Solar eclipse of May 22, 2077
Map
Type of eclipse
NatureTotal
Gamma−0.5725
Magnitude1.029
Maximum eclipse
Duration174 sec (2 m 54 s)
Coordinates13°06′S 148°18′E / 13.1°S 148.3°E / -13.1; 148.3
Max. width of band119 km (74 mi)
Times (UTC)
Greatest eclipse2:46:05
References
Saros129 (55 of 80)
Catalog # (SE5000)9681

A total solar eclipse will occur on Saturday, May 22, 2077. 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.

Tritos

Tzolkinex

Solar eclipses 2076–2079

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 eclipse series sets from 2076–2079
Ascending node   Descending node
SarosMap SarosMap
119June 1, 2076

Partial		 124November 26, 2076

Partial
129May 22, 2077

Total		 134November 15, 2077

Annular
139May 11, 2078

Total		 144November 4, 2078

Annular
149May 1, 2079

Total		 154October 24, 2079

Annular

Saros 129

It is a part of Saros cycle 129, repeating every 18 years, 11 days, containing 80 events. The series started with partial solar eclipse on October 3, 1103. It contains annular eclipses on May 6, 1464 through March 18, 1969, hybrid eclipses from March 29, 1987 through April 20, 2023 and total eclipses from April 30, 2041 through July 26, 2185. The series ends at member 80 as a partial eclipse on February 21, 2528. The longest duration of totality was 3 minutes, 43 seconds on June 25, 2131 . All eclipses in this series occurs at the Moon’s ascending node.[2]

Series members 46–56 occur between 1901 and 2100:
46 47 48

February 14, 1915
February 24, 1933
March 7, 1951
49 50 51

March 18, 1969
March 29, 1987
April 8, 2005
52 53 54

April 20, 2023
April 30, 2041
May 11, 2059
55 56

May 22, 2077
June 2, 2095

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.

In the 19th century:

  • Solar Saros 120: Total Solar Eclipse of 1816 Nov 19
  • Solar Saros 121: Hybrid Solar Eclipse of 1845 Oct 30
  • Solar Saros 122: Annular Solar Eclipse of 1874 Oct 10

In the 22nd century:

  • Solar Saros 130: Total Solar Eclipse of 2106 May 03
  • Solar Saros 131: Annular Solar Eclipse of 2135 Apr 13
  • Solar Saros 132: Hybrid Solar Eclipse of 2164 Mar 23
  • Solar Saros 133: Total Solar Eclipse of 2193 Mar 03

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.
  2. ↑ Espenak, F. "NASA Catalog of Solar Eclipses of Saros 129". eclipse.gsfc.nasa.gov.

References

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