Solar eclipse of November 23, 2003

Total eclipse
Map
Gamma	−0.9638
Magnitude	1.0379
Maximum eclipse
Duration	117 s (1 min 57 s)
Coordinates	72°42′S88°24′E / 72.7°S 88.4°E /-72.7; 88.4
Max. width of band	495 km (308 mi)
Times (UTC)
Greatest eclipse	22:50:22
References
Saros	152 (12 of 70)
Catalog # (SE5000)	9516
←May 31, 2003 April 19, 2004 →

A totalsolar eclipse occurred at the Moon'sdescending node of orbit between Sunday, November 23 and Monday, November 24, 2003,^[1][2] with amagnitude of 1.0379. Asolar eclipse occurs when theMoon passes betweenEarth and theSun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon'sapparent 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 25 minutes beforeperigee (on November 23, 2003, at 23:15 UTC), the Moon's apparent diameter was near its maximum.^[3] Perigee did occur just past the greatest point of this eclipse.

For most solar eclipses the path of totality moves eastwards. In this case the path moved south and then west round Antarctica.

Totality was visible from a corridor in easternAntarctica. A partial eclipse was visible for parts ofAustralia,New Zealand,Antarctica, southernChile, and southernArgentina.

A Russian icebreaker departed fromPort Elizabeth,South Africa carrying tourists to observe the eclipse near theShackleton Ice Shelf andNovolazarevskaya Station, and then sailed toHobart,Tasmania. About 100 people from 15 countries were on board, including Iranian amateur astronomerBabak Amin Tafreshi,NASA'sGoddard Space Flight Center astrophysicistFred Espenak,Williams College professorJay Pasachoff. There are also about 200 scientists and tourists taking two commercialcharter flights to observe it over Antarctica. This was the first time humans observed a total solar eclipse from Antarctica.^[4][5][6]

Solar Eclipse of November 23, 2003
(Local Times)

Country or territory	City or place	Start of partial eclipse	Maximum eclipse	End of partial eclipse	Duration of eclipse (hr:min)	Maximum coverage
Timor-Leste	Baucau[a]	06:04:18 (sunrise)	06:09:36	06:19:38	0:15	0.34%
Timor-Leste	Dili[a]	06:07:39 (sunrise)	06:10:06	06:22:28	0:15	0.65%
Timor-Leste	Same[a]	06:06:41 (sunrise)	06:10:27	06:24:49	0:18	1.01%
Timor-Leste	Suai[a]	06:07:47 (sunrise)	06:10:54	06:27:06	0:19	1.47%
Australia	Darwin[a]	06:22:24	06:41:35	07:01:21	0:39	2.40%
Indonesia	Kupang[a]	05:13:09 (sunrise)	05:15:29	05:33:15	0:20	3.11%
Australia	Tennant Creek[a]	06:17:22	06:48:48	07:21:50	1:04	10.54%
Australia	Alice Springs[a]	06:17:07	06:54:06	07:33:18	1:16	17.97%
Australia	Brisbane[a]	07:04:13	07:31:46	08:00:38	0:56	4.34%
Australia	Eucla[a]	05:36:12	06:21:06	07:09:04	1:33	38.56%
Australia	Perth[a]	05:05:01 (sunrise)	05:39:55	06:27:57	1:23	52.53%
Australia	Adelaide[a]	07:25:03	08:10:58	09:00:12	1:35	32.88%
Australia	Lord Howe Island[a]	08:14:38	08:42:09	09:10:55	0:56	3.66%
Australia	Sydney[a]	08:02:03	08:42:18	09:25:12	1:23	15.27%
Australia	Canberra[a]	08:01:01	08:44:03	09:30:02	1:29	20.11%
Australia	Melbourne[a]	08:00:28	08:47:13	09:37:21	1:37	29.69%
Australia	Hobart[a]	08:07:31	08:57:23	09:50:49	1:43	35.02%
New Zealand	Wellington[a]	10:52:39	11:16:44	11:41:31	0:49	1.65%
New Zealand	Christchurch[a]	10:43:07	11:18:26	11:55:14	1:12	5.93%
New Zealand	Oban[a]	10:34:18	11:19:55	12:07:56	1:34	15.70%
New Zealand	Dunedin[a]	10:38:09	11:20:29	12:04:53	1:27	11.48%
New Zealand	Chatham Islands[a]	12:13:12	12:19:47	12:26:24	0:13	0.03%
Antarctica	Casey Station[a]	05:42:06	06:35:24	07:30:48	1:49	95.21%
Antarctica	Davis Station[a]	04:55:32	05:45:41	06:37:08	1:42	98.53%
Falkland Islands	Stanley	20:25:52	20:32:34	20:36:51 (sunset)	0:11	4.46%
Antarctica	Orcadas Base	20:05:46	20:33:40	20:41:50 (sunset)	0:36	40.80%
Antarctica	Marambio Base	20:05:55	20:54:05	21:40:51	1:35	59.27%
Antarctica	Carlini Base	20:09:46	20:57:06	21:42:58	1:33	54.58%
Argentina	Ushuaia	20:26:25	21:09:00	21:34:28 (sunset)	1:08	33.51%
Chile	Punta Arenas	20:30:51	21:11:45	21:36:10 (sunset)	1:05	28.23%
References:[1]

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.^[7]

This eclipse is part of aneclipse 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 afortnight.

Eclipse season of November 2003

November 9 Ascending node (full moon)	November 23 Descending node (new moon)
Total lunar eclipse Lunar Saros 126	Total solar eclipse Solar Saros 152

• A total lunar eclipse on May 16.
• An annular solar eclipse on May 31.
• A total lunar eclipse on November 9.
• A total solar eclipse on November 23.

• Preceded by:Solar eclipse of February 5, 2000
• Followed by:Solar eclipse of September 11, 2007

• Preceded by:Solar eclipse of October 12, 1996
• Followed by:Solar eclipse of January 4, 2011

• Preceded by:Lunar eclipse of November 18, 1994
• Followed by:Lunar eclipse of November 28, 2012

• Preceded by:Solar eclipse of December 24, 1992
• Followed by:Solar eclipse of October 23, 2014

• Preceded by:Solar eclipse of November 12, 1985
• Followed by:Solar eclipse of December 4, 2021

• Preceded by:Solar eclipse of December 13, 1974
• Followed by:Solar eclipse of November 3, 2032

• Preceded by:Solar eclipse of January 23, 1917
• Followed by:Solar eclipse of September 23, 2090

This eclipse is a member of asemester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternatingnodes of the Moon's orbit.^[8]

The partial solar eclipses onFebruary 5, 2000 andJuly 31, 2000 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 2000 to 2003
Ascending node				Descending node
Saros	Map	Gamma		Saros	Map	Gamma
117	July 1, 2000 Partial	−1.28214		122 Partial projection inMinneapolis, MN, USA	December 25, 2000 Partial	1.13669
127 Totality inLusaka, Zambia	June 21, 2001 Total	−0.57013		132 Partial inMinneapolis, MN, USA	December 14, 2001 Annular	0.40885
137 Partial inLos Angeles, CA, USA	June 10, 2002 Annular	0.19933		142 Totality inWoomera, South Australia	December 4, 2002 Total	−0.30204
147 Annularity inCulloden, Scotland	May 31, 2003 Annular	0.99598		152	November 23, 2003 Total	−0.96381

This eclipse is a part ofSaros series 152, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on July 26, 1805. It contains total eclipses fromNovember 2, 1967 through September 14, 2490; hybrid eclipses from September 26, 2508 through October 17, 2544; and annular eclipses from October 29, 2562 through June 16, 2941. The series ends at member 70 as a partial eclipse on August 20, 3049. Its eclipses are tabulated in three columns; every third eclipse in the same column is oneexeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of totality will be produced by member 30 at 5 minutes, 16 seconds on June 9, 2328, and the longest duration of annularity will be produced by member 53 at 5 minutes, 20 seconds on February 16, 2743. All eclipses in this series occur at the Moon’sdescending node of orbit.^[9]

Series members 1–22 occur between 1805 and 2200:
1	2	3
July 26, 1805	August 6, 1823	August 16, 1841
4	5	6
August 28, 1859	September 7, 1877	September 18, 1895
7	8	9
September 30, 1913	October 11, 1931	October 21, 1949
10	11	12
November 2, 1967	November 12, 1985	November 23, 2003
13	14	15
December 4, 2021	December 15, 2039	December 26, 2057
16	17	18
January 6, 2076	January 16, 2094	January 29, 2112
19	20	21
February 8, 2130	February 19, 2148	March 2, 2166
22
March 12, 2184

Themetonic 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 September 12, 1931 and July 1, 2011
September 11–12	June 30–July 1	April 17–19	February 4–5	November 22–23
114	116	118	120	122
September 12, 1931	June 30, 1935	April 19, 1939	February 4, 1943	November 23, 1946
124	126	128	130	132
September 12, 1950	June 30, 1954	April 19, 1958	February 5, 1962	November 23, 1965
134	136	138	140	142
September 11, 1969	June 30, 1973	April 18, 1977	February 4, 1981	November 22, 1984
144	146	148	150	152
September 11, 1988	June 30, 1992	April 17, 1996	February 5, 2000	November 23, 2003
154	156
September 11, 2007	July 1, 2011

This eclipse is a part of atritos cycle, repeating at alternating nodes every 135synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic 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 November 16, 2134 (part of Saros 164) and October 16, 2145 (part of Saros 165) are also a part of this series but are not included in the table below.

Series members between 1801 and 2069
June 6, 1807 (Saros 134)	May 5, 1818 (Saros 135)	April 3, 1829 (Saros 136)	March 4, 1840 (Saros 137)	February 1, 1851 (Saros 138)
December 31, 1861 (Saros 139)	November 30, 1872 (Saros 140)	October 30, 1883 (Saros 141)	September 29, 1894 (Saros 142)	August 30, 1905 (Saros 143)
July 30, 1916 (Saros 144)	June 29, 1927 (Saros 145)	May 29, 1938 (Saros 146)	April 28, 1949 (Saros 147)	March 27, 1960 (Saros 148)
February 25, 1971 (Saros 149)	January 25, 1982 (Saros 150)	December 24, 1992 (Saros 151)	November 23, 2003 (Saros 152)	October 23, 2014 (Saros 153)
September 21, 2025 (Saros 154)	August 21, 2036 (Saros 155)	July 22, 2047 (Saros 156)	June 21, 2058 (Saros 157)	May 20, 2069 (Saros 158)

This eclipse is a part of the long periodinex cycle, repeating at alternating nodes, every 358synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic 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
April 13, 1801 (Saros 145)	March 24, 1830 (Saros 146)	March 4, 1859 (Saros 147)
February 11, 1888 (Saros 148)	January 23, 1917 (Saros 149)	January 3, 1946 (Saros 150)
December 13, 1974 (Saros 151)	November 23, 2003 (Saros 152)	November 3, 2032 (Saros 153)
October 13, 2061 (Saros 154)	September 23, 2090 (Saros 155)	September 5, 2119 (Saros 156)
August 14, 2148 (Saros 157)	July 25, 2177 (Saros 158)

• Fred Espenak and Jay Anderson. "Total Solar Eclipse of 2003 November 23".NASA, July 2003.
• Earth visibility chart and eclipse statistics Eclipse Predictions byFred Espenak,NASA/GSFC
  • Google interactive map
  • Besselian elements
  • NASA graphics
• Google Map

Photos:

• Prof. Druckmüller's eclipse photography site. Flight over Antarctica
• Images from Antarctica by Crayford Manor House Astronomical SocietyArchived 2009-07-26 at theWayback Machine
• [1]APOD 8/5/2004, An Antarctic Total Solar Eclipse
• [2]APOD 11/27/2003, The Long Shadow of the Moon, Total solar eclipse from satellite over Antarctica

• Total solar eclipses
• 2003 in science
• 21st-century solar eclipses
• November 2003

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