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Solar eclipse of June 2, 2095

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Solar eclipse of June 2, 2095
Map
Type of eclipse
NatureTotal
Gamma−0.6396
Magnitude1.0332
Maximum eclipse
Duration3m s
Coordinates16°42′S 37°12′E / 16.7°S 37.2°E / -16.7; 37.2
Max. width of band145 km (90 mi)
Times (UTC)
Greatest eclipse10:07:40
References
Saros129 (56 of 80)
Catalog # (SE5000)9722

A total solar eclipse will occur at the Moon's ascending node of orbit on Thursday, June 2, 2095,[1] with a magnitude of 1.0332. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent 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 after perigee (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 of South Africa, Namibia, Botswana, Zimbabwe, Mozambique, extreme southern Malawi, and Madagascar. A partial solar eclipse will also be visible for parts of Southern Africa, Central Africa, East Africa, the southern Middle East, and southern India.

Eclipse details

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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]

June 2, 2095 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 2095 June 02 at 07:37:43.5 UTC
First Umbral External Contact 2095 June 02 at 08:44:51.4 UTC
First Central Line 2095 June 02 at 08:45:36.7 UTC
First Umbral Internal Contact 2095 June 02 at 08:46:22.2 UTC
Equatorial Conjunction 2095 June 02 at 09:51:40.9 UTC
Ecliptic Conjunction 2095 June 02 at 10:00:57.6 UTC
Greatest Eclipse 2095 June 02 at 10:07:39.9 UTC
Greatest Duration 2095 June 02 at 10:08:57.6 UTC
Last Umbral Internal Contact 2095 June 02 at 11:29:10.9 UTC
Last Central Line 2095 June 02 at 11:29:53.9 UTC
Last Umbral External Contact 2095 June 02 at 11:30:36.8 UTC
Last Penumbral External Contact 2095 June 02 at 12:37:48.2 UTC
June 2, 2095 Solar Eclipse Parameters
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

Eclipse season

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This eclipse is part of an eclipse 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 a fortnight.

Eclipse season of June 2095
June 2
Ascending node (new moon)
June 17
Descending node (full moon)
Total solar eclipse
Solar Saros 129
Partial lunar eclipse
Lunar Saros 141
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Eclipses in 2095

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Solar Saros 129

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Inex

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Triad

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Solar eclipses of 2094–2098

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This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[4]

The solar eclipses on January 16, 2094 (total) and July 12, 2094 (partial) occur in the previous lunar year eclipse set, and the partial solar eclipses on April 1, 2098 and September 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

Saros 129

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This eclipse is a part of Saros 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 through March 18, 1969; hybrid eclipses from March 29, 1987 through April 20, 2023; and total eclipses from April 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 one exeligmos 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’s ascending 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

Metonic series

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The metonic 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

Tritos series

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This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic 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)

Inex series

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This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic 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)

Notes

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  1. ^ "June 2, 2095 Total Solar Eclipse". timeanddate. Retrieved 24 August 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 24 August 2024.
  3. ^ "Total Solar Eclipse of 2095 Jun 02". EclipseWise.com. Retrieved 24 August 2024.
  4. ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
  5. ^ "NASA - Catalog of Solar Eclipses of Saros 129". eclipse.gsfc.nasa.gov.

References

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