orbit around Earth, it passes in from the Sun and causes a solar eclipse. People can't view it with the naked eye, with consequences are horrible as losing your eyesight. Most of the first stages of a solar eclipse can be visible with the naked eye.[1] 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 kilometers wide. This eclipse is part of solar Saros 118.