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Solar eclipse of September 7, 1820

An annular solar eclipse occurred at the Moon's descending node of orbit on Thursday, September 7, 1820, with a magnitude of 0.9329. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring only about 5 hours before apogee, the Moon's apparent diameter was smaller.

Observation and prediction
This map was drawn in the book Elementa eclipsium, published in Prague in 1816, by Franz Ignaz Cassian Hallaschka (František Ignác Kassián Halaška) (1780-1847), contained maps of the paths of solar eclipses from 1816 and 1860. The geometric constructions used by Hallaschka anticipated the standard theory of eclipses later developed by Friedrich Wilhelm Bessel. == Eclipse details ==
Eclipse details
Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the Moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse. == Eclipse season ==
Eclipse season
This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight. == Related eclipses ==
Related eclipses
Eclipses in 1820 A total solar eclipse on March 14. • A partial lunar eclipse on March 29. • An annular solar eclipse on September 7.A partial lunar eclipse on September 22. Metonic • Preceded by: Solar eclipse of November 19, 1816 • Followed by: Solar eclipse of June 26, 1824 Tzolkinex • Preceded by: Solar eclipse of July 27, 1813 • Followed by: Solar eclipse of October 20, 1827 Half-Saros • Preceded by: Lunar eclipse of September 2, 1811 • Followed by: Lunar eclipse of September 13, 1829 Tritos • Preceded by: Solar eclipse of October 9, 1809 • Followed by: Solar eclipse of August 7, 1831 Solar Saros 122 • Preceded by: Solar eclipse of August 28, 1802 • Followed by: Solar eclipse of September 18, 1838 Inex • Preceded by: Solar eclipse of September 27, 1791 • Followed by: Solar eclipse of August 18, 1849 Triad • Preceded by: Solar eclipse of November 6, 1733 • Followed by: Solar eclipse of July 10, 1907 Solar eclipses of 1819–1823 The partial solar eclipses on April 24, 1819 and October 19, 1819 occur in the previous lunar year eclipse set, and the partial solar eclipses on January 12, 1823 and July 8, 1823 occur in the next lunar year eclipse set. Saros 122 Metonic series All eclipses in this table occur at the Moon's descending node. Tritos series Inex series ==Notes==
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