Solar eclipse of January 16, 2037

Last updated
Solar eclipse of January 16, 2037
SE2037Jan16P.png
Map
Type of eclipse
NaturePartial
Gamma 1.1477
Magnitude 0.7049
Maximum eclipse
Coordinates 68°30′N20°48′E / 68.5°N 20.8°E / 68.5; 20.8
Times (UTC)
Greatest eclipse9:48:55
References
Saros 122 (59 of 70)
Catalog # (SE5000) 9590

A partial solar eclipse will occur at the Moon's descending node of orbit on Friday, January 16, 2037, [1] with a magnitude of 0.7049. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

Contents

A partial eclipse will be visible for parts of Europe, North Africa, the Middle East, and Central Asia.

Images

SE2037Jan16P.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. [2]

January 16, 2037 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2037 January 16 at 07:42:39.8 UTC
Ecliptic Conjunction2037 January 16 at 09:35:36.0 UTC
Greatest Eclipse2037 January 16 at 09:48:55.1 UTC
Equatorial Conjunction2037 January 16 at 10:01:35.5 UTC
Last Penumbral External Contact2037 January 16 at 11:55:08.4 UTC
January 16, 2037 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.70493
Eclipse Obscuration0.60942
Gamma1.14772
Sun Right Ascension19h54m30.1s
Sun Declination-20°49'43.5"
Sun Semi-Diameter16'15.5"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension19h54m05.4s
Moon Declination-19°47'33.7"
Moon Semi-Diameter14'51.8"
Moon Equatorial Horizontal Parallax0°54'32.8"
ΔT77.1 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 January 2037
January 16
Descending node (new moon)
January 31
Ascending node (full moon)
SE2037Jan16P.png Lunar eclipse chart close-2037Jan31.png
Partial solar eclipse
Solar Saros 122
Total lunar eclipse
Lunar Saros 134

Eclipses in 2037

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 122

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. [3]

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 122

This eclipse is a part of Saros series 122, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on April 17, 991 AD. It contains total eclipses from July 12, 1135 through August 3, 1171; hybrid eclipses on August 13, 1189 and August 25, 1207; and annular eclipses from September 4, 1225 through October 10, 1874. The series ends at member 70 as a partial eclipse on May 17, 2235. 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 9 at 1 minutes, 25 seconds on July 12, 1135, and the longest duration of annularity was produced by member 50 at 6 minutes, 28 seconds on October 10, 1874. All eclipses in this series occur at the Moon’s descending node of orbit. [4]

Series members 46–68 occur between 1801 and 2200:
464748
SE1802Aug28A.png
August 28, 1802
SE1820Sep07A.gif
September 7, 1820
SE1838Sep18A.gif
September 18, 1838
495051
SE1856Sep29A.gif
September 29, 1856
SE1874Oct10An.gif
October 10, 1874
SE1892Oct20P.gif
October 20, 1892
525354
SE1910Nov02P.png
November 2, 1910
SE1928Nov12P.png
November 12, 1928
SE1946Nov23P.png
November 23, 1946
555657
SE1964Dec04P.png
December 4, 1964
SE1982Dec15P.png
December 15, 1982
SE2000Dec25P.png
December 25, 2000
585960
SE2019Jan06P.png
January 6, 2019
SE2037Jan16P.png
January 16, 2037
SE2055Jan27P.png
January 27, 2055
616263
SE2073Feb07P.png
February 7, 2073
SE2091Feb18P.png
February 18, 2091
Saros122 63van70 SE2109Mar01P.jpg
March 1, 2109
646566
Saros122 64van70 SE2127Mar13P.jpg
March 13, 2127
Saros122 65van70 SE2145Mar23P.jpg
March 23, 2145
Saros122 66van70 SE2163Apr03P.jpg
April 3, 2163
6768
Saros122 67van70 SE2181Apr14P.jpg
April 14, 2181
Saros122 68van70 SE2199Apr25P.jpg
April 25, 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 descending node.

22 eclipse events between June 12, 2029 and November 4, 2116
June 11–12March 30–31January 16November 4–5August 23–24
118120122124126
SE2029Jun12P.png
June 12, 2029
SE2033Mar30T.png
March 30, 2033
SE2037Jan16P.png
January 16, 2037
SE2040Nov04P.png
November 4, 2040
SE2044Aug23T.png
August 23, 2044
128130132134136
SE2048Jun11A.png
June 11, 2048
SE2052Mar30T.png
March 30, 2052
SE2056Jan16A.png
January 16, 2056
SE2059Nov05A.png
November 5, 2059
SE2063Aug24T.png
August 24, 2063
138140142144146
SE2067Jun11A.png
June 11, 2067
SE2071Mar31A.png
March 31, 2071
SE2075Jan16T.png
January 16, 2075
SE2078Nov04A.png
November 4, 2078
SE2082Aug24T.png
August 24, 2082
148150152154156
SE2086Jun11T.png
June 11, 2086
SE2090Mar31P.png
March 31, 2090
SE2094Jan16T.png
January 16, 2094
SE2097Nov04A.png
November 4, 2097
Saros156 06van69 SE2101Aug24P.jpg
August 24, 2101
158160162164
Saros158 03van70 SE2105Jun12P.jpg
June 12, 2105
Saros164 02van80 SE2116Nov04P.jpg
November 4, 2116

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.

The partial solar eclipses on March 27, 1884 (part of Saros 108) and December 24, 1916 (part of Saros 111) are also a part of this series but are not included in the table below.

Series members between 1971 and 2200
SE1971Jul22P.png
July 22, 1971
(Saros 116)
SE1982Jun21P.png
June 21, 1982
(Saros 117)
SE1993May21P.png
May 21, 1993
(Saros 118)
SE2004Apr19P.png
April 19, 2004
(Saros 119)
SE2015Mar20T.png
March 20, 2015
(Saros 120)
SE2026Feb17A.png
February 17, 2026
(Saros 121)
SE2037Jan16P.png
January 16, 2037
(Saros 122)
SE2047Dec16P.png
December 16, 2047
(Saros 123)
SE2058Nov16P.png
November 16, 2058
(Saros 124)
SE2069Oct15P.png
October 15, 2069
(Saros 125)
SE2080Sep13P.png
September 13, 2080
(Saros 126)
SE2091Aug15T.png
August 15, 2091
(Saros 127)
SE2102Jul15A.png
July 15, 2102
(Saros 128)
SE2113Jun13T.png
June 13, 2113
(Saros 129)
SE2124May14T.png
May 14, 2124
(Saros 130)
SE2135Apr13A.png
April 13, 2135
(Saros 131)
SE2146Mar12A.png
March 12, 2146
(Saros 132)
SE2157Feb09T.png
February 9, 2157
(Saros 133)
SE2168Jan10A.png
January 10, 2168
(Saros 134)
SE2178Dec09A.png
December 9, 2178
(Saros 135)
SE2189Nov08T.png
November 8, 2189
(Saros 136)
SE2200Oct09A.png
October 9, 2200
(Saros 137)

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
SE1805Jun26P.gif
June 26, 1805
(Saros 114)
SE1834Jun07P.gif
June 7, 1834
(Saros 115)
SE1863May17P.gif
May 17, 1863
(Saros 116)
SE1892Apr26T.png
April 26, 1892
(Saros 117)
SE1921Apr08A.png
April 8, 1921
(Saros 118)
SE1950Mar18A.png
March 18, 1950
(Saros 119)
SE1979Feb26T.png
February 26, 1979
(Saros 120)
SE2008Feb07A.png
February 7, 2008
(Saros 121)
SE2037Jan16P.png
January 16, 2037
(Saros 122)
SE2065Dec27P.png
December 27, 2065
(Saros 123)
SE2094Dec07P.png
December 7, 2094
(Saros 124)
Saros125 60van73 SE2123Nov18P.jpg
November 18, 2123
(Saros 125)
Saros126 55van72 SE2152Oct28P.jpg
October 28, 2152
(Saros 126)
Saros127 67van82 SE2181Oct08P.jpg
October 8, 2181
(Saros 127)

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References

  1. "January 16, 2037 Partial Solar Eclipse". timeanddate. Retrieved 14 August 2024.
  2. "Partial Solar Eclipse of 2037 Jan 16". EclipseWise.com. Retrieved 14 August 2024.
  3. 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.
  4. "NASA - Catalog of Solar Eclipses of Saros 122". eclipse.gsfc.nasa.gov.