Solar eclipse of May 21, 2031

Summary

An annular solar eclipse will occur on Wednesday, May 21, 2031. 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 (Apogee on May 25, 2031), the Moon's apparent diameter will be smaller.

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

Images edit

 
Animated path

Related eclipses edit

Solar eclipses 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
118 June 12, 2029
 
Partial
123 December 5, 2029
 
Partial
128 June 1, 2030
 
Annular
133 November 25, 2030
 
Total
138 May 21, 2031
 
Annular
143 November 14, 2031
 
Hybrid
148 May 9, 2032
 
Annular
153 November 3, 2032
 
Partial

Saros 138 edit

It is a part of Saros cycle 138, repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on June 6, 1472. It contains annular eclipses from August 31, 1598 through February 18, 2482 with a hybrid eclipse on March 1, 2500. It has total eclipses from March 12, 2518 through April 3, 2554. The series ends at member 70 as a partial eclipse on July 11, 2716. The longest duration of totality will be only 56 seconds on April 3, 2554.


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.[2]

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. ^ 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

  • NASA graphics