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).

Solar eclipse of November 30, 1853

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1853 in science

1853 11 30

November 1853 events

Solar eclipse of November 30, 1853