| Partial eclipse | |
 Map | |
| Gamma | 1.1401 |
|---|---|
| Magnitude | 0.7315 |
| Maximum eclipse | |
| Coordinates | 63°42′N40°06′E / 63.7°N 40.1°E /63.7; 40.1 |
| Times (UTC) | |
| Greatest eclipse | 11:43:01 |
| References | |
| Saros | 124 (58 of 73) |
| Catalog # (SE5000) | 9680 |
A partialsolar eclipse will occur at the Moon'sdescending node of orbit on Thursday, November 26, 2076,[1] with amagnitude of 0.7315. 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.
This will be the last of four solar eclipses in 2076, with the others occurring onJanuary 6,June 1, andJuly 1.
The partial solar eclipse will be visible for parts ofGreenland, northernCanada,Alaska, and theRussian Far East.
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 | 2076 November 26 at 09:46:54.5 UTC |
| Equatorial Conjunction | 2076 November 26 at 11:07:03.6 UTC |
| Ecliptic Conjunction | 2076 November 26 at 11:30:38.9 UTC |
| Greatest Eclipse | 2076 November 26 at 11:43:00.9 UTC |
| Last Penumbral External Contact | 2076 November 26 at 13:39:16.9 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.73147 |
| Eclipse Obscuration | 0.65559 |
| Gamma | 1.14014 |
| Sun Right Ascension | 16h12m39.7s |
| Sun Declination | -21°08'26.9" |
| Sun Semi-Diameter | 16'12.3" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 16h13m56.6s |
| Moon Declination | -20°05'16.9" |
| Moon Semi-Diameter | 15'44.2" |
| Moon Equatorial Horizontal Parallax | 0°57'45.3" |
| ΔT | 102.9 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.
| November 26 Descending node (new moon) | December 10 Ascending node (full moon) |
|---|---|
|  |
| Partial solar eclipse Solar Saros 124 | Total lunar eclipse Lunar Saros 136 |
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 6, 2076 andJuly 1, 2076 occur in the previous lunar year eclipse set.
| Solar eclipse series sets from 2076 to 2079 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 119 | June 1, 2076 Partial | −1.3897 | 124 | November 26, 2076 Partial | 1.1401 | |
| 129 | May 22, 2077 Total | −0.5725 | 134 | November 15, 2077 Annular | 0.4705 | |
| 139 | May 11, 2078 Total | 0.1838 | 144 | November 4, 2078 Annular | −0.2285 | |
| 149 | May 1, 2079 Total | 0.9081 | 154 | October 24, 2079 Annular | −0.9243 | |
This eclipse is a part ofSaros series 124, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on March 6, 1049. It contains total eclipses from June 12, 1211 throughSeptember 22, 1968, and a hybrid eclipse onOctober 3, 1986. There are no annular eclipses in this set. The series ends at member 73 as a partial eclipse on May 11, 2347. 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 39 at 5 minutes, 46 seconds on May 3, 1734. All eclipses in this series occur at the Moon’sdescending node of orbit.[4]
| Series members 43–64 occur between 1801 and 2200: | ||
|---|---|---|
| 43 | 44 | 45 |
 June 16, 1806 |  June 26, 1824 |  July 8, 1842 |
| 46 | 47 | 48 |
 July 18, 1860 |  July 29, 1878 |  August 9, 1896 |
| 49 | 50 | 51 |
 August 21, 1914 |  August 31, 1932 |  September 12, 1950 |
| 52 | 53 | 54 |
 September 22, 1968 |  October 3, 1986 |  October 14, 2004 |
| 55 | 56 | 57 |
 October 25, 2022 |  November 4, 2040 |  November 16, 2058 |
| 58 | 59 | 60 |
November 26, 2076 |  December 7, 2094 |  December 19, 2112 |
| 61 | 62 | 63 |
 December 30, 2130 |  January 9, 2149 |  January 21, 2167 |
| 64 | ||
 January 31, 2185 | ||
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 descending node.
| 22 eclipse events between July 3, 2065 and November 26, 2152 | ||||
|---|---|---|---|---|
| July 3–4 | April 21–23 | February 7–8 | November 26–27 | September 13–15 |
| 118 | 120 | 122 | 124 | 126 |
 July 3, 2065 |  April 21, 2069 |  February 7, 2073 | November 26, 2076 |  September 13, 2080 |
| 128 | 130 | 132 | 134 | 136 |
 July 3, 2084 |  April 21, 2088 |  February 7, 2092 |  November 27, 2095 |  September 14, 2099 |
| 138 | 140 | 142 | 144 | 146 |
 July 4, 2103 |  April 23, 2107 |  February 8, 2111 |  November 27, 2114 |  September 15, 2118 |
| 148 | 150 | 152 | 154 | 156 |
 July 4, 2122 |  April 22, 2126 |  February 8, 2130 |  November 26, 2133 |  September 15, 2137 |
| 158 | 160 | 162 | 164 | |
 July 3, 2141 |  November 26, 2152 | |||
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 onApril 8, 1902 (part of Saros 108) andJanuary 5, 1935 (part of Saros 111) are also a part of this series but are not included in the table below.
| Series members between 2000 and 2200 | ||||
|---|---|---|---|---|
 July 1, 2000 (Saros 117) |  June 1, 2011 (Saros 118) |  April 30, 2022 (Saros 119) |  March 30, 2033 (Saros 120) |  February 28, 2044 (Saros 121) |
 January 27, 2055 (Saros 122) |  December 27, 2065 (Saros 123) | November 26, 2076 (Saros 124) |  October 26, 2087 (Saros 125) |  September 25, 2098 (Saros 126) |
 August 26, 2109 (Saros 127) |  July 25, 2120 (Saros 128) |  June 25, 2131 (Saros 129) |  May 25, 2142 (Saros 130) |  April 23, 2153 (Saros 131) |
 March 23, 2164 (Saros 132) |  February 21, 2175 (Saros 133) |  January 20, 2186 (Saros 134) |  December 19, 2196 (Saros 135) | |
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 | ||
|---|---|---|
 May 27, 1816 (Saros 115) |  May 6, 1845 (Saros 116) |  April 16, 1874 (Saros 117) |
 March 29, 1903 (Saros 118) |  March 7, 1932 (Saros 119) |  February 15, 1961 (Saros 120) |
 January 26, 1990 (Saros 121) |  January 6, 2019 (Saros 122) |  December 16, 2047 (Saros 123) |
November 26, 2076 (Saros 124) |  November 6, 2105 (Saros 125) |  October 17, 2134 (Saros 126) |
 September 28, 2163 (Saros 127) |  September 6, 2192 (Saros 128) | |
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