A total solar eclipse occurred on November 30, 1853. 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
Solar eclipse set 1852-1855
Saros 130
References
NASA chart graphics
Googlemap
NASA Besselian elements
The total eclipse of the sun of November 30, 1853 Astronomical Journal, vol. 3, iss. 67, p. 145–146 (1854).

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