Solar eclipse of November 3, 2013

Solar eclipse of November 3, 2013
Solar eclipse of November 3, 2013
	Partial from Libreville, Gabon
	Map
Type of eclipse
Nature	Hybrid
Gamma	0.3272
Magnitude	1.0159
Maximum eclipse
Duration	100 s (1 min 40 s)
Coordinates	3°30′N 11°42′W / 3.5°N 11.7°W
Max. width of band	58 km (36 mi)
Times (UTC)
(P1) Partial begin	10:04:34
(U1) Total begin	11:05:17
Greatest eclipse	12:47:36
(U4) Total end	14:27:42
(P4) Partial end	15:28:21
References
Saros	143 (23 of 72)
Catalog # (SE5000)	9538

A total solar eclipse occurred at the Moon's ascending node on 3 November 2013.^[1]^[2]^[3] It was a hybrid eclipse of the Sun with a magnitude of 1.0159, with a small portion over the western Atlantic Ocean at sunrise as an annular eclipse, and the rest of the path as a narrow total solar 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 hybrid solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's in sunrise and sunset, but at Greatest Eclipse the Moon's apparent diameter is larger than the Sun's.

In this particular case the eclipse path starts out as annular and ends as total.

It was the 23rd eclipse of the 143rd Saros cycle, which began with a partial eclipse on March 7, 1617, and will conclude with a partial eclipse on April 23, 2897.

Viewing[edit]

Totality was visible from the northern Atlantic Ocean (east of Florida) to Africa (Gabon (landfall), R. Congo, DR Congo, Uganda, South Sudan, Kenya, Ethiopia, Somalia), with a maximum duration of totality of 1 minute and 39 seconds, visible from the Atlantic Ocean south of Ivory Coast and Ghana.^[4]

Places with partial darkening were the Eastern coast of North America, southern Greenland, Bermuda, the Caribbean islands, Costa Rica, Panama, Northern South America, almost all the African continent, the Iberian Peninsula, Italy, Greece, Malta, Southern Russia, the Caucasus, Turkey and the Middle East.

This solar eclipse happened simultaneously with the 2013 Abu Dhabi Grand Prix, and it was possible to observe a partial solar eclipse in Abu Dhabi before the sunset while the F1 race took place, as shown briefly during its broadcast.^[5]

From space[edit]

Simulated shadow path

Photo gallery[edit]

Wind angle view in Agüimes, Las Palmas during the eclipse

An eclipse monument in Pakwach, Uganda
From Ottawa, Canada at sunrise, 11:24 UTC
From Liberty State Park, New Jersey at sunrise, 11:37 UTC
From Egg Harbor Township, New Jersey at sunrise, 11:40 UTC
From Melbourne, Florida at sunrise, 11:45 UTC
Partial from Las Palmas, Canary Islands, 12:01 UTC
Partial from Tétouan, Morocco, 12:27 UTC
Partial from Bayeux, Brazil, 12:35 UTC
Partial from Lake Turkana, Kenya, 13:54 UTC
From Triolet, Mauritius at sunset, 14:18 UTC
From Bunia, DR Congo at greatest eclipse, 14:22 UTC
From Addis Ababa, Ethiopia at sunset, 14:50 UTC

Related eclipses[edit]

Eclipses of 2013[edit]

A partial lunar eclipse on April 25.
An annular solar eclipse on May 10.
A penumbral lunar eclipse on May 25.
A penumbral lunar eclipse on October 18.
A hybrid solar eclipse on November 3.

Solar eclipses 2011–2014[edit]

This eclipse is a member of the 2011–2014 solar eclipse 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.^[6]^{[Note 1]}

Solar eclipse series sets from 2011 to 2014
Saros	Map	Gamma	Saros	Map	Gamma
Descending node			Ascending node
118 Partial from Tromsø, Norway	2011 June 01 Partial (north)	1.21300	123 Hinode XRT footage	2011 November 25 Partial (south)	−1.05359
128 Middlegate, Nevada	2012 May 20 Annular	0.48279	133 Cairns, Australia	2012 November 13 Total	−0.37189
138 Churchills Head, Australia	2013 May 10 Annular	−0.26937	143 Partial from Libreville, Gabon	2013 November 03 Hybrid	0.32715
148 Partial from Adelaide, Australia	2014 April 29 Annular (non-central)	−0.99996	153 Partial from Minneapolis	2014 October 23 Partial (north)	1.09078

Saros 143[edit]

It is a part of Saros cycle 143, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on March 7, 1617 and total event from June 24, 1797 through October 24, 1995. It has hybrid eclipses from November 3, 2013 through December 6, 2067, and annular eclipses from December 16, 2085 through September 16, 2536. The series ends at member 72 as a partial eclipse on April 23, 2873. The longest duration of totality was 3 minutes, 50 seconds on August 19, 1887. All eclipses in this series occurs at the Moon’s ascending node.

Series members 17–28 occur between 1741 and 2100
8	9	10
May 23, 1743	June 3, 1761	June 14, 1779
11	12	13
June 24, 1797	July 6, 1815	July 17, 1833
14	15	16
July 28, 1851	August 7, 1869	August 19, 1887
17	18	19
August 30, 1905	September 10, 1923	September 21, 1941
20	21	22
October 2, 1959	October 12, 1977	October 24, 1995
23	24	25
November 3, 2013	November 14, 2031	November 25, 2049
26	27	28
December 6, 2067	December 16, 2085

Inex series[edit]

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.

Inex series members between 1901 and 2100:
January 3, 1927 (Saros 140)	December 14, 1955 (Saros 141)	November 22, 1984 (Saros 142)
November 3, 2013 (Saros 143)	October 14, 2042 (Saros 144)	September 23, 2071 (Saros 145)
September 4, 2100 (Saros 146)

Tritos series[edit]

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 1901 and 2100
September 9, 1904 (Saros 133)	August 10, 1915 (Saros 134)	July 9, 1926 (Saros 135)
June 8, 1937 (Saros 136)	May 9, 1948 (Saros 137)	April 8, 1959 (Saros 138)
March 7, 1970 (Saros 139)	February 4, 1981 (Saros 140)	January 4, 1992 (Saros 141)
December 4, 2002 (Saros 142)	November 3, 2013 (Saros 143)	October 2, 2024 (Saros 144)
September 2, 2035 (Saros 145)	August 2, 2046 (Saros 146)	July 1, 2057 (Saros 147)
May 31, 2068 (Saros 148)	May 1, 2079 (Saros 149)	March 31, 2090 (Saros 150)

Metonic series[edit]

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, progressing from south to north between June 10, 1964, and August 21, 2036
June 10–11	March 27–29	January 15–16	November 3	August 21–22
117	119	121	123	125
June 10, 1964	March 28, 1968	January 16, 1972	November 3, 1975	August 22, 1979
127	129	131	133	135
June 11, 1983	March 29, 1987	January 15, 1991	November 3, 1994	August 22, 1998
137	139	141	143	145
June 10, 2002	March 29, 2006	January 15, 2010	November 3, 2013	August 21, 2017
147	149	151	153	155
June 10, 2021	March 29, 2025	January 14, 2029	November 3, 2032	August 21, 2036