Solar eclipse of December 5, 2048
| Solar eclipse of December 5, 2048 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Total |
| Gamma | -0.3973 |
| Magnitude | 1.044 |
| Maximum eclipse | |
| Duration | 208 sec (3 m 28 s) |
| Coordinates | 46°06′S 56°24′W / 46.1°S 56.4°W |
| Max. width of band | 160 km (99 mi) |
| Times (UTC) | |
| Greatest eclipse | 15:35:27 |
| References | |
| Saros | 133 (47 of 72) |
| Catalog # (SE5000) | 9616 |
A total solar eclipse will occur on December 5, 2048. 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.
Images
Animated path
Related eclipses
Solar eclipses of 2047-2050
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 lunar eclises on January 26, 2047 and July 22, 2047 occur on the previous lunar year eclipse set.
| Ascending node | Descending node | |||
|---|---|---|---|---|
| 118 | June 23, 2047 Partial |
123 | December 16, 2047 Partial | |
| 128 | June 11, 2048 Annular |
133 | December 5, 2048 Total | |
| 138 | May 31, 2049 Annular |
143 | November 25, 2049 Hybrid | |
| 148 | May 20, 2049 Hybrid |
153 | November 14, 2050 Partial | |
Saros 133
Solar Saros 133, repeating every 18 years, 11 days, contains 72 events. The series started with a partial solar eclipse on July 13, 1219. It contains annular eclipses from November 20, 1435, through January 13, 1526, with a hybrid eclipse on January 24, 1544. It has total eclipses from February 3, 1562, through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. The longest duration of totality was 6 minutes, 50 seconds on August 7, 1850.[1] The total eclipses of this saros series are getting shorter and farther south with each iteration.
| 30 | 31 | 32 |
|---|---|---|
| June 3, 1742 | June 13, 1760 |  June 24, 1778 |
| 33 | 34 | 35 |
| July 4, 1796 | July 17, 1814 | July 27, 1832 |
| 36 | 37 | 38 |
| August 7, 1850 |  August 18, 1868 |
 August 29, 1886 |
| 39 | 40 | 41 |
 September 9, 1904 |
 September 21, 1922 |
 October 1, 1940 |
| 42 | 43 | 44 |
 October 12, 1958 |
 October 23, 1976 |
 November 3, 1994 |
| 45 | 46 | 47 |
 November 13, 2012 |
 November 25, 2030 |
December 5, 2048 |
| 48 | 49 | 50 |
 December 17, 2066 |
 December 27, 2084 |
January 8, 2103 |
References
External links
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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Wikimedia Commons has media related to Solar eclipse of 2048 December 5. |
