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 at the Moon's ascending node of orbit between Saturday, April 19 and Sunday, April 20, 2042, [1] with a magnitude of 1.0614. 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. Occurring about 21 hours after perigee (on April 19, 2042, at 5:25 UTC), the Moon's apparent diameter will be larger. [2]

Contents

The path of totality will be visible from parts of western Indonesia (particularly Sumatra), eastern Malaysia, Brunei and the Philippines. A partial solar eclipse will be visible for parts of South Asia, Southeast Asia, northern Australia, East Asia, Northeast Asia, Hawaii, and northwestern North America.

Images

SE2042Apr20T.gif
Animated path

Eclipse details

Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse. [3]

April 20, 2042 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2042 April 19 at 23:41:45.0 UTC
First Umbral External Contact2042 April 20 at 00:37:26.5 UTC
First Central Line2042 April 20 at 00:38:41.2 UTC
First Umbral Internal Contact2042 April 20 at 00:39:55.9 UTC
First Penumbral Internal Contact2042 April 20 at 01:40:21.0 UTC
Greatest Eclipse2042 April 20 at 02:17:30.1 UTC
Ecliptic Conjunction2042 April 20 at 02:20:31.9 UTC
Greatest Duration2042 April 20 at 02:21:20.1 UTC
Equatorial Conjunction2042 April 20 at 02:32:33.0 UTC
Last Penumbral Internal Contact2042 April 20 at 02:54:18.5 UTC
Last Umbral Internal Contact2042 April 20 at 03:54:56.1 UTC
Last Central Line2042 April 20 at 03:56:09.9 UTC
Last Umbral External Contact2042 April 20 at 03:57:23.7 UTC
Last Penumbral External Contact2042 April 20 at 04:53:11.4 UTC
April 20, 2042 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude1.06144
Eclipse Obscuration1.12666
Gamma0.29559
Sun Right Ascension01h52m12.4s
Sun Declination+11°31'19.4"
Sun Semi-Diameter15'55.3"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension01h51m39.9s
Moon Declination+11°47'27.9"
Moon Semi-Diameter16'37.6"
Moon Equatorial Horizontal Parallax1°01'01.4"
ΔT79.8 s

Eclipse season

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.

Eclipse season of April 2042
April 5
Descending node (full moon)
April 20
Ascending node (new moon)
Lunar eclipse chart close-2042Apr05.png SE2042Apr20T.png
Penumbral lunar eclipse
Lunar Saros 113
Total solar eclipse
Solar Saros 139

Eclipses in 2042

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 139

Inex

Triad

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. [4]

Solar eclipse series sets from 2040 to 2043
Ascending node Descending node
SarosMapGammaSarosMapGamma
119 May 11, 2040
SE2040May11P.png
Partial
−1.2529124 November 4, 2040
SE2040Nov04P.png
Partial
1.0993
129 April 30, 2041
SE2041Apr30T.png
Total
−0.4492134 October 25, 2041
SE2041Oct25A.png
Annular
0.4133
139 April 20, 2042
SE2042Apr20T.png
Total
0.2956144 October 14, 2042
SE2042Oct14A.png
Annular
−0.303
149 April 9, 2043
SE2043Apr09T.png
Total (non-central)
1.0031154 October 3, 2043
SE2043Oct03A.png
Annular (non-central)
1.0102

Saros 139

This eclipse is a part of Saros series 139, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on May 17, 1501. It contains hybrid eclipses from August 11, 1627 through December 9, 1825 and total eclipses from December 21, 1843 through March 26, 2601. There are no annular eclipses in this set. 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 longest duration of totality will be produced by member 61 at 7 minutes, 29.22 seconds on July 16, 2186. This date is the longest solar eclipse computed between 4000 BC and AD 6000. [5] All eclipses in this series occur at the Moon’s ascending node of orbit. [6]

Series members 18–39 occur between 1801 and 2200:
181920
SE1807Nov29H.png
November 29, 1807
SE1825Dec09H.png
December 9, 1825
SE1843Dec21T.png
December 21, 1843
212223
SE1861Dec31T.png
December 31, 1861
SE1880Jan11T.png
January 11, 1880
SE1898Jan22T.png
January 22, 1898
242526
SE1916Feb03T.png
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
39
SE2186Jul16T.png
July 16, 2186

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 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
157
SE2076Jul01P.png
July 1, 2076

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200
SE1802Mar04T.png
March 4, 1802
(Saros 117)
SE1813Feb01A.gif
February 1, 1813
(Saros 118)
SE1824Jan01A.gif
January 1, 1824
(Saros 119)
SE1834Nov30T.gif
November 30, 1834
(Saros 120)
SE1845Oct30H.png
October 30, 1845
(Saros 121)
SE1856Sep29A.gif
September 29, 1856
(Saros 122)
SE1867Aug29T.png
August 29, 1867
(Saros 123)
SE1878Jul29T.png
July 29, 1878
(Saros 124)
SE1889Jun28A.png
June 28, 1889
(Saros 125)
SE1900May28T.png
May 28, 1900
(Saros 126)
SE1911Apr28T.png
April 28, 1911
(Saros 127)
SE1922Mar28A.png
March 28, 1922
(Saros 128)
SE1933Feb24A.png
February 24, 1933
(Saros 129)
SE1944Jan25T.png
January 25, 1944
(Saros 130)
SE1954Dec25A.png
December 25, 1954
(Saros 131)
SE1965Nov23A.png
November 23, 1965
(Saros 132)
SE1976Oct23T.png
October 23, 1976
(Saros 133)
SE1987Sep23A.png
September 23, 1987
(Saros 134)
SE1998Aug22A.png
August 22, 1998
(Saros 135)
SE2009Jul22T.png
July 22, 2009
(Saros 136)
SE2020Jun21A.png
June 21, 2020
(Saros 137)
SE2031May21A.png
May 21, 2031
(Saros 138)
SE2042Apr20T.png
April 20, 2042
(Saros 139)
SE2053Mar20A.png
March 20, 2053
(Saros 140)
SE2064Feb17A.png
February 17, 2064
(Saros 141)
SE2075Jan16T.png
January 16, 2075
(Saros 142)
SE2085Dec16A.png
December 16, 2085
(Saros 143)
SE2096Nov15A.png
November 15, 2096
(Saros 144)
SE2107Oct16T.png
October 16, 2107
(Saros 145)
SE2118Sep15T.png
September 15, 2118
(Saros 146)
SE2129Aug15A.png
August 15, 2129
(Saros 147)
Saros148 28van75 SE2140Jul14T.jpg
July 14, 2140
(Saros 148)
Saros149 28van71 SE2151Jun14T.jpg
June 14, 2151
(Saros 149)
Saros150 25van71 SE2162May14A.jpg
May 14, 2162
(Saros 150)
Saros151 23van72 SE2173Apr12A.jpg
April 12, 2173
(Saros 151)
Saros152 22van70 SE2184Mar12T.jpg
March 12, 2184
(Saros 152)
Saros153 19van70 SE2195Feb10A.jpg
February 10, 2195
(Saros 153)

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.

Series members between 1801 and 2200
SE1810Sep28A.gif
September 28, 1810
(Saros 131)
SE1839Sep07A.png
September 7, 1839
(Saros 132)
SE1868Aug18T.png
August 18, 1868
(Saros 133)
SE1897Jul29A.gif
July 29, 1897
(Saros 134)
SE1926Jul09A.png
July 9, 1926
(Saros 135)
SE1955Jun20T.png
June 20, 1955
(Saros 136)
SE1984May30A.png
May 30, 1984
(Saros 137)
SE2013May10A.png
May 10, 2013
(Saros 138)
SE2042Apr20T.png
April 20, 2042
(Saros 139)
SE2071Mar31A.png
March 31, 2071
(Saros 140)
SE2100Mar10A.png
March 10, 2100
(Saros 141)
SE2129Feb18T.png
February 18, 2129
(Saros 142)
SE2158Jan30A.png
January 30, 2158
(Saros 143)
SE2187Jan09A.png
January 9, 2187
(Saros 144)

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References

  1. "April 19–20, 2042 Total Solar Eclipse". timeanddate. Retrieved 14 August 2024.
  2. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 14 August 2024.
  3. "Total Solar Eclipse of 2042 Apr 20". EclipseWise.com. Retrieved 14 August 2024.
  4. 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.
  5. Ten Millennium Catalog of Long Solar Eclipses, −3999 to +6000 (4000 BCE to 6000 CE) Fred Espenak.
  6. "NASA - Catalog of Solar Eclipses of Saros 139". eclipse.gsfc.nasa.gov.