| Hybrid eclipse | |
 Map | |
| Gamma | 0.3078 |
|---|---|
| Magnitude | 1.0106 |
| Maximum eclipse | |
| Duration | 68 s (1 min 8 s) |
| Coordinates | 0°36′S137°36′W / 0.6°S 137.6°W /-0.6; -137.6 |
| 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 totalsolar eclipse will occur at the Moon'sascending node of orbit on Friday, November 14, 2031,[1] with amagnitude of 1.0106. It is a hybrid event, with portions of its central path near sunrise and sunset as an annular eclipse. Asolar eclipse occurs when theMoon passes betweenEarth and theSun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon'sapparent 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. Occurring about 3.1 days beforeperigee (on November 17, 2031, at 22:00 UTC), the Moon's apparent diameter will be larger.[2]
Since most of the path of this eclipse is narrow and passes over thePacific Ocean, no land areas will witness totality. However, annularity will be visible from parts ofPanama near sunset. A partial eclipse will be visible for parts of northernOceania,Hawaii, southernNorth America,Central America, theCaribbean, and northwesternSouth America.
Animated path
| Country or territory | City or place | Start of partial eclipse | Maximum eclipse | End of partial eclipse | Duration of eclipse (hr:min) | Maximum coverage | |||
|---|---|---|---|---|---|---|---|---|---|
 United States Minor Outlying Islands | Wake Island[a] | 07:00:41 (sunrise) | 07:23:17 | 08:28:39 | 1:28 | 78.44% | |||
 Federated States of Micronesia | Palikir[a] | 06:17:26 (sunrise) | 06:24:16 | 07:12:35 | 0:55 | 26.08% | |||
 Marshall Islands | Majuro[a] | 06:32:07 | 07:27:00 | 08:28:37 | 1:57 | 42.07% | |||
| United States Minor Outlying Islands | Midway Atoll | 07:27:58 | 08:32:10 | 09:44:53 | 2:17 | 66.05% | |||
 United States | Honolulu | 08:39:10 | 09:55:27 | 11:23:23 | 2:44 | 57.79% | |||
 Kiribati | Kiritimati[a] | 08:44:40 | 10:08:22 | 11:46:07 | 3:01 | 77.84% | |||
 French Polynesia | Papeete | 09:36:04 | 10:49:11 | 12:07:03 | 2:31 | 26.08% | |||
| French Polynesia | Taioha'e | 10:00:02 | 11:38:11 | 13:17:57 | 3:18 | 67.46% | |||
| United States | Washington, D.C. | 16:43:21 | 16:52:09 | 16:55:09 (sunset) | 0:12 | 2.39% | |||
 Haiti | Port-au-Prince | 16:43:35 | 17:05:11 | 17:11:57 (sunset) | 0:28 | 20.63% | |||
 Venezuela | Maracaibo | 17:46:28 | 18:17:52 | 18:20:11 (sunset) | 0:34 | 38.53% | |||
 Bahamas | Nassau | 16:41:03 | 17:18:29 | 17:21:59 (sunset) | 0:41 | 32.23% | |||
 Clipperton Island | Clipperton Island | 12:53:36 | 14:21:59 | 15:36:18 | 2:43 | 59.97% | |||
| Venezuela | San Cristóbal | 17:47:29 | 18:24:11 | 18:26:29 (sunset) | 0:39 | 47.56% | |||
 Jamaica | Kingston | 16:42:02 | 17:26:49 | 17:30:33 (sunset) | 0:49 | 52.05% | |||
 Mexico | Mexico City | 15:20:07 | 16:30:46 | 17:32:05 | 2:12 | 39.25% | |||
 Colombia | Bogotá | 16:48:04 | 17:35:08 | 17:38:09 (sunset) | 0:50 | 63.13% | |||
 Cuba | Havana | 16:38:46 | 17:39:22 | 17:45:09 (sunset) | 1:06 | 44.16% | |||
 Belize | Belmopan | 15:33:16 | 16:41:09 | 17:19:34 (sunset) | 1:46 | 56.12% | |||
 Guatemala | Guatemala City | 15:31:06 | 16:41:47 | 17:30:22 (sunset) | 1:59 | 63.10% | |||
 Cayman Islands | George Town | 16:39:23 | 17:42:40 | 17:47:00 (sunset) | 1:08 | 57.44% | |||
 El Salvador | San Salvador | 15:32:40 | 16:43:06 | 17:26:17 (sunset) | 1:54 | 67.76% | |||
 Honduras | Tegucigalpa | 15:34:50 | 16:43:54 | 17:17:45 (sunset) | 1:43 | 68.63% | |||
 Nicaragua | Managua | 15:35:57 | 16:45:19 | 17:16:41 (sunset) | 1:41 | 76.65% | |||
 Ecuador | Galápagos Islands | 15:35:17 | 16:46:51 | 17:47:33 (sunset) | 2:12 | 78.25% | |||
 Costa Rica | San José | 15:38:28 | 16:47:02 | 17:11:01 (sunset) | 1:33 | 87.35% | |||
 Peru | Lima | 16:59:05 | 17:48:05 | 18:12:27 (sunset) | 1:13 | 25.48% | |||
 Panama | Panama City | 16:42:36 | 17:48:22 | 17:54:02 (sunset) | 1:11 | 96.39% | |||
| Peru | Piura | 16:48:52 | 17:49:27 | 18:17:25 (sunset) | 1:29 | 51.65% | |||
| Ecuador | Quito | 16:47:32 | 17:50:01 | 18:02:17 (sunset) | 1:15 | 67.02% | |||
| References:[1] | |||||||||
Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the Moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.[3]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 2031 November 14 at 18:24:26.5 UTC |
| First Umbral External Contact | 2031 November 14 at 19:25:05.7 UTC |
| First Central Line | 2031 November 14 at 19:25:17.7 UTC |
| First Umbral Internal Contact | 2031 November 14 at 19:25:29.6 UTC |
| First Penumbral Internal Contact | 2031 November 14 at 20:32:10.8 UTC |
| Equatorial Conjunction | 2031 November 14 at 21:02:09.9 UTC |
| Greatest Eclipse | 2031 November 14 at 21:07:30.7 UTC |
| Ecliptic Conjunction | 2031 November 14 at 21:10:47.9 UTC |
| Greatest Duration | 2031 November 14 at 21:11:43.9 UTC |
| Last Penumbral Internal Contact | 2031 November 14 at 21:43:00.1 UTC |
| Last Umbral Internal Contact | 2031 November 14 at 22:49:37.4 UTC |
| Last Central Line | 2031 November 14 at 22:49:46.9 UTC |
| Last Umbral External Contact | 2031 November 14 at 22:49:56.3 UTC |
| Last Penumbral External Contact | 2031 November 14 at 23:50:31.9 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 1.01059 |
| Eclipse Obscuration | 1.02128 |
| Gamma | 0.30776 |
| Sun Right Ascension | 15h19m31.2s |
| Sun Declination | -18°20'14.5" |
| Sun Semi-Diameter | 16'09.9" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 15h19m43.3s |
| Moon Declination | -18°02'21.3" |
| Moon Semi-Diameter | 16'05.0" |
| Moon Equatorial Horizontal Parallax | 0°59'01.4" |
| ΔT | 74.7 s |
This eclipse is part of aneclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by afortnight.
| October 30 Descending node (full moon) | November 14 Ascending node (new moon) |
|---|---|
 | |
| Penumbral lunar eclipse Lunar Saros 117 | Hybrid solar eclipse Solar Saros 143 |
This eclipse is a member of asemester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternatingnodes of the Moon's orbit.[4]
The partial solar eclipses onJanuary 14, 2029 andJuly 11, 2029 occur in the previous lunar year eclipse set.
| Solar eclipse series sets from 2029 to 2032 | ||||||
|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 118 | June 12, 2029 Partial | 1.29431 | 123 | December 5, 2029 Partial | −1.06090 | |
| 128 | June 1, 2030 Annular | 0.56265 | 133 | November 25, 2030 Total | −0.38669 | |
| 138 | May 21, 2031 Annular | −0.19699 | 143 | November 14, 2031 Hybrid | 0.30776 | |
| 148 | May 9, 2032 Annular | −0.93748 | 153 | November 3, 2032 Partial | 1.06431 | |
This eclipse is a part ofSaros series 143, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on March 7, 1617. It contains total eclipses from June 24, 1797 throughOctober 24, 1995; hybrid eclipses fromNovember 3, 2013 throughDecember 6, 2067; and annular eclipses fromDecember 16, 2085 through September 16, 2536. The series ends at member 72 as a partial eclipse on April 23, 2897. Its eclipses are tabulated in three columns; every third eclipse in the same column is oneexeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of totality was produced by member 16 at 3 minutes, 50 seconds onAugust 19, 1887, and the longest duration of annularity will be produced by member 51 at 4 minutes, 54 seconds on September 6, 2518. All eclipses in this series occur at the Moon’sascending node of orbit.[5]
| Series members 12–33 occur between 1801 and 2200: | ||
|---|---|---|
| 12 | 13 | 14 |
 July 6, 1815 |  July 17, 1833 |  July 28, 1851 |
| 15 | 16 | 17 |
 August 7, 1869 |  August 19, 1887 |  August 30, 1905 |
| 18 | 19 | 20 |
 September 10, 1923 |  September 21, 1941 |  October 2, 1959 |
| 21 | 22 | 23 |
 October 12, 1977 |  October 24, 1995 |  November 3, 2013 |
| 24 | 25 | 26 |
November 14, 2031 |  November 25, 2049 |  December 6, 2067 |
| 27 | 28 | 29 |
 December 16, 2085 |  December 29, 2103 |  January 8, 2122 |
| 30 | 31 | 32 |
 January 20, 2140 |  January 30, 2158 |  February 10, 2176 |
| 33 | ||
 February 21, 2194 | ||
Themetonic 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 |
| 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 | ||||
This eclipse is a part of atritos cycle, repeating at alternating nodes every 135synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.
| Series members between 1801 and 2200 | ||||
|---|---|---|---|---|
 August 28, 1802 (Saros 122) |  July 27, 1813 (Saros 123) |  June 26, 1824 (Saros 124) |  May 27, 1835 (Saros 125) |  April 25, 1846 (Saros 126) |
 March 25, 1857 (Saros 127) |  February 23, 1868 (Saros 128) |  January 22, 1879 (Saros 129) |  December 22, 1889 (Saros 130) |  November 22, 1900 (Saros 131) |
 October 22, 1911 (Saros 132) |  September 21, 1922 (Saros 133) |  August 21, 1933 (Saros 134) |  July 20, 1944 (Saros 135) |  June 20, 1955 (Saros 136) |
 May 20, 1966 (Saros 137) |  April 18, 1977 (Saros 138) |  March 18, 1988 (Saros 139) |  February 16, 1999 (Saros 140) |  January 15, 2010 (Saros 141) |
 December 14, 2020 (Saros 142) | November 14, 2031 (Saros 143) |  October 14, 2042 (Saros 144) |  September 12, 2053 (Saros 145) |  August 12, 2064 (Saros 146) |
 July 13, 2075 (Saros 147) |  June 11, 2086 (Saros 148) |  May 11, 2097 (Saros 149) |  April 11, 2108 (Saros 150) |  March 11, 2119 (Saros 151) |
 February 8, 2130 (Saros 152) |  January 8, 2141 (Saros 153) |  December 8, 2151 (Saros 154) |  November 7, 2162 (Saros 155) |  October 7, 2173 (Saros 156) |
 September 4, 2184 (Saros 157) |  August 5, 2195 (Saros 158) | |||
This eclipse is a part of the long periodinex cycle, repeating at alternating nodes, every 358synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.
| Series members between 1801 and 2200 | ||
|---|---|---|
 April 3, 1829 (Saros 136) |  March 15, 1858 (Saros 137) |  February 22, 1887 (Saros 138) |
 February 3, 1916 (Saros 139) |  January 14, 1945 (Saros 140) |  December 24, 1973 (Saros 141) |
 December 4, 2002 (Saros 142) | November 14, 2031 (Saros 143) |  October 24, 2060 (Saros 144) |
 October 4, 2089 (Saros 145) |  September 15, 2118 (Saros 146) |  August 26, 2147 (Saros 147) |
 August 4, 2176 (Saros 148) | ||
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