Solar eclipse of June 1, 2076
| Partial eclipse | |
| Gamma | −1.3897 |
|---|---|
| Magnitude | 0.2897 |
| Maximum eclipse | |
| Coordinates | Lua error: callParserFunction: function "#coordinates" was not found. |
| Times (UTC) | |
| Greatest eclipse | 17:31:22 |
| References | |
| Saros | 119 (69 of 71) |
| Catalog # (SE5000) | 9679 |
A partial solar eclipse will occur at the Moon's ascending node of orbit on Monday, June 1, 2076,[1] with a magnitude of 0.2897. 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 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 second of four solar eclipses in 2076, with the others occurring on January 6, July 1, and November 26.
The partial solar eclipse will be visible for parts of southern South America and the Antarctic Peninsula.
Eclipse details
[edit | edit source]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 June 1 at 16:11:56.2 UTC |
| Equatorial Conjunction | 2076 June 1 at 16:54:32.2 UTC |
| Ecliptic Conjunction | 2076 June 1 at 17:16:09.9 UTC |
| Greatest Eclipse | 2076 June 1 at 17:31:21.9 UTC |
| Last Penumbral External Contact | 2076 June 1 at 18:51:07.6 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.28972 |
| Eclipse Obscuration | 0.17696 |
| Gamma | −1.38966 |
| Sun Right Ascension | 04h42m27.8s |
| Sun Declination | +22°14'01.6" |
| Sun Semi-Diameter | 15'46.3" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 04h43m42.6s |
| Moon Declination | +20°58'42.6" |
| Moon Semi-Diameter | 15'11.7" |
| Moon Equatorial Horizontal Parallax | 0°55'45.9" |
| ΔT | 102.5 s |
Eclipse season
[edit | edit source]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. The first and last eclipse in this sequence is separated by one synodic month.
| June 1 Ascending node (new moon) |
June 17 Descending node (full moon) |
July 1 Ascending node (new moon) |
|---|---|---|
| File:SE2076Jun01P.png | File:Lunar eclipse chart close-2076Jun17.png | File:SE2076Jul01P.png |
| Partial solar eclipse Solar Saros 119 |
Total lunar eclipse Lunar Saros 131 |
Partial solar eclipse Solar Saros 157 |
Related eclipses
[edit | edit source]Eclipses in 2076
[edit | edit source]- A total solar eclipse on January 6.
- A partial solar eclipse on June 1.
- A total lunar eclipse on June 17.
- A partial solar eclipse on July 1.
- A partial solar eclipse on November 26.
- A total lunar eclipse on December 10.
Metonic
[edit | edit source]- Followed by: Solar eclipse of March 21, 2080
Tzolkinex
[edit | edit source]- Preceded by: Solar eclipse of April 21, 2069
- Followed by: Solar eclipse of July 15, 2083
Half-Saros
[edit | edit source]- Preceded by: Lunar eclipse of May 28, 2067
- Followed by: Lunar eclipse of June 8, 2085
Tritos
[edit | edit source]- Preceded by: Solar eclipse of July 3, 2065
- Followed by: Solar eclipse of May 2, 2087
Solar Saros 119
[edit | edit source]- Preceded by: Solar eclipse of May 22, 2058
- Followed by: Solar eclipse of June 13, 2094
Inex
[edit | edit source]- Preceded by: Solar eclipse of June 23, 2047
- Followed by: Solar eclipse of May 14, 2105
Triad
[edit | edit source]- Followed by: Solar eclipse of April 3, 2163
Solar eclipses of 2076–2079
[edit | edit source]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.[3]
The partial solar eclipses on January 6, 2076 and July 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 File:SE2076Jun01P.png Partial |
−1.3897 | 124 | November 26, 2076 File:SE2076Nov26P.png Partial |
1.1401 | |
| 129 | May 22, 2077 File:SE2077May22T.png Total |
−0.5725 | 134 | November 15, 2077 File:SE2077Nov15A.png Annular |
0.4705 | |
| 139 | May 11, 2078 File:SE2078May11T.png Total |
0.1838 | 144 | November 4, 2078 File:SE2078Nov04A.png Annular |
−0.2285 | |
| 149 | May 1, 2079 File:SE2079May01T.png Total |
0.9081 | 154 | October 24, 2079 File:SE2079Oct24A.png Annular |
−0.9243 | |
Saros 119
[edit | edit source]This eclipse is a part of Saros series 119, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on May 15, 850 AD. It contains total eclipses on August 9, 994 AD and August 20, 1012; a hybrid eclipse on August 31, 1030; and annular eclipses from September 10, 1048 through March 18, 1950. The series ends at member 71 as a partial eclipse on June 24, 2112. 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 totality was produced by member 10 at 32 seconds on August 20, 1012, and the longest duration of annularity was produced by member 44 at 7 minutes, 37 seconds on September 1, 1625. All eclipses in this series occur at the Moon’s ascending node of orbit.[4]
| Series members 54–71 occur between 1801 and 2112: | ||
|---|---|---|
| 54 | 55 | 56 |
| File:SE1805Dec21A.gif December 21, 1805 |
File:SE1824Jan01A.gif January 1, 1824 |
File:SE1842Jan11A.gif January 11, 1842 |
| 57 | 58 | 59 |
| File:SE1860Jan23A.gif January 23, 1860 |
File:SE1878Feb02A.gif February 2, 1878 |
File:Saros119 59van71 SE1896Feb13A.jpg February 13, 1896 |
| 60 | 61 | 62 |
| File:SE1914Feb25A.png February 25, 1914 |
File:SE1932Mar07A.png March 7, 1932 |
File:SE1950Mar18A.png March 18, 1950 |
| 63 | 64 | 65 |
| File:SE1968Mar28P.png March 28, 1968 |
File:SE1986Apr09P.png April 9, 1986 |
File:SE2004Apr19P.png April 19, 2004 |
| 66 | 67 | 68 |
| File:SE2022Apr30P.png April 30, 2022 |
File:SE2040May11P.png May 11, 2040 |
File:SE2058May22P.png May 22, 2058 |
| 69 | 70 | 71 |
| File:SE2076Jun01P.png June 1, 2076 |
File:SE2094Jun13P.png June 13, 2094 |
File:Saros119 71van71 SE2112Jun24P.jpg June 24, 2112 |
Metonic series
[edit | edit source]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.
Tritos series
[edit | edit source]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 2054 and 2200 | ||||
|---|---|---|---|---|
| File:SE2054Aug03P.png August 3, 2054 (Saros 117) |
File:SE2065Jul03P.png July 3, 2065 (Saros 118) |
File:SE2076Jun01P.png June 1, 2076 (Saros 119) |
File:SE2087May02P.png May 2, 2087 (Saros 120) |
File:SE2098Apr01P.png April 1, 2098 (Saros 121) |
| File:SE2109Mar01P.png March 1, 2109 (Saros 122) |
File:Saros123 59van70 SE2120Jan30P.jpg January 30, 2120 (Saros 123) |
File:Saros124 61van73 SE2130Dec30P.jpg December 30, 2130 (Saros 124) |
File:Saros125 61van73 SE2141Nov28P.jpg November 28, 2141 (Saros 125) |
File:Saros126 55van72 SE2152Oct28P.jpg October 28, 2152 (Saros 126) |
| File:Saros127 66van82 SE2163Sep28P.jpg September 28, 2163 (Saros 127) |
File:Saros128 67van73 SE2174Aug27P.jpg August 27, 2174 (Saros 128) |
File:Saros129 61van80 SE2185Jul26T.jpg July 26, 2185 (Saros 129) |
File:SE2196Jun26T.png June 26, 2196 (Saros 130) | |
Inex series
[edit | edit source]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 1844 and 2200 | ||
|---|---|---|
| File:SE1844Nov10P.png November 10, 1844 (Saros 111) |
||
| File:SE1931Sep12P.png September 12, 1931 (Saros 114) |
||
| File:SE2018Jul13P.png July 13, 2018 (Saros 117) |
File:SE2047Jun23P.png June 23, 2047 (Saros 118) |
File:SE2076Jun01P.png June 1, 2076 (Saros 119) |
| File:Saros120 66van71 SE2105May14P.jpg May 14, 2105 (Saros 120) |
File:Saros121 67van71 SE2134Apr24P.jpg April 24, 2134 (Saros 121) |
File:Saros122 66van70 SE2163Apr03P.jpg April 3, 2163 (Saros 122) |
| File:Saros123 63van70 SE2192Mar13P.jpg March 13, 2192 (Saros 123) |
||
References
[edit | edit source]- ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
- ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
- ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
- ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
External links
[edit | edit source]- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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