Solar eclipse of January 16, 2056

Last updated
Solar eclipse of January 16, 2056
SE2056Jan16A.png
Map
Type of eclipse
NatureAnnular
Gamma 0.4199
Magnitude 0.9759
Maximum eclipse
Duration172 s (2 min 52 s)
Coordinates 3°54′N153°30′W / 3.9°N 153.5°W / 3.9; -153.5
Max. width of band95 km (59 mi)
Times (UTC)
Greatest eclipse22:16:45
References
Saros 132 (48 of 71)
Catalog # (SE5000) 9632

An annular solar eclipse will occur at the Moon's descending node of orbit on Sunday, January 16, 2056, with a magnitude of 0.9759. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

Contents

Eclipses in 2056

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 132

Inex

Triad

Solar eclipses of 2054–2058

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]

The partial solar eclipses on March 9, 2054 and September 2, 2054 occur in the previous lunar year eclipse set, and the partial solar eclipses on May 22, 2058 and November 16, 2058 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2054 to 2058
Ascending node Descending node
SarosMapGammaSarosMapGamma
117 August 3, 2054
SE2054Aug03P.png
Partial
−1.4941122 January 27, 2055
SE2055Jan27P.png
Partial
1.155
127 July 24, 2055
SE2055Jul24T.png
Total
−0.8012132 January 16, 2056
SE2056Jan16A.png
Annular
0.4199
137 July 12, 2056
SE2056Jul12A.png
Annular
−0.0426142 January 5, 2057
SE2057Jan05T.png
Total
−0.2837
147 July 1, 2057
SE2057Jul01A.png
Annular
0.7455152 December 26, 2057
SE2057Dec26T.png
Total
−0.9405
157 June 21, 2058
SE2058Jun21P.png
Partial
1.4869

Saros 132

This eclipse is a part of Saros series 132, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on August 13, 1208. It contains annular eclipses from March 17, 1569 through March 12, 2146; hybrid eclipses on March 23, 2164 and April 3, 2182; and total eclipses from April 14, 2200 through June 19, 2308. The series ends at member 71 as a partial eclipse on September 25, 2470. 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 annularity was produced by member 25 at 6 minutes, 56 seconds on May 9, 1641, and the longest duration of totality will be produced by member 61 at 2 minutes, 14 seconds on June 8, 2290. All eclipses in this series occur at the Moon’s descending node of orbit. [2]

Series members 34–56 occur between 1801 and 2200:
343536
SE1803Aug17A.png
August 17, 1803
SE1821Aug27A.png
August 27, 1821
SE1839Sep07A.png
September 7, 1839
373839
SE1857Sep18A.png
September 18, 1857
SE1875Sep29A.png
September 29, 1875
SE1893Oct09A.png
October 9, 1893
404142
SE1911Oct22A.png
October 22, 1911
SE1929Nov01A.png
November 1, 1929
SE1947Nov12A.png
November 12, 1947
434445
SE1965Nov23A.png
November 23, 1965
SE1983Dec04A.png
December 4, 1983
SE2001Dec14A.png
December 14, 2001
464748
SE2019Dec26A.png
December 26, 2019
SE2038Jan05A.png
January 5, 2038
SE2056Jan16A.png
January 16, 2056
495051
SE2074Jan27A.png
January 27, 2074
SE2092Feb07A.png
February 7, 2092
SE2110Feb18A.png
February 18, 2110
525354
SE2128Mar01A.png
March 1, 2128
SE2146Mar12A.png
March 12, 2146
SE2164Mar23H.png
March 23, 2164
5556
SE2182Apr03H.png
April 3, 2182
SE2200Apr14T.png
April 14, 2200

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.

Series members between 1801 and 2200
SE1805Jan01P.gif
January 1, 1805
(Saros 109)
SE1826Oct31P.gif
October 31, 1826
(Saros 111)
SE1848Aug28P.gif
August 28, 1848
(Saros 113)
SE1859Jul29P.gif
July 29, 1859
(Saros 114)
SE1870Jun28P.gif
June 28, 1870
(Saros 115)
SE1881May27P.gif
May 27, 1881
(Saros 116)
SE1892Apr26T.png
April 26, 1892
(Saros 117)
SE1903Mar29A.png
March 29, 1903
(Saros 118)
SE1914Feb25A.png
February 25, 1914
(Saros 119)
SE1925Jan24T.png
January 24, 1925
(Saros 120)
SE1935Dec25A.png
December 25, 1935
(Saros 121)
SE1946Nov23P.png
November 23, 1946
(Saros 122)
SE1957Oct23T.png
October 23, 1957
(Saros 123)
SE1968Sep22T.png
September 22, 1968
(Saros 124)
SE1979Aug22A.png
August 22, 1979
(Saros 125)
SE1990Jul22T.png
July 22, 1990
(Saros 126)
SE2001Jun21T.png
June 21, 2001
(Saros 127)
SE2012May20A.png
May 20, 2012
(Saros 128)
SE2023Apr20H.png
April 20, 2023
(Saros 129)
SE2034Mar20T.png
March 20, 2034
(Saros 130)
SE2045Feb16A.png
February 16, 2045
(Saros 131)
SE2056Jan16A.png
January 16, 2056
(Saros 132)
SE2066Dec17T.png
December 17, 2066
(Saros 133)
SE2077Nov15A.png
November 15, 2077
(Saros 134)
SE2088Oct14A.png
October 14, 2088
(Saros 135)
SE2099Sep14T.png
September 14, 2099
(Saros 136)
SE2110Aug15A.png
August 15, 2110
(Saros 137)
SE2121Jul14A.png
July 14, 2121
(Saros 138)
SE2132Jun13T.png
June 13, 2132
(Saros 139)
SE2143May14A.png
May 14, 2143
(Saros 140)
SE2154Apr12A.png
April 12, 2154
(Saros 141)
SE2165Mar12T.png
March 12, 2165
(Saros 142)
SE2176Feb10A.png
February 10, 2176
(Saros 143)
SE2187Jan09A.png
January 9, 2187
(Saros 144)
SE2197Dec09T.png
December 9, 2197
(Saros 145)

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
SE1824Jun26T.png
June 26, 1824
(Saros 124)
SE1853Jun06A.gif
June 6, 1853
(Saros 125)
SE1882May17T.png
May 17, 1882
(Saros 126)
SE1911Apr28T.png
April 28, 1911
(Saros 127)
SE1940Apr07A.png
April 7, 1940
(Saros 128)
SE1969Mar18A.png
March 18, 1969
(Saros 129)
SE1998Feb26T.png
February 26, 1998
(Saros 130)
SE2027Feb06A.png
February 6, 2027
(Saros 131)
SE2056Jan16A.png
January 16, 2056
(Saros 132)
SE2084Dec27T.png
December 27, 2084
(Saros 133)
SE2113Dec08A.png
December 8, 2113
(Saros 134)
SE2142Nov17A.png
November 17, 2142
(Saros 135)
SE2171Oct29T.png
October 29, 2171
(Saros 136)
SE2200Oct09A.png
October 9, 2200
(Saros 137)

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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. "NASA - Catalog of Solar Eclipses of Saros 132". eclipse.gsfc.nasa.gov.