Solar eclipse of March 21, 2099

Last updated
Solar eclipse of March 21, 2099
SE2099Mar21A.png
Map
Type of eclipse
NatureAnnular
Gamma −0.4016
Magnitude 0.93
Maximum eclipse
Duration452 sec (7 m 32 s)
Coordinates 20°S149°W / 20°S 149°W / -20; -149
Max. width of band275 km (171 mi)
Times (UTC)
Greatest eclipse22:54:32
References
Saros 131 (55 of 70)
Catalog # (SE5000) 9731

An annular solar eclipse will occur on Saturday, March 21, 2099. 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.

Contents

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]

Solar eclipses 2098–2100
121 April 1, 2098
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Partial
126 September 25, 2098
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Partial
131 March 21, 2099
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Annular
136 September 14, 2099
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Total
141 March 10, 2100
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Annular
146 September 4, 2100
SE2100Sep04T.png
Total

Inex series

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Saros 131

It is a part of Saros cycle 131, repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on August 1, 1125. It contains total eclipses from March 27, 1522 through May 30, 1612 and hybrid eclipses from June 10, 1630 through July 24, 1702, and annular eclipses from August 4, 1720 through June 18, 2243. The series ends at member 70 as a partial eclipse on September 2, 2369. The longest duration of totality was only 58 seconds on May 30, 1612. All eclipses in this series occurs at the Moon’s ascending node.

Series members 33–70 occur between 1702 and 2369
333435
SE1702Jul24H.png
July 24, 1702
SE1720Aug04A.png
August 4, 1720
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August 15, 1738
363738
SE1756Aug25A.png
August 25, 1756
SE1774Sep06A.png
September 6, 1774
SE1792Sep16A.png
September 16, 1792
394041
SE1810Sep28A.png
September 28, 1810
SE1828Oct09A.png
October 9, 1828
SE1846Oct20A.png
October 20, 1846
424344
SE1864Oct30A.png
October 30, 1864
SE1882Nov10A.png
November 10, 1882
SE1900Nov22A.png
November 22, 1900
454647
SE1918Dec03A.png
December 3, 1918
SE1936Dec13A.png
December 13, 1936
SE1954Dec25A.png
December 25, 1954
484950
SE1973Jan04A.png
January 4, 1973
SE1991Jan15A.png
January 15, 1991
SE2009Jan26A.png
January 26, 2009
515253
SE2027Feb06A.png
February 6, 2027
SE2045Feb16A.png
February 16, 2045
SE2063Feb28A.png
February 28, 2063
545556
SE2081Mar10A.png
March 10, 2081
SE2099Mar21A.png
March 21, 2099
SE2117Apr02A.png
April 2, 2117
575859
SE2135Apr13A.png
April 13, 2135
SE2153Apr23A.png
April 23, 2153
SE2171May05A.png
May 5, 2171
606162
SE2189May15A.png
May 15, 2189
SE2207May27A.png
May 27, 2207
SE2225Jun06A.png
June 6, 2225
636465
SE2243Jun18A.png
June 18, 2243
SE2261Jun28P.png
June 28, 2261
SE2279Jul09P.png
July 9, 2279
666768
SE2297Jul20P.png
July 20, 2297
SE2315Aug01P.png
August 1, 2315
SE2333Aug11P.png
August 11, 2333
6970
SE2351Aug22P.png
August 22, 2351
SE2369Sep02P.png
September 2, 2369

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.

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References