Solar eclipse of November 30, 1853
Introduction 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 280px
Related eclipses === Solar eclipse set 1852-1855=== Solar eclipse series sets from 1852 to 1855Ascending node Descending node115June 17, 1852150pxPartial120December 11, 1852150pxTotal125June 6, 1853150pxAnnular130November 30, 1853150pxTotal135May 26, 1854150pxAnnular140November 20, 1854150pxHybrid145May 16, 1855150pxPartial150November 9, 1855150pxPartial=== 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).