Solar eclipse of March 30, 2033

Last updated
Solar eclipse of March 30, 2033
SE2033Mar30T.png
Map
Type of eclipse
NatureTotal
Gamma 0.9778
Magnitude 1.0462
Maximum eclipse
Duration157 s (2 min 37 s)
Coordinates 71°18′N155°48′W / 71.3°N 155.8°W / 71.3; -155.8
Max. width of band781 km (485 mi)
Times (UTC)
Greatest eclipse18:02:36
References
Saros 120 (62 of 71)
Catalog # (SE5000) 9581

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]

Contents

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

SE2033Mar30T.gif
Animated path

Details of totality in some places or cities

Solar Eclipse of March 30 and March 31, 2033
Country or TerritoryPlace or CityStart

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
Flag of the United States (23px).png  United States Gambell, Alaska 08:57:55 (sunrise)09:44:2209:46:402 min 18s10:42:151,044
Flag of the United States (23px).png  United States Nome, Alaska 08:51:5309:46:0509:48:352 min 30s10:45:171,045
Flag of Russia.svg  Russia Anadyr, Chukotka Autonomous Okrug 05:39:24 (sunrise) (March 31)06:47:12 (March 31)06:48:01 (March 31)50 s07:42:27 (March 31)1,043
Flag of Russia.svg  Russia Uelen, Chukotka Autonomous Okrug 05:55:06 (March 31)06:48:57 (March 31)06:50:55 (March 31)1 min 58 s07:47:02 (March 31)1,045
Flag of the United States (23px).png  United States Kotzebue, Alaska 08:56:0109:50:4809:53:192 min 31s10:50:251,046
Flag of the United States (23px).png  United States Utqiagvik, Alaska 09:04:0809:59:4610:02:222 min 36s10:59:521,046

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. [3]

March 30, 2033 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2033 March 30 at 16:00:45.9 UTC
First Umbral External Contact2033 March 30 at 17:37:02.7 UTC
First Central Line2033 March 30 at 17:42:17.4 UTC
First Umbral Internal Contact2033 March 30 at 17:49:24.8 UTC
Ecliptic Conjunction2033 March 30 at 17:52:49.1 UTC
Greatest Duration2033 March 30 at 18:02:19.5 UTC
Greatest Eclipse2033 March 30 at 18:02:35.7 UTC
Last Umbral Internal Contact2033 March 30 at 18:15:23.7 UTC
Last Central Line2033 March 30 at 18:22:30.8 UTC
Last Umbral External Contact2033 March 30 at 18:27:45.2 UTC
Equatorial Conjunction2033 March 30 at 18:34:26.6 UTC
Last Penumbral External Contact2033 March 30 at 20:04:11.4 UTC
March 30, 2033 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude1.04616
Eclipse Obscuration1.09444
Gamma0.97777
Sun Right Ascension00h38m02.8s
Sun Declination+04°05'47.8"
Sun Semi-Diameter16'00.8"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension00h36m50.4s
Moon Declination+05°02'48.6"
Moon Semi-Diameter16'42.2"
Moon Equatorial Horizontal Parallax1°01'18.3"
ΔT75.3 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 March–April 2033
March 30
Descending node (new moon)
April 14
Ascending node (full moon)
SE2033Mar30T.png Lunar eclipse chart close-2033Apr14.png
Partial solar eclipse
Solar Saros 120
Total lunar eclipse
Lunar Saros 132

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.

Solar eclipse series sets from 2033 to 2036
Descending node Ascending node
SarosMapGammaSarosMapGamma
120 March 30, 2033
SE2033Mar30T.png
Total
0.9778125 September 23, 2033
SE2033Sep23P.png
Partial
−1.1583
130 March 20, 2034
SE2034Mar20T.png
Total
0.2894135 September 12, 2034
SE2034Sep12A.png
Annular
−0.3936
140 March 9, 2035
SE2035Mar09A.png
Annular
−0.4368145 September 2, 2035
SE2035Sep02T.png
Total
0.3727
150 February 27, 2036
SE2036Feb27P.png
Partial
−1.1942155 August 21, 2036
SE2036Aug21P.png
Partial
1.0825

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]

Series members 50–71 occur between 1801 and 2195:
505152
SE1816Nov19T.gif
November 19, 1816
SE1834Nov30T.gif
November 30, 1834
SE1852Dec11T.gif
December 11, 1852
535455
SE1870Dec22T.gif
December 22, 1870
SE1889Jan01T.png
January 1, 1889
SE1907Jan14T.png
January 14, 1907
565758
SE1925Jan24T.png
January 24, 1925
SE1943Feb04T.png
February 4, 1943
SE1961Feb15T.png
February 15, 1961
596061
SE1979Feb26T.png
February 26, 1979
SE1997Mar09T.png
March 9, 1997
SE2015Mar20T.png
March 20, 2015
626364
SE2033Mar30T.png
March 30, 2033
SE2051Apr11P.png
April 11, 2051
SE2069Apr21P.png
April 21, 2069
656667
SE2087May02P.png
May 2, 2087
Saros120 66van71 SE2105May14P.jpg
May 14, 2105
Saros120 67van71 SE2123May25P.jpg
May 25, 2123
686970
Saros120 68van71 SE2141Jun04P.jpg
June 4, 2141
Saros120 69van71 SE2159Jun16P.jpg
June 16, 2159
Saros120 70van71 SE2177Jun26P.jpg
June 26, 2177
71
Saros120 71van71 SE2195Jul07P.jpg
July 7, 2195

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 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.

Series members between 2000 and 2200
SE2000Jul01P.png
July 1, 2000
(Saros 117)
SE2011Jun01P.png
June 1, 2011
(Saros 118)
SE2022Apr30P.png
April 30, 2022
(Saros 119)
SE2033Mar30T.png
March 30, 2033
(Saros 120)
SE2044Feb28A.png
February 28, 2044
(Saros 121)
SE2055Jan27P.png
January 27, 2055
(Saros 122)
SE2065Dec27P.png
December 27, 2065
(Saros 123)
SE2076Nov26P.png
November 26, 2076
(Saros 124)
SE2087Oct26P.png
October 26, 2087
(Saros 125)
SE2098Sep25P.png
September 25, 2098
(Saros 126)
Saros127 63van82 SE2109Aug26P.jpg
August 26, 2109
(Saros 127)
SE2120Jul25A.png
July 25, 2120
(Saros 128)
Saros129 58van80 SE2131Jun25T.jpg
June 25, 2131
(Saros 129)
SE2142May25T.png
May 25, 2142
(Saros 130)
SE2153Apr23A.png
April 23, 2153
(Saros 131)
SE2164Mar23H.png
March 23, 2164
(Saros 132)
SE2175Feb21T.png
February 21, 2175
(Saros 133)
SE2186Jan20A.png
January 20, 2186
(Saros 134)
SE2196Dec19A.png
December 19, 2196
(Saros 135)

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
SE1801Sep08P.png
September 8, 1801
(Saros 112)
SE1830Aug18P.gif
August 18, 1830
(Saros 113)
SE1859Jul29P.gif
July 29, 1859
(Saros 114)
SE1888Jul09P.gif
July 9, 1888
(Saros 115)
SE1917Jun19P.png
June 19, 1917
(Saros 116)
SE1946May30P.png
May 30, 1946
(Saros 117)
SE1975May11P.png
May 11, 1975
(Saros 118)
SE2004Apr19P.png
April 19, 2004
(Saros 119)
SE2033Mar30T.png
March 30, 2033
(Saros 120)
SE2062Mar11P.png
March 11, 2062
(Saros 121)
SE2091Feb18P.png
February 18, 2091
(Saros 122)
Saros123 59van70 SE2120Jan30P.jpg
January 30, 2120
(Saros 123)
Saros124 62van73 SE2149Jan09P.jpg
January 9, 2149
(Saros 124)
Saros125 63van73 SE2177Dec20P.jpg
December 20, 2177
(Saros 125)

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References

  1. "March 30, 2033 Total Solar Eclipse". timeanddate. Retrieved 14 August 2024.
  2. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 14 August 2024.
  3. "Total Solar Eclipse of 2033 Mar 30". EclipseWise.com. Retrieved 14 August 2024.
  4. 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.
  5. "NASA - Catalog of Solar Eclipses of Saros 120". eclipse.gsfc.nasa.gov.