Solar eclipse of July 13, 2037

Last updated
Solar eclipse of July 13, 2037
SE2037Jul13T.png
Map
Type of eclipse
NatureTotal
Gamma −0.7246
Magnitude 1.0413
Maximum eclipse
Duration238 s (3 min 58 s)
Coordinates 24°48′S139°06′E / 24.8°S 139.1°E / -24.8; 139.1
Max. width of band201 km (125 mi)
Times (UTC)
Greatest eclipse2:40:36
References
Saros 127 (59 of 82)
Catalog # (SE5000) 9591

A total solar eclipse will occur at the Moon's ascending node of orbit on Monday, July 13, 2037, [1] with a magnitude of 1.0413. 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 2.6 days before perigee (on July 15, 2037, at 17:50 UTC), the Moon's apparent diameter will be larger. [2]

Contents

Totality will be visible from parts of Australia (including the center of Brisbane and the Gold Coast, as well as Geraldton, Western Australia) and New Zealand. A partial eclipse will be visible for parts of Indonesia, Australia, and Oceania.

Images

SE2037Jul13T.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]

July 13, 2037 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2037 July 13 at 00:16:24.2 UTC
First Umbral External Contact2037 July 13 at 01:26:24.0 UTC
First Central Line2037 July 13 at 01:27:34.1 UTC
First Umbral Internal Contact2037 July 13 at 01:28:44.8 UTC
Ecliptic Conjunction2037 July 13 at 02:33:00.2 UTC
Greatest Eclipse2037 July 13 at 02:40:35.9 UTC
Greatest Duration2037 July 13 at 02:41:03.4 UTC
Equatorial Conjunction2037 July 13 at 02:44:56.2 UTC
Last Umbral Internal Contact2037 July 13 at 03:52:21.3 UTC
Last Central Line2037 July 13 at 03:53:34.4 UTC
Last Umbral External Contact2037 July 13 at 03:54:46.8 UTC
Last Penumbral External Contact2037 July 13 at 05:04:40.9 UTC
July 13, 2037 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude1.04131
Eclipse Obscuration1.08433
Gamma−0.72458
Sun Right Ascension07h31m06.7s
Sun Declination+21°46'57.5"
Sun Semi-Diameter15'44.0"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension07h30m56.4s
Moon Declination+21°04'03.1"
Moon Semi-Diameter16'12.0"
Moon Equatorial Horizontal Parallax0°59'27.3"
ΔT77.3 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 July 2037
July 13
Ascending node (new moon)
 July 27
Descending node (full moon)
SE2037Jul13T.png Lunar eclipse chart close-2037Jul27.png
Total solar eclipse
Solar Saros 127		 Partial lunar eclipse
Lunar Saros 139

Eclipses in 2037

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 127

Inex

Triad

Solar eclipses of 2036–2039

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]

The partial solar eclipses on February 27, 2036 and August 21, 2036 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 2036 to 2039
Ascending node Descending node
SarosMapGammaSarosMapGamma
117 July 23, 2036
SE2036Jul23P.png
Partial		−1.425122 January 16, 2037
SE2037Jan16P.png
Partial		1.1477
127 July 13, 2037
SE2037Jul13T.png
Total		−0.7246132 January 5, 2038
SE2038Jan05A.png
Annular		0.4169
137 July 2, 2038
SE2038Jul02A.png
Annular		0.0398142 December 26, 2038
SE2038Dec26T.png
Total		−0.2881
147 June 21, 2039
SE2039Jun21A.png
Annular		0.8312152 December 15, 2039
SE2039Dec15T.png
Total		−0.9458

Saros 127

This eclipse is a part of Saros series 127, repeating every 18 years, 11 days, and containing 82 events. The series started with a partial solar eclipse on October 10, 991 AD. It contains total eclipses from May 14, 1352 through August 15, 2091. There are no annular or hybrid eclipses in this set. The series ends at member 82 as a partial eclipse on March 21, 2452. 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 was produced by member 31 at 5 minutes, 40 seconds on August 30, 1532. All eclipses in this series occur at the Moon’s ascending node of orbit. [5]

Series members 46–68 occur between 1801 and 2200:
464748
SE1803Feb21T.png
February 21, 1803		 SE1821Mar04T.gif
March 4, 1821		 SE1839Mar15T.gif
March 15, 1839
495051
SE1857Mar25T.gif
March 25, 1857 		SE1875Apr06T.png
April 6, 1875 		SE1893Apr16T.png
April 16, 1893
525354
SE1911Apr28T.png
April 28, 1911 		SE1929May09T.png
May 9, 1929 		SE1947May20T.png
May 20, 1947
555657
SE1965May30T.png
May 30, 1965 		SE1983Jun11T.png
June 11, 1983 		SE2001Jun21T.png
June 21, 2001
585960
SE2019Jul02T.png
July 2, 2019 		SE2037Jul13T.png
July 13, 2037 		SE2055Jul24T.png
July 24, 2055
616263
SE2073Aug03T.png
August 3, 2073 		SE2091Aug15T.png
August 15, 2091 		Saros127 63van82 SE2109Aug26P.jpg
August 26, 2109
646566
Saros127 64van82 SE2127Sep06P.jpg
September 6, 2127		 Saros127 65van82 SE2145Sep16P.jpg
September 16, 2145		 Saros127 66van82 SE2163Sep28P.jpg
September 28, 2163
6768
Saros127 67van82 SE2181Oct08P.jpg
October 8, 2181		 Saros127 68van82 SE2199Oct19P.jpg
October 19, 2199

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 13, 2018 and July 12, 2094
July 12–13April 30–May 1February 16–17December 5–6September 22–23
117119121123125
SE2018Jul13P.png
July 13, 2018 		SE2022Apr30P.png
April 30, 2022 		SE2026Feb17A.png
February 17, 2026 		SE2029Dec05P.png
December 5, 2029 		SE2033Sep23P.png
September 23, 2033
127129131133135
SE2037Jul13T.png
July 13, 2037 		SE2041Apr30T.png
April 30, 2041 		SE2045Feb16A.png
February 16, 2045 		SE2048Dec05T.png
December 5, 2048 		SE2052Sep22A.png
September 22, 2052
137139141143145
SE2056Jul12A.png
July 12, 2056 		SE2060Apr30T.png
April 30, 2060 		SE2064Feb17A.png
February 17, 2064 		SE2067Dec06H.png
December 6, 2067 		SE2071Sep23T.png
September 23, 2071
147149151153155
SE2075Jul13A.png
July 13, 2075 		SE2079May01T.png
May 1, 2079 		SE2083Feb16P.png
February 16, 2083 		SE2086Dec06P.png
December 6, 2086 		SE2090Sep23T.png
September 23, 2090
157
SE2094Jul12P.png
July 12, 2094

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
SE1819Mar25P.gif
March 25, 1819
(Saros 107)		 SE1830Feb23P.gif
February 23, 1830
(Saros 108)		 SE1841Jan22P.gif
January 22, 1841
(Saros 109)		 SE1862Nov21P.gif
November 21, 1862
(Saros 111)
SE1895Aug20P.gif
August 20, 1895
(Saros 114)		 SE1906Jul21P.png
July 21, 1906
(Saros 115)		 SE1917Jun19P.png
June 19, 1917
(Saros 116)
SE1928May19T.png
May 19, 1928
(Saros 117)		 SE1939Apr19A.png
April 19, 1939
(Saros 118)		 SE1950Mar18A.png
March 18, 1950
(Saros 119)		 SE1961Feb15T.png
February 15, 1961
(Saros 120)		 SE1972Jan16A.png
January 16, 1972
(Saros 121)
SE1982Dec15P.png
December 15, 1982
(Saros 122)		 SE1993Nov13P.png
November 13, 1993
(Saros 123)		 SE2004Oct14P.png
October 14, 2004
(Saros 124)		 SE2015Sep13P.png
September 13, 2015
(Saros 125)		 SE2026Aug12T.png
August 12, 2026
(Saros 126)
SE2037Jul13T.png
July 13, 2037
(Saros 127)		 SE2048Jun11A.png
June 11, 2048
(Saros 128)		 SE2059May11T.png
May 11, 2059
(Saros 129)		 SE2070Apr11T.png
April 11, 2070
(Saros 130)		 SE2081Mar10A.png
March 10, 2081
(Saros 131)
SE2092Feb07A.png
February 7, 2092
(Saros 132)		 SE2103Jan08T.png
January 8, 2103
(Saros 133)		 SE2113Dec08A.png
December 8, 2113
(Saros 134)		 SE2124Nov06A.png
November 6, 2124
(Saros 135)		 SE2135Oct07T.png
October 7, 2135
(Saros 136)
SE2146Sep06A.png
September 6, 2146
(Saros 137)		 SE2157Aug05A.png
August 5, 2157
(Saros 138)		 SE2168Jul05T.png
July 5, 2168
(Saros 139)		 SE2179Jun05A.png
June 5, 2179
(Saros 140)		 SE2190May04A.png
May 4, 2190
(Saros 141)

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
SE1805Dec21A.gif
December 21, 1805
(Saros 119)		 SE1834Nov30T.gif
November 30, 1834
(Saros 120)		 SE1863Nov11A.png
November 11, 1863
(Saros 121)
SE1892Oct20P.gif
October 20, 1892
(Saros 122)		 SE1921Oct01T.png
October 1, 1921
(Saros 123)		 SE1950Sep12T.png
September 12, 1950
(Saros 124)
SE1979Aug22A.png
August 22, 1979
(Saros 125)		 SE2008Aug01T.png
August 1, 2008
(Saros 126)		 SE2037Jul13T.png
July 13, 2037
(Saros 127)
SE2066Jun22A.png
June 22, 2066
(Saros 128)		 SE2095Jun02T.png
June 2, 2095
(Saros 129)		 SE2124May14T.png
May 14, 2124
(Saros 130)
SE2153Apr23A.png
April 23, 2153
(Saros 131)		 SE2182Apr03H.png
April 3, 2182
(Saros 132)

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References

  1. ↑ "July 13, 2037 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 2037 Jul 13". 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. ↑ "NASA - Catalog of Solar Eclipses of Saros 127". eclipse.gsfc.nasa.gov.
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