Solar eclipse of May 20, 2050

Last updated

Solar eclipse of May 20, 2050
SE2050May20H.png
Map
Type of eclipse
NatureHybrid
Gamma −0.8688
Magnitude 1.0038
Maximum eclipse
Duration21 s (0 min 21 s)
Coordinates 40°06′S123°42′W / 40.1°S 123.7°W / -40.1; -123.7
Max. width of band27 km (17 mi)
Times (UTC)
Greatest eclipse20:42:50
References
Saros 148 (23 of 75)
Catalog # (SE5000) 9619

A total solar eclipse will occur on May 20, 2050. 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. This eclipse is a hybrid eclipse, starting and ending as an annular solar eclipse.

Contents

This hybrid eclipse is notable in that it does not hit land anywhere on Earth.

Solar eclipses 2047–2050

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 lunar eclipses on January 26, 2047 and July 22, 2047 occur on the previous lunar year eclipse set.

Solar eclipse sets from 2047 to 2050
Descending node Ascending node
118 June 23, 2047
SE2047Jun23P.png
Partial		123 December 16, 2047
SE2047Dec16P.png
Partial
128 June 11, 2048
SE2048Jun11A.png
Annular		133 December 5, 2048
SE2048Dec05T.png
Total
138 May 31, 2049
SE2049May31A.png
Annular		143 November 25, 2049
SE2049Nov25H.png
Hybrid
148 May 20, 2050
SE2050May20H.png
Hybrid		153 November 14, 2050
SE2050Nov14P.png
Partial

Saros 148

Solar saros 148, repeating every about 18 years and 11 days, contains 75 events. The series started with a partial solar eclipse on September 21, 1653. It has annular eclipses on April 29, 2014, and May 9, 2032, and a hybrid eclipse on May 20, 2050. It has total eclipses from May 31, 2068, to August 3, 2771. The series ends at member 75 as a partial eclipse on December 12, 2987. The longest total eclipse will be on April 26, 2609, at 5 minutes and 23 seconds. [2]

Series members 15–25 occur between 1901 and 2100:
151617
SE1906Feb23P.png
February 23, 1906 		SE1924Mar05P.png
March 5, 1924 		SE1942Mar16P.png
March 16, 1942
181920
SE1960Mar27P.png
March 27, 1960 		SE1978Apr07P.png
April 7, 1978 		SE1996Apr17P.png
April 17, 1996
212223
SE2014Apr29A.png
April 29, 2014 		SE2032May09A.png
May 9, 2032 		SE2050May20H.png
May 20, 2050
2425
SE2068May31T.png
May 31, 2068 		SE2086Jun11T.png
June 11, 2086

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:

In the 22nd century:

Metonic series

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 20–21March 8–9December 25–26October 13–14August 1–2
98100102104106
May 21, 1955March 9, 1959December 26, 1962October 14, 1966August 2, 1970
108110112114116
May 21, 1974March 9, 1978December 26, 1981October 14, 1985August 1, 1989
118120122124126
SE1993May21P.png
May 21, 1993 		SE1997Mar09T.png
March 9, 1997 		SE2000Dec25P.png
December 25, 2000 		SE2004Oct14P.png
October 14, 2004 		SE2008Aug01T.png
August 1, 2008
128130132134136
SE2012May20A.png
May 20, 2012 		SE2016Mar09T.png
March 9, 2016 		SE2019Dec26A.png
December 26, 2019 		SE2023Oct14A.png
October 14, 2023 		SE2027Aug02T.png
August 2, 2027
138140142144146
SE2031May21A.png
May 21, 2031 		SE2035Mar09A.png
March 9, 2035 		SE2038Dec26T.png
December 26, 2038 		SE2042Oct14A.png
October 14, 2042 		SE2046Aug02T.png
August 2, 2046
148150152154156
SE2050May20H.png
May 20, 2050 		SE2054Mar09P.png
March 9, 2054 		SE2057Dec26T.png
December 26, 2057 		SE2061Oct13A.png
October 13, 2061 		SE2065Aug02P.png
August 2, 2065
158160162164166
SE2069May20P.png
May 20, 2069 		March 8, 2073December 26, 2076October 13, 2080August 1, 2084

Notes

  1. ↑ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved October 6, 2018.
  2. ↑ Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site.
  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.

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References

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