| Partial eclipse | |
 Map | |
| Gamma | 1.0447 |
|---|---|
| Magnitude | 0.8874 |
| Maximum eclipse | |
| Coordinates | 69°30′N1°00′E / 69.5°N 1°E /69.5; 1 |
| Times (UTC) | |
| Greatest eclipse | 13:30:53 |
| References | |
| Saros | 153 (11 of 70) |
| Catalog # (SE5000) | 9620 |
A partialsolar eclipse will occur at the Moon'sascending node of orbit on Monday, November 14, 2050,[1] with amagnitude of 0.8874. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
The partial solar eclipse will be visible for parts of theNortheastern United States, easternCanada,Greenland,Europe,West Africa, andNorth Africa.
| Country or territory | City or place | Start of partial eclipse | Maximum eclipse | End of partial eclipse | Duration of eclipse (hr:min) | Maximum coverage | |||
|---|---|---|---|---|---|---|---|---|---|
 Greenland | Nuuk | 09:53:26 (sunrise) | 10:43:25 | 12:00:07 | 2:07 | 64.70% | |||
| Greenland | Ittoqqortoormiit | 09:54:36 | 11:11:17 | 12:28:14 | 2:34 | 80.64% | |||
 Iceland | Reykjavík | 11:50:32 | 13:11:36 | 14:33:07 | 2:43 | 79.11% | |||
 Faroe Islands | Tórshavn | 12:06:04 | 13:29:33 | 14:50:37 | 2:45 | 81.49% | |||
 Ireland | Dublin | 12:08:27 | 13:38:06 | 15:03:34 | 2:55 | 75.42% | |||
 Isle of Man | Douglas | 12:11:01 | 13:39:55 | 15:04:21 | 2:53 | 76.31% | |||
 Finland | Helsinki | 14:44:10 | 15:46:16 | 15:51:46 (sunset) | 1:08 | 64.40% | |||
 Portugal | Lisbon | 12:11:15 | 13:47:37 | 15:17:26 | 3:06 | 54.71% | |||
 United Kingdom | London | 12:19:36 | 13:49:14 | 15:12:43 | 2:53 | 73.53% | |||
 Norway | Oslo | 13:28:38 | 14:50:26 | 15:50:02 (sunset) | 2:21 | 79.39% | |||
 Estonia | Tallinn | 14:45:06 | 15:50:38 | 15:56:55 (sunset) | 1:12 | 67.63% | |||
 Netherlands | Amsterdam | 13:27:22 | 14:54:56 | 16:15:46 | 2:48 | 73.81% | |||
 France | Paris | 13:26:08 | 14:56:14 | 16:18:57 | 2:53 | 70.00% | |||
 Belgium | Brussels | 13:27:52 | 14:56:20 | 16:17:42 | 2:50 | 72.14% | |||
 Spain | Madrid | 13:21:45 | 14:56:40 | 16:23:16 | 3:02 | 57.86% | |||
 Sweden | Stockholm | 13:38:01 | 14:57:38 | 15:24:12 (sunset) | 1:46 | 76.99% | |||
 Denmark | Copenhagen | 13:35:36 | 14:58:44 | 16:04:47 (sunset) | 2:29 | 75.38% | |||
 Luxembourg | Luxembourg | 13:32:12 | 15:00:26 | 16:20:57 | 2:49 | 70.19% | |||
 Germany | Berlin | 13:40:40 | 15:04:31 | 16:14:37 (sunset) | 2:34 | 71.60% | |||
 Latvia | Riga | 14:48:19 | 16:06:05 | 16:12:44 (sunset) | 1:24 | 72.39% | |||
 Switzerland | Zurich | 13:39:10 | 15:06:49 | 16:25:55 | 2:47 | 66.35% | |||
 Russia | Kaliningrad | 14:47:31 | 16:07:21 | 16:37:20 (sunset) | 1:50 | 71.39% | |||
 Belarus | Minsk | 15:57:17 | 17:08:16 | 17:12:33 (sunset) | 1:15 | 65.70% | |||
 Czech Republic | Prague | 13:45:35 | 15:09:25 | 16:19:06 (sunset) | 2:34 | 68.01% | |||
 Lithuania | Vilnius | 14:53:22 | 16:10:49 | 16:18:22 (sunset) | 1:25 | 69.14% | |||
 Poland | Warsaw | 13:52:01 | 15:11:55 | 15:45:12 (sunset) | 1:53 | 67.99% | |||
 Austria | Vienna | 13:51:31 | 15:14:22 | 16:17:20 (sunset) | 2:26 | 64.37% | |||
 Croatia | Zagreb | 13:54:40 | 15:17:42 | 16:25:56 (sunset) | 2:31 | 60.70% | |||
 Hungary | Budapest | 13:56:56 | 15:18:01 | 16:08:47 (sunset) | 2:12 | 61.87% | |||
 Italy | Rome | 13:54:40 | 15:19:43 | 16:35:02 | 2:40 | 55.59% | |||
| 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.[2]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 2050 November 14 at 11:17:27.7 UTC |
| Equatorial Conjunction | 2050 November 14 at 13:11:24.1 UTC |
| Greatest Eclipse | 2050 November 14 at 13:30:52.8 UTC |
| Ecliptic Conjunction | 2050 November 14 at 13:42:38.5 UTC |
| Last Penumbral External Contact | 2050 November 14 at 15:44:21.5 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.88738 |
| Eclipse Obscuration | 0.83218 |
| Gamma | 1.04468 |
| Sun Right Ascension | 15h19m50.5s |
| Sun Declination | -18°21'19.2" |
| Sun Semi-Diameter | 16'09.8" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 15h20m29.5s |
| Moon Declination | -17°24'01.9" |
| Moon Semi-Diameter | 15'10.6" |
| Moon Equatorial Horizontal Parallax | 0°55'41.9" |
| ΔT | 84.6 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) |
|---|---|
 | |
| Total lunar eclipse Lunar Saros 127 | Partial solar eclipse Solar Saros 153 |
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.[3]
The partial solar eclipses onJanuary 26, 2047 andJuly 22, 2047 occur in the previous lunar year eclipse set.
| Solar eclipse series sets from 2047 to 2050 | ||||||
|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 118 | June 23, 2047 Partial | 1.3766 | 123 | December 16, 2047 Partial | −1.0661 | |
| 128 | June 11, 2048 Annular | 0.6468 | 133 | December 5, 2048 Total | −0.3973 | |
| 138 | May 31, 2049 Annular | −0.1187 | 143 | November 25, 2049 Hybrid | 0.2943 | |
| 148 | May 20, 2050 Hybrid | −0.8688 | 153 | November 14, 2050 Partial | 1.0447 | |
This eclipse is a part ofSaros series 153, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on July 28, 1870. It contains annular eclipses from December 17, 2104 through May 26, 2970. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on August 22, 3114. 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 annularity will be produced by member 38 at 7 minutes, 1 seconds on September 5, 2537. All eclipses in this series occur at the Moon’sascending node of orbit.[4]
| Series members 1–19 occur between 1870 and 2200: | ||
|---|---|---|
| 1 | 2 | 3 |
 July 28, 1870 |  August 7, 1888 |  August 20, 1906 |
| 4 | 5 | 6 |
 August 30, 1924 |  September 10, 1942 |  September 20, 1960 |
| 7 | 8 | 9 |
 October 2, 1978 |  October 12, 1996 |  October 23, 2014 |
| 10 | 11 | 12 |
 November 3, 2032 | November 14, 2050 |  November 24, 2068 |
| 13 | 14 | 15 |
 December 6, 2086 |  December 17, 2104 |  December 28, 2122 |
| 16 | 17 | 18 |
 January 8, 2141 |  January 19, 2159 |  January 29, 2177 |
| 19 | ||
 February 10, 2195 | ||
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.
The partial solar eclipses on December 7, 2170 (part of Saros 164) and November 7, 2181 (part of Saros 165) are also a part of this series but are not included in the table below.
| Series members between 1801 and 2105 | ||||
|---|---|---|---|---|
 September 28, 1810 (Saros 131) |  August 27, 1821 (Saros 132) |  July 27, 1832 (Saros 133) |  June 27, 1843 (Saros 134) |  May 26, 1854 (Saros 135) |
 April 25, 1865 (Saros 136) |  March 25, 1876 (Saros 137) |  February 22, 1887 (Saros 138) |  January 22, 1898 (Saros 139) |  December 23, 1908 (Saros 140) |
 November 22, 1919 (Saros 141) |  October 21, 1930 (Saros 142) |  September 21, 1941 (Saros 143) |  August 20, 1952 (Saros 144) |  July 20, 1963 (Saros 145) |
 June 20, 1974 (Saros 146) |  May 19, 1985 (Saros 147) |  April 17, 1996 (Saros 148) |  March 19, 2007 (Saros 149) |  February 15, 2018 (Saros 150) |
 January 14, 2029 (Saros 151) |  December 15, 2039 (Saros 152) | November 14, 2050 (Saros 153) |  October 13, 2061 (Saros 154) |  September 12, 2072 (Saros 155) |
 August 13, 2083 (Saros 156) |  July 12, 2094 (Saros 157) |  June 12, 2105 (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 24, 1819 (Saros 145) |  April 3, 1848 (Saros 146) |  March 15, 1877 (Saros 147) |
 February 23, 1906 (Saros 148) |  February 3, 1935 (Saros 149) |  January 14, 1964 (Saros 150) |
 December 24, 1992 (Saros 151) |  December 4, 2021 (Saros 152) | November 14, 2050 (Saros 153) |
 October 24, 2079 (Saros 154) |  October 5, 2108 (Saros 155) |  September 15, 2137 (Saros 156) |
 August 25, 2166 (Saros 157) |  August 5, 2195 (Saros 158) | |
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