Solar eclipse of June 2, 2095
Template:Short description Script error: No such module "Solar eclipse". 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
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 |
Eclipse season
Script error: No such module "Labelled list hatnote". 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.
| June 2 Ascending node (new moon) |
June 17 Descending node (full moon) |
|---|---|
| File:SE2095Jun02T.png | |
| Total solar eclipse Solar Saros 129 |
Partial lunar eclipse Lunar Saros 141 |
Related eclipses
Eclipses in 2095
- A total solar eclipse on June 2.
- A partial lunar eclipse on June 17.
- An annular solar eclipse on November 27.
- A partial lunar eclipse on December 11.
Metonic
- Preceded by: Solar eclipse of August 15, 2091
- Followed by: Solar eclipse of March 21, 2099
Tzolkinex
- Preceded by: Solar eclipse of April 21, 2088
- Followed by: Solar eclipse of July 15, 2102
Half-Saros
- Preceded by: Lunar eclipse of May 28, 2086
- Followed by: Lunar eclipse of June 8, 2104
Tritos
- Preceded by: Solar eclipse of July 3, 2084
- Followed by: Solar eclipse of May 3, 2106
Solar Saros 129
- Preceded by: Solar eclipse of May 22, 2077
- Followed by: Solar eclipse of June 13, 2113
Inex
- Preceded by: Solar eclipse of June 22, 2066
- Followed by: Solar eclipse of May 14, 2124
Triad
- Preceded by: Solar eclipse of August 1, 2008
- Followed by: Solar eclipse of April 3, 2182
Solar eclipses of 2094–2098
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 File:SE2094Jun13P.png Partial |
−1.4613 | 124 | December 7, 2094 File:SE2094Dec07P.png Partial |
1.1547 | |
| 129 | June 2, 2095 File:SE2095Jun02T.png Total |
−0.6396 | 134 | November 27, 2095 File:SE2095Nov27A.png Annular |
0.4903 | |
| 139 | May 22, 2096 File:SE2096May22T.png Total |
0.1196 | 144 | November 15, 2096 File:SE2096Nov15A.png Annular |
−0.20 | |
| 149 | May 11, 2097 File:SE2097May11T.png Total |
0.8516 | 154 | November 4, 2097 File:SE2097Nov04A.png Annular |
−0.8926 | |
| 159 | May 1, 2098 | 164 | October 24, 2098 File:SE2098Oct24P.png Partial |
−1.5407 | ||
Saros 129
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]
Metonic series
Template:Solar Metonic series 2076–2163
Tritos series
Template:Solar Tritos series 2008 February 7
Inex series
Template:Solar Inex series 2008 August 1
Notes
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References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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