Solar eclipse of November 23, 2003 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | −0.9638 |
Magnitude | 1.0379 |
Maximum eclipse | |
Duration | 117 sec (1 m 57 s) |
Coordinates | 72°42′S88°24′E / 72.7°S 88.4°E |
Max. width of band | 495 km (308 mi) |
Times (UTC) | |
Greatest eclipse | 22:50:22 |
References | |
Saros | 152 (12 of 70) |
Catalog # (SE5000) | 9516 |
A total solar eclipse took place on Sunday, November 23, 2003, [1] with a magnitude of 1.0379. 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 corridor in the Antarctic region. A partial eclipse was seen from the much broader path of the Moon's penumbra, including the southern tip of South America and most of Australia.
For most solar eclipses the path of totality moves eastwards. In this case the path moved south and then west round Antarctica.
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]
Partial solar eclipses on February 5, 2000 and July 31, 2000 occur in the previous lunar year set.
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 |
Solar saros 152, repeating every about 18 years and 11 days, contains 70 events. The series started with a partial solar eclipse on July 26, 1805. It has total eclipses from November 2, 1967, to September 14, 2490; hybrid eclipses from September 26, 2508, to October 17, 2544; and annular eclipses from October 29, 2562, to June 16, 2941. The series ends at member 70 as a partial eclipse on August 20, 3049. The longest total eclipse will occur on June 9, 2328, at 5 minutes and 15 seconds; the longest annular eclipse will occur on February 16, 2743, at 5 minutes and 20 seconds. [3]
Series members 7–17 occur between 1901 and 2100: | ||
---|---|---|
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 | |
January 6, 2076 | January 16, 2094 |
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.
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 |
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