Solar eclipse of December 4, 2002

Solar eclipse of December 4, 2002
Solar eclipse of December 4, 2002
	The diamond ring effect at the end of totality, taken near Woomera, South Australia
	Map
Type of eclipse
Nature	Total
Gamma	-0.302
Magnitude	1.0244
Maximum eclipse
Duration	124 sec (2 m 4 s)
Coordinates	39°30′S 59°36′E / 39.5°S 59.6°E
Max. width of band	87 km (54 mi)
Times (UTC)
Greatest eclipse	7:32:16
References
Saros	142 (22 of 72)
Catalog # (SE5000)	9514

A total solar eclipse took place on December 4, 2002, with a magnitude of 1.0244. 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. It was visible from a narrow corridor in southern Africa, the Indian Ocean and southern Australia. A partial eclipse was seen from the much broader path of the Moon's penumbra, including most of Africa and Australia. During the sunset after the eclipse many observers in Australia saw numerous and unusual forms of a green flash.^[1]

In some parts of Angola, it was the second total eclipse of the Sun within 18 months, following the Solar eclipse of June 21, 2001.

Images[]

Related eclipses[]

Eclipses of 2002[]

A penumbral lunar eclipse on May 26.
An annular solar eclipse on June 10.
A penumbral lunar eclipse on June 24.
A penumbral lunar eclipse on November 20.
A total solar eclipse on December 4.

Tzolkinex[]

Preceded: Solar eclipse of October 24, 1995

Followed: Solar eclipse of January 15, 2010

Half-Saros[]

Preceded: Lunar eclipse of November 29, 1993

Followed: Lunar eclipse of December 10, 2011

Tritos[]

Preceded: Solar eclipse of January 4, 1992

Followed: Solar eclipse of November 3, 2013

Solar Saros 142[]

Preceded: Solar eclipse of November 22, 1984

Followed: Solar eclipse of December 14, 2020

Inex[]

Preceded: Solar eclipse of December 24, 1973

Followed: Solar eclipse of November 14, 2031

Solar eclipses 2000–2003[]

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.^[2]

Note: Partial solar eclipses on February 5, 2000 and July 31, 2000 occur in the previous lunar year set.

Solar eclipse series sets from 2000–2003
Ascending node			Descending node
Saros	Map	Gamma	Saros	Map	Gamma
117	2000 July 01 Partial (south)	-1.28214	122	2000 December 25 Partial (north)	1.13669
127 Totality from Lusaka, Zambia	2001 June 21 Total	-0.57013	132 Partial from Minneapolis, MN	2001 December 14 Annular	0.40885
137 Partial from Los Angeles, CA	2002 June 10 Annular	0.19933	142 Totality from Woomera	2002 December 04 Total	-0.30204
147 Culloden, Scotland	2003 May 31 Annular	0.99598	152	2003 November 23 Total	-0.96381

Saros 142[]

It is a part of Saros cycle 142, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on April 17, 1624. It contains one hybrid eclipse on July 14, 1768, and total eclipses from July 25, 1786 through October 29, 2543. The series ends at member 72 as a partial eclipse on June 5, 2904. The longest duration of totality will be 6 minutes, 34 seconds on May 28, 2291. All eclipses in this series occurs at the Moon’s descending node.^[3]

Series members 17–41 occur between 1901 and 2359
17	18	19
October 10, 1912	October 21, 1930	November 1, 1948
20	21	22
November 12, 1966	November 22, 1984	December 4, 2002
23	24	25
December 14, 2020	December 26, 2038	January 5, 2057
26	27	28
January 16, 2075	January 27, 2093	February 8, 2111
29	30	31
February 18, 2129	March 2, 2147	March 12, 2165
32	33	34
March 23, 2183	April 4, 2201	April 15, 2219
35	36	37
April 25, 2237	May 7, 2255	May 17, 2273
38	39	40
May 28, 2291	June 9, 2309	June 20, 2327
41
June 30, 2345

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 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[]

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.

21 eclipse events, progressing from north to south between July 11, 1953 and July 11, 2029
July 10–12	April 29–30	February 15–16	December 4–5	September 21–23
116	118	120	122	124
July 11, 1953	April 30, 1957	February 15, 1961	December 4, 1964	September 22, 1968
126	128	130	132	134
July 10, 1972	April 29, 1976	February 16, 1980	December 4, 1983	September 23, 1987
136	138	140	142	144
July 11, 1991	April 29, 1995	February 16, 1999	December 4, 2002	September 22, 2006
146	148	150	152	154
July 11, 2010	April 29, 2014	February 15, 2018	December 4, 2021	September 21, 2025
156	158	160	162	164
July 11, 2029