| Solar eclipse of November 14, 2031 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Hybrid |
| Gamma | 0.3078 |
| Magnitude | 1.0106 |
| Maximum eclipse | |
| Duration | 68 s (1 min 8 s) |
| Coordinates | 0°36′S 137°36′W / 0.6°S 137.6°W |
| Max. width of band | 38 km (24 mi) |
| Times (UTC) | |
| Greatest eclipse | 21:07:31 |
| References | |
| Saros | 143 (24 of 72) |
| Catalog # (SE5000) | 9578 |
A total solar eclipse will occur on Friday, November 14, 2031. It is a hybrid event, with portions of its central path near sunrise and sunset 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. 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.
Animated path
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.[1]
Note: Partial solar eclipses on January 14, 2029 and July 11, 2029 occur on the previous lunar year eclipse set.
| Solar eclipse series sets from 2029 to 2032 | ||||
|---|---|---|---|---|
| Descending node | Ascending node | |||
| 118 | June 12, 2029 Partial |
123 | December 5, 2029 Partial | |
| 128 | June 1, 2030 Annular |
133 | November 25, 2030 Total | |
| 138 | May 21, 2031 Annular |
143 | November 14, 2031 Hybrid | |
| 148 | May 9, 2032 Annular |
153 | November 3, 2032 Partial | |
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. All eclipses in this series occurs at the Moon’s ascending node.
| Series members 17–28 occur between 1741 and 2100 | ||
|---|---|---|
| 8 | 9 | 10 |
 May 23, 1743 |
 June 3, 1761 |
 June 14, 1779 |
| 11 | 12 | 13 |
 June 24, 1797 |
 July 6, 1815 |
 July 17, 1833 |
| 14 | 15 | 16 |
 July 28, 1851 |
 August 7, 1869 |
 August 19, 1887 |
| 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 | |
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 ascending node.
| 21 eclipse events between June 21, 1982, and June 21, 2058 | ||||
|---|---|---|---|---|
| June 21 | April 8–9 | January 26 | November 13–14 | September 1–2 |
| 107 | 109 | 111 | 113 | 115 |
| June 21, 1963 | April 9, 1967 | January 26, 1971 | November 14, 1974 | September 2, 1978 |
| 117 | 119 | 121 | 123 | 125 |
 June 21, 1982 |
 April 9, 1986 |
 January 26, 1990 |
 November 13, 1993 |
 September 2, 1997 |
| 127 | 129 | 131 | 133 | 135 |
 June 21, 2001 |
 April 8, 2005 |
 January 26, 2009 |
 November 13, 2012 |
 September 1, 2016 |
| 137 | 139 | 141 | 143 | 145 |
 June 21, 2020 |
 April 8, 2024 |
 January 26, 2028 |
November 14, 2031 |
 September 2, 2035 |
| 147 | 149 | 151 | 153 | 155 |
 June 21, 2039 |
 April 9, 2043 |
 January 26, 2047 |
 November 14, 2050 |
 September 2, 2054 |
| 157 | ||||
 June 21, 2058 | ||||
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