Solar eclipse of March 11, 2062

Future partial solar eclipse From Wikipedia, the free encyclopedia

Solar eclipse of March 11, 2062

A partial solar eclipse will occur at the Moon's ascending node of orbit on Saturday, March 11, 2062,[1] with a magnitude of 0.9331. 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.

Quick Facts Gamma, Magnitude ...
Solar eclipse of March 11, 2062
Partial eclipse
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Map
Gamma−1.0238
Magnitude0.9331
Maximum eclipse
Coordinates61°S 147.1°W / -61; -147.1
Times (UTC)
Greatest eclipse4:26:16
References
Saros121 (63 of 71)
Catalog # (SE5000)9646
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The partial solar eclipse will be visible for much of Antarctica, Eastern Australia, New Zealand, and Oceania.

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]

More information Event, Time (UTC) ...
March 11, 2062 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 2062 March 11 at 02:14:37.0 UTC
Equatorial Conjunction 2062 March 11 at 03:22:56.6 UTC
Ecliptic Conjunction 2062 March 11 at 04:14:52.2 UTC
Greatest Eclipse 2062 March 11 at 04:26:16.2 UTC
Last Penumbral External Contact 2062 March 11 at 06:38:14.6 UTC
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More information Parameter, Value ...
March 11, 2062 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.93309
Eclipse Obscuration 0.89604
Gamma −1.02380
Sun Right Ascension 23h26m28.0s
Sun Declination -03°36'57.3"
Sun Semi-Diameter 16'06.2"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 23h28m20.0s
Moon Declination -04°27'39.9"
Moon Semi-Diameter 15'26.8"
Moon Equatorial Horizontal Parallax 0°56'41.5"
ΔT 91.9 s
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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.

More information March 11Ascending node (new moon), March 25Descending node (full moon) ...
Eclipse season of March 2062
March 11
Ascending node (new moon)
March 25
Descending node (full moon)
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Partial solar eclipse
Solar Saros 121
Total lunar eclipse
Lunar Saros 133
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Eclipses in 2062

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 121

Inex

Triad

Solar eclipses of 2062–2065

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 July 3, 2065 and December 27, 2065 occur in the next lunar year eclipse set.

More information series sets from 2062 to 2065, Ascending node ...
Solar eclipse series sets from 2062 to 2065
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
121 March 11, 2062
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Partial
−1.0238 126 September 3, 2062
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Partial
1.0191
131 February 28, 2063
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Annular
−0.336 136 August 24, 2063
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Total
0.2771
141 February 17, 2064
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Annular
0.3597 146 August 12, 2064
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Total
−0.4652
151 February 5, 2065
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Partial
1.0336 156 August 2, 2065
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Partial
−1.2759
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Saros 121

This eclipse is a part of Saros series 121, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on April 25, 944 AD. It contains total eclipses from July 10, 1070 through October 9, 1809; hybrid eclipses on October 20, 1827 and October 30, 1845; and annular eclipses from November 11, 1863 through February 28, 2044. The series ends at member 71 as a partial eclipse on June 7, 2206. 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 39 at 6 minutes, 20 seconds on June 21, 1629, and the longest duration of annularity will be produced by member 62 at 2 minutes, 27 seconds on February 28, 2044. All eclipses in this series occur at the Moon’s ascending node of orbit.[4]

More information Series members 49–70 occur between 1801 and 2200: ...
Series members 49–70 occur between 1801 and 2200:
49 50 51
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October 9, 1809
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October 20, 1827
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October 30, 1845
52 53 54
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November 11, 1863
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November 21, 1881
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December 3, 1899
55 56 57
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December 14, 1917
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December 25, 1935
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January 5, 1954
58 59 60
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January 16, 1972
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January 26, 1990
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February 7, 2008
61 62 63
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February 17, 2026
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February 28, 2044
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March 11, 2062
64 65 66
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March 21, 2080
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April 1, 2098
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April 13, 2116
67 68 69
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April 24, 2134
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May 4, 2152
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May 16, 2170
70
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May 26, 2188
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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.

More information 23 eclipse events between August 3, 2054 and October 16, 2145, August 3–4 ...
23 eclipse events between August 3, 2054 and October 16, 2145
August 3–4 May 22–24 March 10–11 December 27–29 October 14–16
117 119 121 123 125
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August 3, 2054
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May 22, 2058
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March 11, 2062
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December 27, 2065
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October 15, 2069
127 129 131 133 135
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August 3, 2073
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May 22, 2077
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March 10, 2081
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December 27, 2084
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October 14, 2088
137 139 141 143 145
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August 3, 2092
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May 22, 2096
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March 10, 2100
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December 29, 2103
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October 16, 2107
147 149 151 153 155
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August 4, 2111
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May 24, 2115
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March 11, 2119
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December 28, 2122
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October 16, 2126
157 159 161 163 165
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August 4, 2130
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May 23, 2134
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October 16, 2145
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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.

More information Series members between 2018 and 2200 ...
Series members between 2018 and 2200
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July 13, 2018
(Saros 117)
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June 12, 2029
(Saros 118)
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May 11, 2040
(Saros 119)
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April 11, 2051
(Saros 120)
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March 11, 2062
(Saros 121)
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February 7, 2073
(Saros 122)
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January 7, 2084
(Saros 123)
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December 7, 2094
(Saros 124)
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November 6, 2105
(Saros 125)
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October 6, 2116
(Saros 126)
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September 6, 2127
(Saros 127)
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August 5, 2138
(Saros 128)
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July 5, 2149
(Saros 129)
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June 4, 2160
(Saros 130)
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May 5, 2171
(Saros 131)
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April 3, 2182
(Saros 132)
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March 3, 2193
(Saros 133)
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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.

More information Series members between 1801 and 2200 ...
Series members between 1801 and 2200
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September 8, 1801
(Saros 112)
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August 18, 1830
(Saros 113)
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July 29, 1859
(Saros 114)
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July 9, 1888
(Saros 115)
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June 19, 1917
(Saros 116)
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May 30, 1946
(Saros 117)
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May 11, 1975
(Saros 118)
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April 19, 2004
(Saros 119)
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March 30, 2033
(Saros 120)
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March 11, 2062
(Saros 121)
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February 18, 2091
(Saros 122)
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January 30, 2120
(Saros 123)
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January 9, 2149
(Saros 124)
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December 20, 2177
(Saros 125)
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References

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