A total solar eclipse occurred on Sunday, February 9, 1766. 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.
Observations
Related eclipses
It is a part of solar Saros 117.
References
- Mabel Loomis Todd (1900). Total Eclipses of the Sun. Little, Brown.
- NASA chart graphics
- Googlemap
- NASA Besselian elements
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