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Solar eclipse of May 21, 2031

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Solar eclipse of May 21, 2031
Map
Type of eclipse
NatureAnnular
Gamma−0.197
Magnitude0.9589
Maximum eclipse
Duration326 s (5 min 26 s)
Coordinates8°54′N 71°42′E / 8.9°N 71.7°E / 8.9; 71.7
Max. width of band152 km (94 mi)
Times (UTC)
Greatest eclipse7:16:04
References
Saros138 (32 of 70)
Catalog # (SE5000)9577

An annular solar eclipse will occur at the Moon's descending node of orbit on Wednesday, May 21, 2031, with a magnitude of 0.9589. 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 3.8 days before apogee ( on May 25, 2031), the Moon's apparent diameter will be smaller.

Images[edit]


Animated path

Related eclipses[edit]

Eclipses of 2031[edit]

Metonic[edit]

Tzolkinex[edit]

Half-Saros[edit]

Tritos[edit]

Solar Saros 138[edit]

Inex[edit]

Triad[edit]

Solar eclipses of 2029–2032[edit]

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]

Note: Partial solar eclipses on January 14, 2029 and July 11, 2029 occur on the previous lunar year eclipse set.

Solar eclipse series sets from 2029 to 2032
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
118 June 12, 2029

Partial
1.29431 123 December 5, 2029

Partial
-1.06090
128 June 1, 2030

Annular
0.56265 133 November 25, 2030

Total
-0.38669
138 May 21, 2031

Annular
-0.19699 143 November 14, 2031

Hybrid
0.30776
148 May 9, 2032

Annular
-0.93748 153 November 3, 2032

Partial
1.06431

Saros 138[edit]

This eclipse is a part of Saros series 138, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on June 6, 1472. It contains annular eclipses from August 31, 1598 through February 18, 2482; a hybrid eclipse on March 1, 2500; and total eclipses from March 12, 2518 through April 3, 2554. The series ends at member 70 as a partial eclipse on July 11, 2716. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of annularity was produced by member 23 at 8 minutes, 2 seconds on February 11, 1869, and the longest duration of totality will be produced by member 61 at 56 seconds on April 3, 2554. All eclipses in this series occur at the Moon’s descending node of orbit.[2]

Series members 20–41 occur between 1801 and 2200:
20 21 22

January 10, 1815

January 20, 1833

February 1, 1851
23 24 25

February 11, 1869

February 22, 1887

March 6, 1905
26 27 28

March 17, 1923

March 27, 1941

April 8, 1959
29 30 31

April 18, 1977

April 29, 1995

May 10, 2013
32 33 34

May 21, 2031

May 31, 2049

June 11, 2067
35 36 37

June 22, 2085

July 4, 2103

July 14, 2121
38 39 40

July 25, 2139

August 5, 2157

August 16, 2175
41

August 26, 2193

Metonic series[edit]

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's descending node.[3]

Octon series with 21 events between May 21, 1993 and August 2, 2065
May 20–21 March 8–9 December 25–26 October 13–14 August 1–2
98 100 102 104 106
May 21, 1955 March 9, 1959 December 26, 1962 October 14, 1966 August 2, 1970
108 110 112 114 116
May 21, 1974 March 9, 1978 December 26, 1981 October 14, 1985 August 1, 1989
118 120 122 124 126

May 21, 1993

March 9, 1997

December 25, 2000

October 14, 2004

August 1, 2008
128 130 132 134 136

May 20, 2012

March 9, 2016

December 26, 2019

October 14, 2023

August 2, 2027
138 140 142 144 146

May 21, 2031

March 9, 2035

December 26, 2038

October 14, 2042

August 2, 2046
148 150 152 154 156

May 20, 2050

March 9, 2054

December 26, 2057

October 13, 2061

August 2, 2065
158 160 162 164 166

May 20, 2069
March 8, 2073 December 26, 2076 October 13, 2080 August 1, 2084

References[edit]

  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.
  2. ^ "NASA - Catalog of Solar Eclipses of Saros 138". eclipse.gsfc.nasa.gov.
  3. ^ Note S1: Eclipses & Predictions in Freeth, Tony (2014). "Eclipse Prediction on the Ancient Greek Astronomical Calculating Machine Known as the Antikythera Mechanism". PLOS ONE. 9 (7): e103275. Bibcode:2014PLoSO...9j3275F. doi:10.1371/journal.pone.0103275. PMC 4116162. PMID 25075747.

External links[edit]