| Annular eclipse | |
 Map | |
| Gamma | −0.20 |
|---|---|
| Magnitude | 0.9237 |
| Maximum eclipse | |
| Duration | 533 s (8 min 53 s) |
| Coordinates | 29°42′S163°18′E / 29.7°S 163.3°E /-29.7; 163.3 |
| Max. width of band | 294 km (183 mi) |
| Times (UTC) | |
| Greatest eclipse | 0:36:15 |
| References | |
| Saros | 144 (21 of 70) |
| Catalog # (SE5000) | 9725 |
An annularsolar eclipse will occur at the Moon'sdescending node of orbit between Wednesday, November 14 and Thursday, November 15, 2096,[1] with amagnitude of 0.9237. Asolar eclipse occurs when theMoon passes betweenEarth and theSun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon'sapparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like anannulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 1.2 days beforeapogee (on November 16, 2096, at 5:05 UTC), the Moon's apparent diameter will be smaller.[2]
The path of annularity will be visible from parts ofMalaysia,Brunei,Indonesia,Papua New Guinea, northeasternAustralia, andNew Zealand. A partial solar eclipse will also be visible for parts ofdva plus dva ravno 4
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 | 2096 November 14 at 21:30:31.9 UTC |
| First Umbral External Contact | 2096 November 14 at 22:36:23.1 UTC |
| First Central Line | 2096 November 14 at 22:39:40.3 UTC |
| First Umbral Internal Contact | 2096 November 14 at 22:42:57.9 UTC |
| First Penumbral Internal Contact | 2096 November 14 at 23:51:31.4 UTC |
| Greatest Eclipse | 2096 November 15 at 00:36:14.8 UTC |
| Ecliptic Conjunction | 2096 November 15 at 00:38:40.8 UTC |
| Equatorial Conjunction | 2096 November 15 at 00:45:04.6 UTC |
| Greatest Duration | 2096 November 15 at 00:52:33.0 UTC |
| Last Penumbral Internal Contact | 2096 November 15 at 01:20:44.7 UTC |
| Last Umbral Internal Contact | 2096 November 15 at 02:29:25.5 UTC |
| Last Central Line | 2096 November 15 at 02:32:43.9 UTC |
| Last Umbral External Contact | 2096 November 15 at 02:36:02.1 UTC |
| Last Penumbral External Contact | 2096 November 15 at 03:41:56.0 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.92371 |
| Eclipse Obscuration | 0.85323 |
| Gamma | −0.20182 |
| Sun Right Ascension | 15h25m10.4s |
| Sun Declination | -18°40'58.6" |
| Sun Semi-Diameter | 16'10.0" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 15h24m54.6s |
| Moon Declination | -18°51'10.6" |
| Moon Semi-Diameter | 14'42.9" |
| Moon Equatorial Horizontal Parallax | 0°54'00.1" |
| ΔT | 120.5 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. The first and last eclipse in this sequence is separated by onesynodic month.
| October 31 Ascending node (full moon) | November 15 Descending node (new moon) | November 29 Ascending node (full moon) |
|---|---|---|
| ||
| Penumbral lunar eclipse Lunar Saros 118 | Annular solar eclipse Solar Saros 144 | Penumbral lunar eclipse Lunar Saros 156 |
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 solar eclipses onJanuary 16, 2094 (total) andJuly 12, 2094 (partial) occur in the previous lunar year eclipse set, and the partial solar eclipses onApril 1, 2098 andSeptember 25, 2098 occur in the next lunar year eclipse set.
| Solar eclipse series sets from 2094 to 2098 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 119 | June 13, 2094 Partial | −1.4613 | 124 | December 7, 2094 Partial | 1.1547 | |
| 129 | June 2, 2095 Total | −0.6396 | 134 | November 27, 2095 Annular | 0.4903 | |
| 139 | May 22, 2096 Total | 0.1196 | 144 | November 15, 2096 Annular | −0.20 | |
| 149 | May 11, 2097 Total | 0.8516 | 154 | November 4, 2097 Annular | −0.8926 | |
| 159 | May 1, 2098 | 164 | October 24, 2098 Partial | −1.5407 | ||
This eclipse is a part ofSaros series 144, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on April 11, 1736. It contains annular eclipses from July 7, 1880 through August 27, 2565. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on May 5, 2980. 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 51 at 9 minutes, 52 seconds on December 29, 2168. All eclipses in this series occur at the Moon’sdescending node of orbit.[5]
| Series members 5–26 occur between 1801 and 2200: | ||
|---|---|---|
| 5 | 6 | 7 |
 May 25, 1808 |  June 5, 1826 |  June 16, 1844 |
| 8 | 9 | 10 |
 June 27, 1862 |  July 7, 1880 |  July 18, 1898 |
| 11 | 12 | 13 |
 July 30, 1916 |  August 10, 1934 |  August 20, 1952 |
| 14 | 15 | 16 |
 August 31, 1970 |  September 11, 1988 |  September 22, 2006 |
| 17 | 18 | 19 |
 October 2, 2024 |  October 14, 2042 |  October 24, 2060 |
| 20 | 21 | 22 |
 November 4, 2078 | November 15, 2096 |  November 27, 2114 |
| 23 | 24 | 25 |
 December 7, 2132 |  December 19, 2150 |  December 29, 2168 |
| 26 | ||
 January 9, 2187 | ||
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 June 23, 2047 and November 16, 2134 | ||||
|---|---|---|---|---|
| June 22–23 | April 10–11 | January 27–29 | November 15–16 | September 3–5 |
| 118 | 120 | 122 | 124 | 126 |
 June 23, 2047 |  April 11, 2051 |  January 27, 2055 |  November 16, 2058 |  September 3, 2062 |
| 128 | 130 | 132 | 134 | 136 |
 June 22, 2066 |  April 11, 2070 |  January 27, 2074 |  November 15, 2077 |  September 3, 2081 |
| 138 | 140 | 142 | 144 | 146 |
 June 22, 2085 |  April 10, 2089 |  January 27, 2093 | November 15, 2096 |  September 4, 2100 |
| 148 | 150 | 152 | 154 | 156 |
 June 22, 2104 |  April 11, 2108 |  January 29, 2112 |  November 16, 2115 |  September 5, 2119 |
| 158 | 160 | 162 | 164 | |
 June 23, 2123 |  November 16, 2134 | |||
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 | ||||
|---|---|---|---|---|
 March 4, 1802 (Saros 117) |  February 1, 1813 (Saros 118) |  January 1, 1824 (Saros 119) |  November 30, 1834 (Saros 120) |  October 30, 1845 (Saros 121) |
 September 29, 1856 (Saros 122) |  August 29, 1867 (Saros 123) |  July 29, 1878 (Saros 124) |  June 28, 1889 (Saros 125) |  May 28, 1900 (Saros 126) |
 April 28, 1911 (Saros 127) |  March 28, 1922 (Saros 128) |  February 24, 1933 (Saros 129) |  January 25, 1944 (Saros 130) |  December 25, 1954 (Saros 131) |
 November 23, 1965 (Saros 132) |  October 23, 1976 (Saros 133) |  September 23, 1987 (Saros 134) |  August 22, 1998 (Saros 135) |  July 22, 2009 (Saros 136) |
 June 21, 2020 (Saros 137) |  May 21, 2031 (Saros 138) |  April 20, 2042 (Saros 139) |  March 20, 2053 (Saros 140) |  February 17, 2064 (Saros 141) |
 January 16, 2075 (Saros 142) |  December 16, 2085 (Saros 143) | November 15, 2096 (Saros 144) |  October 16, 2107 (Saros 145) |  September 15, 2118 (Saros 146) |
 August 15, 2129 (Saros 147) |  July 14, 2140 (Saros 148) |  June 14, 2151 (Saros 149) |  May 14, 2162 (Saros 150) |  April 12, 2173 (Saros 151) |
 March 12, 2184 (Saros 152) |  February 10, 2195 (Saros 153) | |||
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 | ||
|---|---|---|
 June 6, 1807 (Saros 134) |  May 15, 1836 (Saros 135) |  April 25, 1865 (Saros 136) |
 April 6, 1894 (Saros 137) |  March 17, 1923 (Saros 138) |  February 25, 1952 (Saros 139) |
 February 4, 1981 (Saros 140) |  January 15, 2010 (Saros 141) |  December 26, 2038 (Saros 142) |
 December 6, 2067 (Saros 143) | November 15, 2096 (Saros 144) |  October 26, 2125 (Saros 145) |
 October 7, 2154 (Saros 146) |  September 16, 2183 (Saros 147) | |
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