Solar eclipse of November 25, 2030

Last updated
Solar eclipse of November 25, 2030
SE2030Nov25T.png
Map
Type of eclipse
NatureTotal
Gamma −0.3867
Magnitude 1.0468
Maximum eclipse
Duration224 s (3 min 44 s)
Coordinates 43°36′S71°12′E / 43.6°S 71.2°E / -43.6; 71.2
Max. width of band169 km (105 mi)
Times (UTC)
Greatest eclipse6:51:37
References
Saros 133 (46 of 72)
Catalog # (SE5000) 9576

A total solar eclipse will occur at the Moon's ascending node of orbit on Monday, November 25, 2030, [1] with a magnitude of 1.0468. 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 only about 14 hours before perigee (on November 25, 2030, at 21:10 UTC), the Moon's apparent diameter will be larger. [2]

Contents

Totality will be visible in Namibia, Botswana, South Africa, Lesotho, and Australia. A partial eclipse will be visible for much of Central and Southern Africa, Antarctica, Australia, and Indonesia.

Path

The path of totality will begin in the Atlantic Ocean. It will then pass through Namibia (serving the capital Windhoek), Botswana (serving Tsabong), and South Africa (serving Durban; also visible in parts of Lesotho). After that, it will pass through the Indian Ocean, where it will terminate in Australia (visiting the states of South Australia, New South Wales, and Queensland). [3]

Images

SE2030Nov25T.gif
Animated path

Details of totality in some places or cities

Solar Eclipse of November 25, 2030
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 Namibia.svg  Namibia Henties Bay, Erongo Region 06:24:4107:18:3607:19:3458 s08:19:121,034
Flag of Namibia.svg  Namibia Windhoek, Khomas Region 06:24:0407:18:5607:20:481 min 52s08:21:251,035
Flag of Namibia.svg  Namibia Rehoboth, Hardap Region 06:25:0907:20:0007:21:251 min 25 s08:22:201,035
Flag of Botswana.svg  Botswana Tsabong, Kgalagadi District 06:27:1707:24:4507:25:471 min 02s08:29:551,037
Flag of South Africa.svg  South Africa Vryburg, North West Province 06:28:1807:26:2707:28:171 min 50 s08:33:231,038
Flag of South Africa.svg  South Africa Matlosana, North West Province 06:28:1507:27:2307:28:571 min 34 s08:35:181,038
Flag of South Africa.svg  South Africa Welkom, Free State Province 06:29:3707:28:4607:30:371 min 51 s08:36:561,038
Flag of South Africa.svg  South Africa Bethlehem, Free State Province 06:30:0507:29:4007:32:072 min 27 s08:39:041,039
Flag of Lesotho.svg  Lesotho Butha-Buthe, Butha-Buthe District 06:30:4407:30:4107:32:271 min 47 s08:39:431,039
Flag of Lesotho.svg  Lesotho Mokhotlong, Mokhotlong District 06:31:3007:32:0407:33:261 min 22 s08:41:231,039
Flag of South Africa.svg  South Africa Pietermaritzburg, KwaZulu-Natal Province 06:32:0807:32:5407:35:132 min 19 s08:43:311,040
Flag of South Africa.svg  South Africa Durban, KwaZulu-Natal Province 06:32:3707:33:4107:36:042 min 24 s08:44:431,040
Flag of Australia (converted).svg  Australia Wudinna, South Australia 17:49:3918:50:0518:51:121 min 06 s19:16:021,035
Flag of Australia (converted).svg  Australia Cunnamulla, Queensland 17:29:0618:24:4518:25:591 min 14 s18:50:51 (sunset)1,032
Flag of Australia (converted).svg  Australia Condamine, Queensland 17:30:5018:24:3518:26:041 min 29 s18:30:47 (sunset)1,030

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. [4]

November 25, 2030 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2030 November 25 at 04:17:55.5 UTC
First Umbral External Contact2030 November 25 at 05:15:34.1 UTC
First Central Line2030 November 25 at 05:16:26.9 UTC
First Umbral Internal Contact2030 November 25 at 05:17:19.8 UTC
First Penumbral Internal Contact2030 November 25 at 06:25:54.6 UTC
Ecliptic Conjunction2030 November 25 at 06:47:39.2 UTC
Greatest Eclipse2030 November 25 at 06:51:36.9 UTC
Greatest Duration2030 November 25 at 06:53:10.2 UTC
Equatorial Conjunction2030 November 25 at 06:55:25.4 UTC
Last Penumbral Internal Contact2030 November 25 at 07:17:13.7 UTC
Last Umbral Internal Contact2030 November 25 at 08:25:50.4 UTC
Last Central Line2030 November 25 at 08:26:44.0 UTC
Last Umbral External Contact2030 November 25 at 08:27:37.6 UTC
Last Penumbral External Contact2030 November 25 at 09:25:15.0 UTC
November 25, 2030 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude1.04684
Eclipse Obscuration1.09588
Gamma−0.38669
Sun Right Ascension16h03m58.7s
Sun Declination-20°45'39.0"
Sun Semi-Diameter16'12.1"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension16h03m49.1s
Moon Declination-21°09'10.6"
Moon Semi-Diameter16'41.7"
Moon Equatorial Horizontal Parallax1°01'16.4"
ΔT74.2 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 November–December 2030
November 25
Ascending node (new moon)
December 9
Descending node (full moon)
SE2030Nov25T.png Lunar eclipse chart close-2030Dec09.png
Total solar eclipse
Solar Saros 133
Penumbral lunar eclipse
Lunar Saros 145

Eclipses in 2030

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 133

Inex

Triad

Solar eclipses of 2029–2032

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. [5]

The partial solar eclipses on January 14, 2029 and July 11, 2029 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 2029 to 2032
Descending node Ascending node
SarosMapGammaSarosMapGamma
118 June 12, 2029
SE2029Jun12P.png
Partial
1.29431123 December 5, 2029
SE2029Dec05P.png
Partial
−1.06090
128 June 1, 2030
SE2030Jun01A.png
Annular
0.56265133 November 25, 2030
SE2030Nov25T.png
Total
−0.38669
138 May 21, 2031
SE2031May21A.png
Annular
−0.19699143 November 14, 2031
SE2031Nov14H.png
Hybrid
0.30776
148 May 9, 2032
SE2032May09A.png
Annular
−0.93748153 November 3, 2032
SE2032Nov03P.png
Partial
1.06431

Saros 133

This eclipse is a part of Saros series 133, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on July 13, 1219. It contains annular eclipses from November 20, 1435 through January 13, 1526; a hybrid eclipse on January 24, 1544; and total eclipses from February 3, 1562 through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. 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 1 minutes, 14 seconds on November 30, 1453, and the longest duration of totality was produced by member 61 at 6 minutes, 50 seconds on August 7, 1850. All eclipses in this series occur at the Moon’s ascending node of orbit. [6]

Series members 34–55 occur between 1801 and 2200:
343536
SE1814Jul17T.png
July 17, 1814
SE1832Jul27T.png
July 27, 1832
SE1850Aug07T.png
August 7, 1850
373839
SE1868Aug18T.png
August 18, 1868
SE1886Aug29T.png
August 29, 1886
SE1904Sep09T.png
September 9, 1904
404142
SE1922Sep21T.png
September 21, 1922
SE1940Oct01T.png
October 1, 1940
SE1958Oct12T.png
October 12, 1958
434445
SE1976Oct23T.png
October 23, 1976
SE1994Nov03T.png
November 3, 1994
SE2012Nov13T.png
November 13, 2012
464748
SE2030Nov25T.png
November 25, 2030
SE2048Dec05T.png
December 5, 2048
SE2066Dec17T.png
December 17, 2066
495051
SE2084Dec27T.png
December 27, 2084
SE2103Jan08T.png
January 8, 2103
SE2121Jan19T.png
January 19, 2121
525354
SE2139Jan30T.png
January 30, 2139
SE2157Feb09T.png
February 9, 2157
SE2175Feb21T.png
February 21, 2175
55
SE2193Mar03T.png
March 3, 2193

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 1, 2000 and July 1, 2076
July 1–2April 19–20February 5–7November 24–25September 12–13
117119121123125
SE2000Jul01P.png
July 1, 2000
SE2004Apr19P.png
April 19, 2004
SE2008Feb07A.png
February 7, 2008
SE2011Nov25P.png
November 25, 2011
SE2015Sep13P.png
September 13, 2015
127129131133135
SE2019Jul02T.png
July 2, 2019
SE2023Apr20H.png
April 20, 2023
SE2027Feb06A.png
February 6, 2027
SE2030Nov25T.png
November 25, 2030
SE2034Sep12A.png
September 12, 2034
137139141143145
SE2038Jul02A.png
July 2, 2038
SE2042Apr20T.png
April 20, 2042
SE2046Feb05A.png
February 5, 2046
SE2049Nov25H.png
November 25, 2049
SE2053Sep12T.png
September 12, 2053
147149151153155
SE2057Jul01A.png
July 1, 2057
SE2061Apr20T.png
April 20, 2061
SE2065Feb05P.png
February 5, 2065
SE2068Nov24P.png
November 24, 2068
SE2072Sep12T.png
September 12, 2072
157
SE2076Jul01P.png
July 1, 2076

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
SE1801Sep08P.png
September 8, 1801
(Saros 112)
SE1812Aug07P.gif
August 7, 1812
(Saros 113)
SE1823Jul08P.gif
July 8, 1823
(Saros 114)
SE1834Jun07P.gif
June 7, 1834
(Saros 115)
SE1845May06An.gif
May 6, 1845
(Saros 116)
SE1856Apr05T.gif
April 5, 1856
(Saros 117)
SE1867Mar06A.gif
March 6, 1867
(Saros 118)
SE1878Feb02A.gif
February 2, 1878
(Saros 119)
SE1889Jan01T.png
January 1, 1889
(Saros 120)
SE1899Dec03A.png
December 3, 1899
(Saros 121)
SE1910Nov02P.png
November 2, 1910
(Saros 122)
SE1921Oct01T.png
October 1, 1921
(Saros 123)
SE1932Aug31T.png
August 31, 1932
(Saros 124)
SE1943Aug01A.png
August 1, 1943
(Saros 125)
SE1954Jun30T.png
June 30, 1954
(Saros 126)
SE1965May30T.png
May 30, 1965
(Saros 127)
SE1976Apr29A.png
April 29, 1976
(Saros 128)
SE1987Mar29H.png
March 29, 1987
(Saros 129)
SE1998Feb26T.png
February 26, 1998
(Saros 130)
SE2009Jan26A.png
January 26, 2009
(Saros 131)
SE2019Dec26A.png
December 26, 2019
(Saros 132)
SE2030Nov25T.png
November 25, 2030
(Saros 133)
SE2041Oct25A.png
October 25, 2041
(Saros 134)
SE2052Sep22A.png
September 22, 2052
(Saros 135)
SE2063Aug24T.png
August 24, 2063
(Saros 136)
SE2074Jul24A.png
July 24, 2074
(Saros 137)
SE2085Jun22A.png
June 22, 2085
(Saros 138)
SE2096May22T.png
May 22, 2096
(Saros 139)
SE2107Apr23A.png
April 23, 2107
(Saros 140)
SE2118Mar22A.png
March 22, 2118
(Saros 141)
SE2129Feb18T.png
February 18, 2129
(Saros 142)
SE2140Jan20A.png
January 20, 2140
(Saros 143)
SE2150Dec19A.png
December 19, 2150
(Saros 144)
SE2161Nov17T.png
November 17, 2161
(Saros 145)
SE2172Oct17H.png
October 17, 2172
(Saros 146)
Saros147 32van80 SE2183Sep16A.jpg
September 16, 2183
(Saros 147)
Saros148 31van75 SE2194Aug16T.jpg
August 16, 2194
(Saros 148)

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
Saros126 37van72 SE1828Apr14H.jpg
April 14, 1828
(Saros 126)
SE1857Mar25T.png
March 25, 1857
(Saros 127)
SE1886Mar05A.gif
March 5, 1886
(Saros 128)
SE1915Feb14A.png
February 14, 1915
(Saros 129)
SE1944Jan25T.png
January 25, 1944
(Saros 130)
SE1973Jan04A.png
January 4, 1973
(Saros 131)
SE2001Dec14A.png
December 14, 2001
(Saros 132)
SE2030Nov25T.png
November 25, 2030
(Saros 133)
SE2059Nov05A.png
November 5, 2059
(Saros 134)
SE2088Oct14A.png
October 14, 2088
(Saros 135)
SE2117Sep26T.png
September 26, 2117
(Saros 136)
SE2146Sep06A.png
September 6, 2146
(Saros 137)
SE2175Aug16A.png
August 16, 2175
(Saros 138)

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<span class="mw-page-title-main">Solar eclipse of October 12, 1939</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit on Thursday, October 12, 1939, with a magnitude of 1.0266. 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 1.8 days after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of October 1, 1921</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit on Saturday, October 1, 1921, with a magnitude of 1.0293. 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 1.9 days after perigee, the Moon's apparent diameter was larger.

References

  1. "November 25, 2030 Total Solar Eclipse". timeanddate. Retrieved 13 August 2024.
  2. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 13 August 2024.
  3. "Total Solar Eclipse on November 25, 2030: Path Map and Times". www.timeanddate.com. Retrieved 2024-04-19.
  4. "Total Solar Eclipse of 2030 Nov 25". EclipseWise.com. Retrieved 13 August 2024.
  5. 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.
  6. "NASA - Catalog of Solar Eclipses of Saros 133". eclipse.gsfc.nasa.gov.