Solar eclipse of April 30, 2041

Last updated
Solar eclipse of April 30, 2041
SE2041Apr30T.png
Map
Type of eclipse
NatureTotal
Gamma −0.4492
Magnitude 1.0189
Maximum eclipse
Duration111 s (1 min 51 s)
Coordinates 9°36′S12°12′E / 9.6°S 12.2°E / -9.6; 12.2
Max. width of band72 km (45 mi)
Times (UTC)
Greatest eclipse11:52:21
References
Saros 129 (53 of 80)
Catalog # (SE5000) 9599

A total solar eclipse will occur on Tuesday, April 30, 2041. 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.

Contents

Images

SE2041Apr30T.gif
Animated path

Solar eclipses of 2040–2043

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 2040 to 2043
Ascending node Descending node
119 May 11, 2040
SE2040May11P.png
Partial
124 November 4, 2040
SE2040Nov04P.png
Annular
129 April 30, 2041
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Total
134 October 25, 2041
SE2041Oct25A.png
Annular
139 April 20, 2042
SE2042Apr20T.png
Total
144 October 14, 2042
SE2042Oct14A.png
Annular
149 April 9, 2043
SE2043Apr09T.png
Total (non-central)
154 October 3, 2043
SE2043Oct03A.png
Annular (non-central)

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:
464748
SE1915Feb14A.png
February 14, 1915
SE1933Feb24A.png
February 24, 1933
SE1951Mar07A.png
March 7, 1951
495051
SE1969Mar18A.png
March 18, 1969
SE1987Mar29H.png
March 29, 1987
SE2005Apr08H.png
April 8, 2005
525354
SE2023Apr20H.png
April 20, 2023
SE2041Apr30T.png
April 30, 2041
SE2059May11T.png
May 11, 2059
5556
SE2077May22T.png
May 22, 2077
SE2095Jun02T.png
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.

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 ascending node.

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References

  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.