| Total eclipse | |
 Map | |
| Gamma | −0.6396 |
|---|---|
| Magnitude | 1.0332 |
| Maximum eclipse | |
| Duration | 3m s |
| Coordinates | 16°42′S37°12′E / 16.7°S 37.2°E /-16.7; 37.2 |
| Max. width of band | 145 km (90 mi) |
| Times (UTC) | |
| Greatest eclipse | 10:07:40 |
| References | |
| Saros | 129 (56 of 80) |
| Catalog # (SE5000) | 9722 |
A totalsolar eclipse will occur at the Moon'sascending node of orbit on Thursday, June 2, 2095,[1] with amagnitude of 1.0332. 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 days afterperigee (on May 30, 2095, at 9:45 UTC), the Moon's apparent diameter will be larger.[2]
The path of totality will be visible from parts ofSouth Africa,Namibia,Botswana,Zimbabwe,Mozambique, extreme southernMalawi, andMadagascar. A partial solar eclipse will also be visible for parts ofSouthern Africa,Central Africa,East Africa, the southernMiddle East, and southernIndia.
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 | 2095 June 2 at 07:37:43.5 UTC |
| First Umbral External Contact | 2095 June 2 at 08:44:51.4 UTC |
| First Central Line | 2095 June 2 at 08:45:36.7 UTC |
| First Umbral Internal Contact | 2095 June 2 at 08:46:22.2 UTC |
| Equatorial Conjunction | 2095 June 2 at 09:51:40.9 UTC |
| Ecliptic Conjunction | 2095 June 2 at 10:00:57.6 UTC |
| Greatest Eclipse | 2095 June 2 at 10:07:39.9 UTC |
| Greatest Duration | 2095 June 2 at 10:08:57.6 UTC |
| Last Umbral Internal Contact | 2095 June 2 at 11:29:10.9 UTC |
| Last Central Line | 2095 June 2 at 11:29:53.9 UTC |
| Last Umbral External Contact | 2095 June 2 at 11:30:36.8 UTC |
| Last Penumbral External Contact | 2095 June 2 at 12:37:48.2 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 1.03320 |
| Eclipse Obscuration | 1.06750 |
| Gamma | −0.63959 |
| Sun Right Ascension | 04h42m53.4s |
| Sun Declination | +22°14'41.8" |
| Sun Semi-Diameter | 15'46.4" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 04h43m30.2s |
| Moon Declination | +21°37'59.7" |
| Moon Semi-Diameter | 16'05.6" |
| Moon Equatorial Horizontal Parallax | 0°59'03.8" |
| ΔT | 119.2 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.
| June 2 Ascending node (new moon) | June 17 Descending node (full moon) |
|---|---|
| |
| Total solar eclipse Solar Saros 129 | Partial lunar eclipse Lunar Saros 141 |
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 129, repeating every 18 years, 11 days, and containing 80 events. The series started with a partial solar eclipse on October 3, 1103. It contains annular eclipses from May 6, 1464 throughMarch 18, 1969; hybrid eclipses fromMarch 29, 1987 throughApril 20, 2023; and total eclipses fromApril 30, 2041 through July 26, 2185. The series ends at member 80 as a partial eclipse on February 21, 2528. 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 was produced by member 34 at 5 minutes, 10 seconds on October 4, 1698, and the longest duration of totality will be produced by member 58 at 3 minutes, 43 seconds on June 25, 2131. All eclipses in this series occur at the Moon’sascending node of orbit.[5]
| Series members 40–61 occur between 1801 and 2200: | ||
|---|---|---|
| 40 | 41 | 42 |
 December 10, 1806 |  December 20, 1824 |  December 31, 1842 |
| 43 | 44 | 45 |
 January 11, 1861 |  January 22, 1879 |  February 1, 1897 |
| 46 | 47 | 48 |
 February 14, 1915 |  February 24, 1933 |  March 7, 1951 |
| 49 | 50 | 51 |
 March 18, 1969 |  March 29, 1987 |  April 8, 2005 |
| 52 | 53 | 54 |
 April 20, 2023 |  April 30, 2041 |  May 11, 2059 |
| 55 | 56 | 57 |
 May 22, 2077 | June 2, 2095 |  June 13, 2113 |
| 58 | 59 | 60 |
 June 25, 2131 |  July 5, 2149 |  July 16, 2167 |
| 61 | ||
 July 26, 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 ascending node.
| 22 eclipse events between June 1, 2076 and October 27, 2163 | ||||
|---|---|---|---|---|
| June 1–3 | March 21–22 | January 7–8 | October 26–27 | August 14–15 |
| 119 | 121 | 123 | 125 | 127 |
 June 1, 2076 |  March 21, 2080 |  January 7, 2084 |  October 26, 2087 |  August 15, 2091 |
| 129 | 131 | 133 | 135 | 137 |
June 2, 2095 |  March 21, 2099 |  January 8, 2103 |  October 26, 2106 |  August 15, 2110 |
| 139 | 141 | 143 | 145 | 147 |
 June 3, 2114 |  March 22, 2118 |  January 8, 2122 |  October 26, 2125 |  August 15, 2129 |
| 149 | 151 | 153 | 155 | 157 |
 June 3, 2133 |  March 21, 2137 |  January 8, 2141 |  October 26, 2144 |  August 14, 2148 |
| 159 | 161 | 163 | 165 | |
 June 3, 2152 |  October 27, 2163 | |||
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 1866 and 2200 | ||||
|---|---|---|---|---|
 March 16, 1866 (Saros 108) |  December 13, 1898 (Saros 111) | |||
 September 12, 1931 (Saros 114) |  August 12, 1942 (Saros 115) |  July 11, 1953 (Saros 116) |  June 10, 1964 (Saros 117) | |
 May 11, 1975 (Saros 118) |  April 9, 1986 (Saros 119) |  March 9, 1997 (Saros 120) |  February 7, 2008 (Saros 121) |  January 6, 2019 (Saros 122) |
 December 5, 2029 (Saros 123) |  November 4, 2040 (Saros 124) |  October 4, 2051 (Saros 125) |  September 3, 2062 (Saros 126) |  August 3, 2073 (Saros 127) |
 July 3, 2084 (Saros 128) | June 2, 2095 (Saros 129) |  May 3, 2106 (Saros 130) |  April 2, 2117 (Saros 131) |  March 1, 2128 (Saros 132) |
 January 30, 2139 (Saros 133) |  December 30, 2149 (Saros 134) |  November 27, 2160 (Saros 135) |  October 29, 2171 (Saros 136) |  September 27, 2182 (Saros 137) |
 August 26, 2193 (Saros 138) | ||||
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 | ||
|---|---|---|
 December 21, 1805 (Saros 119) |  November 30, 1834 (Saros 120) |  November 11, 1863 (Saros 121) |
 October 20, 1892 (Saros 122) |  October 1, 1921 (Saros 123) |  September 12, 1950 (Saros 124) |
 August 22, 1979 (Saros 125) |  August 1, 2008 (Saros 126) |  July 13, 2037 (Saros 127) |
 June 22, 2066 (Saros 128) | June 2, 2095 (Saros 129) |  May 14, 2124 (Saros 130) |
 April 23, 2153 (Saros 131) |  April 3, 2182 (Saros 132) | |
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