Solar eclipse of November 25, 2049
| Solar eclipse of November 25, 2049 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Hybrid |
| Gamma | 0.2943 |
| Magnitude | 1.0057 |
| Maximum eclipse | |
| Duration | 38 sec (0 m 38 s) |
| Coordinates | 3°48′S 95°12′E / 3.8°S 95.2°E |
| Max. width of band | 21 km (13 mi) |
| Times (UTC) | |
| Greatest eclipse | 5:33:48 |
| References | |
| Saros | 143 (25 of 72) |
| Catalog # (SE5000) | 9618 |
A total solar eclipse will occur on November 25, 2049. It is a hybrid event, with only a fraction of its path as total, and longer sections at the start and end as an annular 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.
Images
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Related eclipses
Solar eclipses 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 143
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.[1]
Series members 17-28 occur between 1901 and 2100:
| 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 |
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).
This series has 21 eclipse events, progressing from north to south between July 1, 2000 and July 1, 2076.
| July 1-2 | April 19-20 | February 5-7 | November 24-25 | September 12-13 |
|---|---|---|---|---|
| 117 | 119 | 121 | 123 | 125 |
 July 1, 2000 |
 April 19, 2004 |
 February 7, 2008 |
 November 25, 2011 |
 September 13, 2015 |
| 127 | 129 | 131 | 133 | 135 |
 July 2, 2019 |
 April 20, 2023 |
 February 6, 2027 |
 November 25, 2030 |
 September 12, 2034 |
| 137 | 139 | 141 | 143 | 145 |
 July 2, 2038 |
 April 20, 2042 |
 February 5, 2046 |
November 25, 2049 |
 September 12, 2053 |
| 147 | 149 | 151 | 153 | 155 |
 July 1, 2057 |
 April 20, 2061 |
 February 5, 2065 |
 November 24, 2068 |
 September 12, 2072 |
| 157 | ||||
 July 1, 2076 |
Notes
References
- 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 2049 November 25. |