Solar eclipse of April 20, 2042

Last updated
Solar eclipse of April 20, 2042
SE2042Apr20T.png
Map
Type of eclipse
NatureTotal
Gamma 0.2956
Magnitude 1.0614
Maximum eclipse
Duration291 s (4 min 51 s)
Coordinates 27°00′N137°18′E / 27°N 137.3°E / 27; 137.3
Max. width of band210 km (130 mi)
Times (UTC)
Greatest eclipse2:17:30
References
Saros 139 (31 of 71)
Catalog # (SE5000) 9601

A total solar eclipse will occur on Sunday, April 20, 2042. 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. It will be seen significantly in Western Indonesia (particularly in Sumatra), Eastern Malaysia, Brunei and the Philippines.

Contents

Images

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Animated path

Solar eclipses of 20402043

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
SE2041Apr30T.png
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 139

This eclipse is a member of saros series 139, repeating every 18 years, 11 days, 8 hours, containing 71 events. The series started with partial solar eclipse on May 17, 1501. It contains hybrid eclipses on August 11, 1627, through to December 9, 1825; and total eclipses from December 21, 1843, through to March 26, 2601. The series ends at member 71 as a partial eclipse on July 3, 2763. 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 solar eclipse of June 13, 2132, will be the longest total solar eclipse since July 11, 1991, at 6 minutes, 55.02 seconds.

The longest duration of totality will be produced by member 39 at 7 minutes, 29.22 seconds on July 16, 2186. [2] After that date, the durations of totality will decrease until the series ends. This date is the longest solar eclipse computed between 4000 BC and AD 6000. [3] Saros series eclipses occur during the Moon's ascending node (a term related to our equator and polar-naming conventions).

Series members 24–45 occur between 1901 and 2300
242526
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February 3, 1916
SE1934Feb14T.png
February 14, 1934
SE1952Feb25T.png
February 25, 1952
272829
SE1970Mar07T.png
March 7, 1970
SE1988Mar18T.png
March 18, 1988
SE2006Mar29T.png
March 29, 2006
303132
SE2024Apr08T.png
April 8, 2024
SE2042Apr20T.png
April 20, 2042
SE2060Apr30T.png
April 30, 2060
333435
SE2078May11T.png
May 11, 2078
SE2096May22T.png
May 22, 2096
SE2114Jun03T.png
June 3, 2114
363738
SE2132Jun13T.png
June 13, 2132
SE2150Jun25T.png
June 25, 2150
SE2168Jul05T.png
July 5, 2168
394041
SE2186Jul16T.png
July 16, 2186
SE2204Jul27T.png
July 27, 2204
SE2222Aug08T.png
August 8, 2222
424344
SE2240Aug18T.png
August 18, 2240
SE2258Aug29T.png
August 29, 2258
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September 9, 2276
45
SE2294Sep20T.png
September 20, 2294

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.

21 eclipse events, progressing from south to north between July 1, 2000 and July 1, 2076
July 1–2April 19–20February 5–7November 24–25September 12–13
117119121123125
SE2000Jul01P.png
July 1, 2000
SE2004Apr19P.png
April 19, 2004
SE2008Feb07A.png
February 7, 2008
SE2011Nov25P.png
November 25, 2011
SE2015Sep13P.png
September 13, 2015
127129131133135
SE2019Jul02T.png
July 2, 2019
SE2023Apr20H.png
April 20, 2023
SE2027Feb06A.png
February 6, 2027
SE2030Nov25T.png
November 25, 2030
SE2034Sep12A.png
September 12, 2034
137139141143145
SE2038Jul02A.png
July 2, 2038
SE2042Apr20T.png
April 20, 2042
SE2046Feb05A.png
February 5, 2046
SE2049Nov25H.png
November 25, 2049
SE2053Sep12T.png
September 12, 2053
147149151153155
SE2057Jul01A.png
July 1, 2057
SE2061Apr20T.png
April 20, 2061
SE2065Feb05P.png
February 5, 2065
SE2068Nov24P.png
November 24, 2068
SE2072Sep12T.png
September 12, 2072
157159161163165
SE2076Jul01P.png
July 1, 2076

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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. Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site.
  3. Ten Millennium Catalog of Long Solar Eclipses, −3999 to +6000 (4000 BCE to 6000 CE) Fred Espenak.