Solar eclipse of November 13, 2012

Last updated
Solar eclipse of November 13, 2012
Solar eclipse of 2012 november 14 near Mt Carbine.jpg
Totality as seen from Mount Carbine, Queensland
SE2012Nov13T.png
Map
Type of eclipse
NatureTotal
Gamma −0.3719
Magnitude 1.05
Maximum eclipse
Duration242 s (4 min 2 s)
Coordinates 40°00′S161°18′W / 40°S 161.3°W / -40; -161.3
Max. width of band179 km (111 mi)
Times (UTC)
(P1) Partial begin19:37:58
(U1) Total begin20:35:08
Greatest eclipse22:12:55
(U4) Total end23:48:24
(P4) Partial end0:45:34
References
Saros 133 (45 of 72)
Catalog # (SE5000) 9536

A total solar eclipse occurred at the Moon's ascending node of orbit between Tuesday, November 13 and Wednesday, November 14, 2012, [1] [2] [3] with a magnitude of 1.05. 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 12 hours before perigee (on November 14, 2012, at 10:20 UTC), the Moon's apparent diameter was larger. [4]

Contents

Because it crossed the International Date Line it began in local time on November 14 west of the date line over northern Australia, and ended in local time on November 13 east of the date line near the west coast of South America. Totality was visible from parts of Northern Australia. A partial eclipse was visible for parts of Australia, New Zealand, Oceania, West Antarctica, the Antarctic Peninsula, and southern South America.

Visibility

SolarEclipse2012Nov13T.GIF

For this eclipse, totality was visible from northern Australia to about 470 km north of the Chilean Juan Fernández Islands in the southern Pacific Ocean where totality ended. The most populous city to experience totality was Cairns, which had around 2 minutes of totality an hour after daybreak (06:39 AEST, 20:39 UTC) with the sun at an altitude of 14°. [5] Norfolk Island, a small Pacific island east of Australia, experienced a partial eclipse with a maximum eclipse of 98% of the sun obscured at 08:37 NFT and an altitude of 42°.

New Zealand experienced a partial eclipse. Auckland had 84.8% of the sun obscured, whereas Wellington, Christchurch and Dunedin respectively had 71.2%, 61.9% and 52.9% of the sun obscured. Maximum eclipse over New Zealand occurred around 10:30 NZDT (21:30 UTC), with Auckland at 10:27, Wellington at 10:34, Christchurch at 10:35 and Dunedin at 10:36. [6] [7]

Most of Chile and parts of Argentina saw a partial eclipse at sunset. In some places over half the sun was obscured. In Chile, Talcahuano in Biobío saw 72% obscured, Castro in Los Lagos saw 56% obscured. Chilean coastal locations were ideally situated to observe an eclipsing sunset over the Pacific Ocean. Points further north, up to about Chañaral, saw the eclipse begin as the sun was setting.

West of the International Date Line the eclipse took place on the morning of November 14. The maximum eclipse totality, of duration 4 min 2 sec, occurred east of the International Date Line on November 13, approximately 2,000 km east of New Zealand, and 9,600 km west of Chile.

On the morning of November 14, skies in Auckland were cloudy, obscuring much of the eclipse, which peaked at 10:27 NZDT. [8] Cloud also obscured the moment of totality at Cairns, disappointing many tourists that had flocked to the area. Eclipse chasers along the northern beaches up through to Port Douglas generally got a clear view, however.

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. [9]

November 13, 2012 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2012 November 13 at 19:39:04.9 UTC
First Umbral External Contact2012 November 13 at 20:36:15.3 UTC
First Central Line2012 November 13 at 20:37:12.9 UTC
First Umbral Internal Contact2012 November 13 at 20:38:10.6 UTC
First Penumbral Internal Contact2012 November 13 at 21:44:49.3 UTC
Ecliptic Conjunction2012 November 13 at 22:09:06.9 UTC
Greatest Eclipse2012 November 13 at 22:12:55.2 UTC
Greatest Duration2012 November 13 at 22:15:06.9 UTC
Equatorial Conjunction2012 November 13 at 22:19:11.7 UTC
Last Penumbral Internal Contact2012 November 13 at 22:40:51.6 UTC
Last Umbral Internal Contact2012 November 13 at 23:47:34.6 UTC
Last Central Line2012 November 13 at 23:48:32.9 UTC
Last Umbral External Contact2012 November 13 at 23:49:31.1 UTC
Last Penumbral External Contact2012 November 14 at 00:46:41.3 UTC
November 13, 2012 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude1.05004
Eclipse Obscuration1.10259
Gamma−0.37189
Sun Right Ascension15h18m06.7s
Sun Declination-18°15'02.6"
Sun Semi-Diameter16'09.9"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension15h17m51.2s
Moon Declination-18°37'29.5"
Moon Semi-Diameter16'42.4"
Moon Equatorial Horizontal Parallax1°01'19.0"
ΔT66.8 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 2012
November 13
Ascending node (new moon)
November 28
Descending node (full moon)
SE2012Nov13T.png Lunar eclipse chart close-2012Nov28.png
Total solar eclipse
Solar Saros 133
Penumbral lunar eclipse
Lunar Saros 145

Eclipses in 2012

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 133

Inex

Triad

Solar eclipses of 2011–2014

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. [10]

The partial solar eclipses on January 4, 2011 and July 1, 2011 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 2011 to 2014
Descending node Ascending node
SarosMapGammaSarosMapGamma
118
Partial solar eclipse Tromso 2011-05-31 (cropped).jpg
Partial in Tromsø, Norway
June 1, 2011
SE2011Jun01P.png
Partial
1.21300123
Partial Solar Eclipse of 2011 11 25 -Hinode XRT- freeze frame.png
Hinode XRT footage
November 25, 2011
SE2011Nov25P.png
Partial
−1.05359
128
Solar Eclipse May 20,2012.jpg
Annularity in Red Bluff, CA, USA
May 20, 2012
SE2012May20A.png
Annular
0.48279133
Solar eclipse of 2012 november 14 near Mt Carbine.jpg
Totality in Mount Carbine, Queensland, Australia
November 13, 2012
SE2012Nov13T.png
Total
−0.37189
138
Annular Solar Eclipse May 10 2013 Northern Territory Australia.JPG
Annularity in Churchills Head, Australia
May 10, 2013
SE2013May10A.png
Annular
−0.26937143
2013 Solar Eclipse Libreville.JPG
Partial in Libreville, Gabon
November 3, 2013
SE2013Nov03H.png
Hybrid
0.32715
148
Partial Solar Eclipse April 29th 2014 (13898733668).jpg
Partial in Adelaide, Australia
April 29, 2014
SE2014Apr29A.png
Annular (non-central)
−0.99996153
Partial solar eclipse Oct 23 2014 Minneapolis 5-36pm Ruen1.png
Partial in Minneapolis, MN, USA
October 23, 2014
SE2014Oct23P.png
Partial
1.09078

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. [11]

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 June 21, 1982 and June 21, 2058
June 21April 8–9January 26November 13–14September 1–2
117119121123125
SE1982Jun21P.png
June 21, 1982
SE1986Apr09P.png
April 9, 1986
SE1990Jan26A.png
January 26, 1990
SE1993Nov13P.png
November 13, 1993
SE1997Sep02P.png
September 2, 1997
127129131133135
SE2001Jun21T.png
June 21, 2001
SE2005Apr08H.png
April 8, 2005
SE2009Jan26A.png
January 26, 2009
SE2012Nov13T.png
November 13, 2012
SE2016Sep01A.png
September 1, 2016
137139141143145
SE2020Jun21A.png
June 21, 2020
SE2024Apr08T.png
April 8, 2024
SE2028Jan26A.png
January 26, 2028
SE2031Nov14H.png
November 14, 2031
SE2035Sep02T.png
September 2, 2035
147149151153155
SE2039Jun21A.png
June 21, 2039
SE2043Apr09T.png
April 9, 2043
SE2047Jan26P.png
January 26, 2047
SE2050Nov14P.png
November 14, 2050
SE2054Sep02P.png
September 2, 2054
157
SE2058Jun21P.png
June 21, 2058

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
SE1805Jun26P.gif
June 26, 1805
(Saros 114)
SE1816May27A.gif
May 27, 1816
(Saros 115)
SE1827Apr26A.gif
April 26, 1827
(Saros 116)
SE1838Mar25T.gif
March 25, 1838
(Saros 117)
SE1849Feb23A.gif
February 23, 1849
(Saros 118)
SE1860Jan23A.png
January 23, 1860
(Saros 119)
SE1870Dec22T.png
December 22, 1870
(Saros 120)
SE1881Nov21A.gif
November 21, 1881
(Saros 121)
SE1892Oct20P.gif
October 20, 1892
(Saros 122)
SE1903Sep21T.png
September 21, 1903
(Saros 123)
SE1914Aug21T.png
August 21, 1914
(Saros 124)
SE1925Jul20A.png
July 20, 1925
(Saros 125)
SE1936Jun19T.png
June 19, 1936
(Saros 126)
SE1947May20T.png
May 20, 1947
(Saros 127)
SE1958Apr19A.png
April 19, 1958
(Saros 128)
SE1969Mar18A.png
March 18, 1969
(Saros 129)
SE1980Feb16T.png
February 16, 1980
(Saros 130)
SE1991Jan15A.png
January 15, 1991
(Saros 131)
SE2001Dec14A.png
December 14, 2001
(Saros 132)
SE2012Nov13T.png
November 13, 2012
(Saros 133)
SE2023Oct14A.png
October 14, 2023
(Saros 134)
SE2034Sep12A.png
September 12, 2034
(Saros 135)
SE2045Aug12T.png
August 12, 2045
(Saros 136)
SE2056Jul12A.png
July 12, 2056
(Saros 137)
SE2067Jun11A.png
June 11, 2067
(Saros 138)
SE2078May11T.png
May 11, 2078
(Saros 139)
SE2089Apr10A.png
April 10, 2089
(Saros 140)
SE2100Mar10A.png
March 10, 2100
(Saros 141)
SE2111Feb08T.png
February 8, 2111
(Saros 142)
SE2122Jan08A.png
January 8, 2122
(Saros 143)
SE2132Dec07A.png
December 7, 2132
(Saros 144)
SE2143Nov07T.png
November 7, 2143
(Saros 145)
SE2154Oct07T.png
October 7, 2154
(Saros 146)
Saros147 31van80 SE2165Sep05A.jpg
September 5, 2165
(Saros 147)
Saros148 30van75 SE2176Aug04T.jpg
August 4, 2176
(Saros 148)
Saros149 30van71 SE2187Jul06T.jpg
July 6, 2187
(Saros 149)
Saros150 27van71 SE2198Jun04A.jpg
June 4, 2198
(Saros 150)

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
SE1810Apr04A.gif
April 4, 1810
(Saros 126)
SE1839Mar15T.gif
March 15, 1839
(Saros 127)
SE1868Feb23A.gif
February 23, 1868
(Saros 128)
SE1897Feb01A.gif
February 1, 1897
(Saros 129)
SE1926Jan14T.png
January 14, 1926
(Saros 130)
SE1954Dec25A.png
December 25, 1954
(Saros 131)
SE1983Dec04A.png
December 4, 1983
(Saros 132)
SE2012Nov13T.png
November 13, 2012
(Saros 133)
SE2041Oct25A.png
October 25, 2041
(Saros 134)
SE2070Oct04A.png
October 4, 2070
(Saros 135)
SE2099Sep14T.png
September 14, 2099
(Saros 136)
SE2128Aug25A.png
August 25, 2128
(Saros 137)
SE2157Aug05A.png
August 5, 2157
(Saros 138)
SE2186Jul16T.png
July 16, 2186
(Saros 139)

Notes

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    <span class="mw-page-title-main">Solar eclipse of March 25, 1857</span> Total eclipse

    A total solar eclipse occurred at the Moon's ascending node of orbit between Wednesday, March 25 and Thursday, March 26, 1857, with a magnitude of 1.0534. 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 1.1 days before perigee, the Moon's apparent diameter was larger.

    <span class="mw-page-title-main">Solar eclipse of October 30, 1845</span> Hybrid (annular/total) solar eclipse October 30, 1845

    A total solar eclipse occurred at the Moon's ascending node of orbit between Thursday, October 30 and Friday, October 31, 1845, with a magnitude of 1.0005. It was a hybrid event, with only a fraction of its path as total, and longer sections at the start and end as an annular eclipse. 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 3.4 days before perigee, the Moon's apparent diameter was larger.

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