Solar eclipse of March 30, 2033

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Solar eclipse of March 30, 2033

A total solar eclipse will occur at the Moon's descending node of orbit on Wednesday, March 30, 2033,[1] with a magnitude of 1.0462. 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 11 hours after perigee (on March 30, 2033, at 7:10 UTC), the Moon's apparent diameter will be larger.[2]

Quick Facts Gamma, Magnitude ...
Solar eclipse of March 30, 2033
Total eclipse
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Map
Gamma0.9778
Magnitude1.0462
Maximum eclipse
Duration157 s (2 min 37 s)
Coordinates71.3°N 155.8°W / 71.3; -155.8
Max. width of band781 km (485 mi)
Times (UTC)
Greatest eclipse18:02:36
References
Saros120 (62 of 71)
Catalog # (SE5000)9581
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Totality will be visible from parts of the Russian Far East and Alaska, including in the cities of Nome, Alaska and Utqiaġvik, Alaska in the mid-morning hours. A partial eclipse will be visible for parts of eastern Russia, Hawaii, North America, Greenland, and Iceland. This will be the last of 55 umbral eclipses in Solar Saros 120.

Images

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Animated path

Details of totality in some places or cities

More information Country or Territory, Place or City ...
Solar Eclipse of March 30 and March 31, 2033
Country or Territory Place or City Start

of
partial
eclipse
(Local Time)

Start of
total
eclipse (Local Time)
End of
total
eclipse (Local Time)
Duration of
total
eclipse
End of
partial
eclipse (Local Time)
Magnitude
 United StatesGambell, Alaska08:57:55 (sunrise)09:44:2209:46:402 min 18s10:42:151,044
 United StatesNome, Alaska08:51:5309:46:0509:48:352 min 30s10:45:171,045
 RussiaAnadyr, Chukotka Autonomous Okrug05:39:24 (sunrise) (March 31)06:47:12 (March 31)06:48:01 (March 31)50 s07:42:27 (March 31)1,043
 RussiaUelen, Chukotka Autonomous Okrug05:55:06 (March 31)06:48:57 (March 31)06:50:55 (March 31)1 min 58 s07:47:02 (March 31)1,045
 United StatesKotzebue, Alaska08:56:0109:50:4809:53:192 min 31s10:50:251,046
 United StatesUtqiagvik, Alaska09:04:0809:59:4610:02:222 min 36s10:59:521,046
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Eclipse details

Summarize
Perspective

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]

More information Event, Time (UTC) ...
March 30, 2033 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 2033 March 30 at 16:00:45.9 UTC
First Umbral External Contact 2033 March 30 at 17:37:02.7 UTC
First Central Line 2033 March 30 at 17:42:17.4 UTC
First Umbral Internal Contact 2033 March 30 at 17:49:24.8 UTC
Ecliptic Conjunction 2033 March 30 at 17:52:49.1 UTC
Greatest Duration 2033 March 30 at 18:02:19.5 UTC
Greatest Eclipse 2033 March 30 at 18:02:35.7 UTC
Last Umbral Internal Contact 2033 March 30 at 18:15:23.7 UTC
Last Central Line 2033 March 30 at 18:22:30.8 UTC
Last Umbral External Contact 2033 March 30 at 18:27:45.2 UTC
Equatorial Conjunction 2033 March 30 at 18:34:26.6 UTC
Last Penumbral External Contact 2033 March 30 at 20:04:11.4 UTC
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More information Parameter, Value ...
March 30, 2033 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 1.04616
Eclipse Obscuration 1.09444
Gamma 0.97777
Sun Right Ascension 00h38m02.8s
Sun Declination +04°05'47.8"
Sun Semi-Diameter 16'00.8"
Sun Equatorial Horizontal Parallax 08.8"
Moon Right Ascension 00h36m50.4s
Moon Declination +05°02'48.6"
Moon Semi-Diameter 16'42.2"
Moon Equatorial Horizontal Parallax 1°01'18.3"
ΔT 75.3 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 30Descending node (new moon), April 14Ascending node (full moon) ...
Eclipse season of March–April 2033
March 30
Descending node (new moon)
April 14
Ascending node (full moon)
ThumbThumb
Partial solar eclipse
Solar Saros 120
Total lunar eclipse
Lunar Saros 132
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Eclipses in 2033

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 120

Inex

Triad

Solar eclipses of 2033–2036

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 eclipse on July 23, 2036 occurs in the next lunar year eclipse set.

More information series sets from 2033 to 2036, Descending node ...
Solar eclipse series sets from 2033 to 2036
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
120 March 30, 2033
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Total
0.9778 125 September 23, 2033
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Partial
−1.1583
130 March 20, 2034
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Total
0.2894 135 September 12, 2034
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Annular
−0.3936
140 March 9, 2035
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Annular
−0.4368 145 September 2, 2035
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Total
0.3727
150 February 27, 2036
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Partial
−1.1942 155 August 21, 2036
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Partial
1.0825
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Saros 120

This eclipse is a part of Saros series 120, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on May 27, 933 AD. It contains annular eclipses from August 11, 1059 through April 26, 1492; hybrid eclipses from May 8, 1510 through June 8, 1564; and total eclipses from June 20, 1582 through March 30, 2033. The series ends at member 71 as a partial eclipse on July 7, 2195. 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 11 at 6 minutes, 24 seconds on September 11, 1113, and the longest duration of totality was produced by member 60 at 2 minutes, 50 seconds on March 9, 1997. All eclipses in this series occur at the Moon’s descending node of orbit.[5]

More information Series members 50–71 occur between 1801 and 2195: ...
Series members 50–71 occur between 1801 and 2195:
50 51 52
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November 19, 1816
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November 30, 1834
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December 11, 1852
53 54 55
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December 22, 1870
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January 1, 1889
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January 14, 1907
56 57 58
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January 24, 1925
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February 4, 1943
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February 15, 1961
59 60 61
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February 26, 1979
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March 9, 1997
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March 20, 2015
62 63 64
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March 30, 2033
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April 11, 2051
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April 21, 2069
65 66 67
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May 2, 2087
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May 14, 2105
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May 25, 2123
68 69 70
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June 4, 2141
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June 16, 2159
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June 26, 2177
71
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July 7, 2195
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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 descending node.

More information 22 eclipse events between June 12, 2029 and November 4, 2116, June 11–12 ...
22 eclipse events between June 12, 2029 and November 4, 2116
June 11–12 March 30–31 January 16 November 4–5 August 23–24
118 120 122 124 126
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June 12, 2029
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March 30, 2033
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January 16, 2037
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November 4, 2040
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August 23, 2044
128 130 132 134 136
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June 11, 2048
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March 30, 2052
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January 16, 2056
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November 5, 2059
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August 24, 2063
138 140 142 144 146
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June 11, 2067
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March 31, 2071
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January 16, 2075
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November 4, 2078
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August 24, 2082
148 150 152 154 156
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June 11, 2086
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March 31, 2090
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January 16, 2094
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November 4, 2097
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August 24, 2101
158 160 162 164
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June 12, 2105
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November 4, 2116
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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.

The partial solar eclipses on April 8, 1902 (part of Saros 108) and January 5, 1935 (part of Saros 111) are also a part of this series but are not included in the table below.

More information Series members between 2000 and 2200 ...
Series members between 2000 and 2200
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July 1, 2000
(Saros 117)
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June 1, 2011
(Saros 118)
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April 30, 2022
(Saros 119)
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March 30, 2033
(Saros 120)
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February 28, 2044
(Saros 121)
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January 27, 2055
(Saros 122)
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December 27, 2065
(Saros 123)
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November 26, 2076
(Saros 124)
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October 26, 2087
(Saros 125)
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September 25, 2098
(Saros 126)
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August 26, 2109
(Saros 127)
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July 25, 2120
(Saros 128)
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June 25, 2131
(Saros 129)
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May 25, 2142
(Saros 130)
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April 23, 2153
(Saros 131)
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March 23, 2164
(Saros 132)
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February 21, 2175
(Saros 133)
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January 20, 2186
(Saros 134)
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December 19, 2196
(Saros 135)
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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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