Solar eclipse of November 23, 2003
| Solar eclipse of November 23, 2003 | |
|---|---|
| Type of eclipse | |
| Nature | Total |
| Gamma | -0.9638 |
| Magnitude | 1.0379 |
| Maximum eclipse | |
| Duration | 1m 57s |
| Coordinates | 72.7S 88.4E |
| Max. width of band | 495 km |
| Times (UTC) | |
| Greatest eclipse | 22:50:22 |
| References | |
| Saros | 152 (12 of 70) |
| Catalog # (SE5000) | 9516 |
A total solar eclipse took place on November 23, 2003 with a magnitude of 1.0379. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partially 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, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across the surface of the Earth, while a partial solar eclipse will be visible over a 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.
Contents |
Images[edit]
Related eclipses[edit]
Solar eclipses 2000-2003[edit]
Each member 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.
Note: Partial solar eclipses on February 5, 2000 and July 31, 2000 occur in the previous lunar year set.
| Ascending node | Descending node | |||
|---|---|---|---|---|
| Saros | Map | Saros | Map | |
| 117 | July 1, 2000 Partial (south) |
122 | December 25, 2000 Partial (north) |
|
| 127 Totality from Zambia |
June 21, 2001 Total |
132 Partial from Minneapolis, MN |
December 14, 2001 Annular |
|
| 137 Partial Los Angeles, CA |
June 10, 2002 Annular |
142 | December 4, 2002 Total |
|
| 147 Partial from Belfort |
May 31, 2003 Annular |
152 | November 23, 2003 Total |
|
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).
This series has 22 eclipse events between September 12, 1931 and July 1, 2011.
| September 11-12 | June 30-July 1 | April 18-19 | 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 |
Notes[edit]
References[edit]
- Fred Espenak and Jay Anderson. "Total Solar Eclipse of 2003 November 23". NASA, July 2003.
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
- Google Map
Photos:
- Prof. Druckmüller's eclipse photography site. Flight over Antarctica
- Images from Antarctica by Crayford Manor House Astronomical Society
- [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
| Wikimedia Commons has media related to: Solar eclipse of 2003 November 23 |
