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Solar eclipse of September 4, 2100

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Solar eclipse of September 4, 2100
Map
Type of eclipse
NatureTotal
Gamma−0.3384
Magnitude1.0402
Maximum eclipse
Duration212 s (3 min 32 s)
Coordinates10°30′S 39°00′E / 10.5°S 39°E / -10.5; 39
Max. width of band142 km (88 mi)
Times (UTC)
Greatest eclipse8:49:20
References
Saros146 (32 of 76)
Catalog # (SE5000)9734

A total solar eclipse is forecast to occur on September 4, 2100. 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.

Solar eclipses 2098-2100

This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[1]

The partial solar eclipse on October 24, 2098 occurs in the previous lunar year eclipse set.

Solar eclipse series sets from 2098 to 2101
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
121 April 1, 2098

Partial 		−1.1005 126 September 25, 2098

Partial 		1.14
131 March 21, 2099

Annular 		−0.4016 136 September 14, 2099

Total 		0.3942
141 March 10, 2100

Annular 		0.3077 146 September 4, 2100

Total 		−0.3384
151 February 28, 2101

Annular 		0.9964 156 August 24, 2101

Partial 		−1.1392

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200

December 21, 1805
(Saros 119)
November 19, 1816
(Saros 120)
October 20, 1827
(Saros 121)
September 18, 1838
(Saros 122)
August 18, 1849
(Saros 123)

July 18, 1860
(Saros 124)
June 18, 1871
(Saros 125)
May 17, 1882
(Saros 126)
April 16, 1893
(Saros 127)
March 17, 1904
(Saros 128)

February 14, 1915
(Saros 129)
January 14, 1926
(Saros 130)
December 13, 1936
(Saros 131)
November 12, 1947
(Saros 132)
October 12, 1958
(Saros 133)

September 11, 1969
(Saros 134)
August 10, 1980
(Saros 135)
July 11, 1991
(Saros 136)
June 10, 2002
(Saros 137)
May 10, 2013
(Saros 138)

April 8, 2024
(Saros 139)
March 9, 2035
(Saros 140)
February 5, 2046
(Saros 141)
January 5, 2057
(Saros 142)
December 6, 2067
(Saros 143)

November 4, 2078
(Saros 144)
October 4, 2089
(Saros 145)
September 4, 2100
(Saros 146)
August 4, 2111
(Saros 147)
July 4, 2122
(Saros 148)

June 3, 2133
(Saros 149)
May 3, 2144
(Saros 150)
April 2, 2155
(Saros 151)
March 2, 2166
(Saros 152)
January 29, 2177
(Saros 153)

December 29, 2187
(Saros 154)
November 28, 2198
(Saros 155)

Notes

  1. ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.

References

Wikimedia Commons has media related to Solar eclipse of 2100 September 4.


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