Solar eclipse of February 16, 2083

Last updated
Solar eclipse of February 16, 2083
SE2083Feb16P.png
Map
Type of eclipse
NaturePartial
Gamma 1.017
Magnitude 0.9433
Maximum eclipse
Coordinates 61°36′N154°06′W / 61.6°N 154.1°W / 61.6; -154.1
Times (UTC)
Greatest eclipse18:06:36
References
Saros 151 (18 of 72)
Catalog # (SE5000) 9693

A partial solar eclipse will occur at the Moon's ascending node of orbit on Tuesday, February 16, 2083, with a magnitude of 0.9433. 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

Eclipses in 2083

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 151

Inex

Triad

Solar eclipses of 2080–2083

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 eclipse on July 15, 2083 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 2080 to 2083
Ascending node Descending node
SarosMapGammaSarosMapGamma
121 March 21, 2080
SE2080Mar21P.png
Partial
−1.0578126 September 13, 2080
SE2080Sep13P.png
Partial
1.0723
131 March 10, 2081
SE2081Mar10A.png
Annular
−0.3653136 September 3, 2081
SE2081Sep03T.png
Total
0.3378
141 February 27, 2082
SE2082Feb27A.png
Annular
0.3361146 August 24, 2082
SE2082Aug24T.png
Total
−0.4004
151 February 16, 2083
SE2083Feb16P.png
Partial
1.017156 August 13, 2083
SE2083Aug13P.png
Partial
−1.2064

Saros 151

This eclipse is a part of Saros series 151, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on August 14, 1776. It contains annular eclipses from February 28, 2101 through April 23, 2191; a hybrid eclipse on May 5, 2209; and total eclipses from May 16, 2227 through July 6, 2912. The series ends at member 72 as a partial eclipse on October 1, 3056. 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 will be produced by member 19 at 2 minutes, 44 seconds on February 28, 2101, and the longest duration of totality will be produced by member 60 at 5 minutes, 41 seconds on May 22, 2840. All eclipses in this series occur at the Moon’s ascending node of orbit. [2]

Series members 3–24 occur between 1801 and 2200:
345
SE1812Sep05P.gif
September 5, 1812
SE1830Sep17P.gif
September 17, 1830
SE1848Sep27P.gif
September 27, 1848
678
SE1866Oct08P.gif
October 8, 1866
SE1884Oct19P.gif
October 19, 1884
SE1902Oct31P.png
October 31, 1902
91011
SE1920Nov10P.png
November 10, 1920
SE1938Nov21P.png
November 21, 1938
SE1956Dec02P.png
December 2, 1956
121314
SE1974Dec13P.png
December 13, 1974
SE1992Dec24P.png
December 24, 1992
SE2011Jan04P.png
January 4, 2011
151617
SE2029Jan14P.png
January 14, 2029
SE2047Jan26P.png
January 26, 2047
SE2065Feb05P.png
February 5, 2065
181920
SE2083Feb16P.png
February 16, 2083
SE2101Feb28A.png
February 28, 2101
Saros151 20van72 SE2119Mar11A.jpg
March 11, 2119
212223
Saros151 21van72 SE2137Mar21A.jpg
March 21, 2137
SE2155Apr02A.png
April 2, 2155
Saros151 23van72 SE2173Apr12A.jpg
April 12, 2173
24
SE2191Apr23A.png
April 23, 2191

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
SE1810Apr04A.gif
April 4, 1810
(Saros 126)
SE1821Mar04T.gif
March 4, 1821
(Saros 127)
SE1832Feb01A.gif
February 1, 1832
(Saros 128)
SE1842Dec31A.gif
December 31, 1842
(Saros 129)
SE1853Nov30T.png
November 30, 1853
(Saros 130)
SE1864Oct30A.gif
October 30, 1864
(Saros 131)
SE1875Sep29A.gif
September 29, 1875
(Saros 132)
SE1886Aug29T.png
August 29, 1886
(Saros 133)
SE1897Jul29A.gif
July 29, 1897
(Saros 134)
SE1908Jun28A.png
June 28, 1908
(Saros 135)
SE1919May29T.png
May 29, 1919
(Saros 136)
SE1930Apr28H.png
April 28, 1930
(Saros 137)
SE1941Mar27A.png
March 27, 1941
(Saros 138)
SE1952Feb25T.png
February 25, 1952
(Saros 139)
SE1963Jan25A.png
January 25, 1963
(Saros 140)
SE1973Dec24A.png
December 24, 1973
(Saros 141)
SE1984Nov22T.png
November 22, 1984
(Saros 142)
SE1995Oct24T.png
October 24, 1995
(Saros 143)
SE2006Sep22A.png
September 22, 2006
(Saros 144)
SE2017Aug21T.png
August 21, 2017
(Saros 145)
SE2028Jul22T.png
July 22, 2028
(Saros 146)
SE2039Jun21A.png
June 21, 2039
(Saros 147)
SE2050May20H.png
May 20, 2050
(Saros 148)
SE2061Apr20T.png
April 20, 2061
(Saros 149)
SE2072Mar19P.png
March 19, 2072
(Saros 150)
SE2083Feb16P.png
February 16, 2083
(Saros 151)
SE2094Jan16T.png
January 16, 2094
(Saros 152)
Saros153 14van70 SE2104Dec17A.jpg
December 17, 2104
(Saros 153)
SE2115Nov16A.png
November 16, 2115
(Saros 154)
SE2126Oct16T.png
October 16, 2126
(Saros 155)
Saros156 08van69 SE2137Sep15P.jpg
September 15, 2137
(Saros 156)
Saros157 06van70 SE2148Aug14P.jpg
August 14, 2148
(Saros 157)
Saros158 06van70 SE2159Jul15P.jpg
July 15, 2159
(Saros 158)
Saros159 03van70 SE2170Jun14P.jpg
June 14, 2170
(Saros 159)
Saros160 01van71 SE2181May13P.jpg
May 13, 2181
(Saros 160)
Saros161 02van72 SE2192Apr12P.jpg
April 12, 2192
(Saros 161)

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

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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 151". eclipse.gsfc.nasa.gov.