Solar eclipse of June 1, 2087
| Partial eclipse | |
| Gamma | −1.4186 |
|---|---|
| Magnitude | 0.2146 |
| Maximum eclipse | |
| Coordinates | Lua error: callParserFunction: function "#coordinates" was not found. |
| Times (UTC) | |
| Greatest eclipse | 1:27:14 |
| References | |
| Saros | 158 (2 of 70) |
| Catalog # (SE5000) | 9703 |
A partial solar eclipse will occur at the Moon's descending node of orbit on Sunday, June 1, 2087,[1] with a magnitude of 0.2146. 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.
The partial solar eclipse will be visible for parts of New Zealand.
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 | 2087 June 1 at 00:27:40.4 UTC |
| Equatorial Conjunction | 2087 June 1 at 01:20:27.8 UTC |
| Greatest Eclipse | 2087 June 1 at 01:27:14.3 UTC |
| Ecliptic Conjunction | 2087 June 1 at 01:41:17.3 UTC |
| Last Penumbral External Contact | 2087 June 1 at 02:26:53.3 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.21464 |
| Eclipse Obscuration | 0.11694 |
| Gamma | −1.41856 |
| Sun Right Ascension | 04h37m04.0s |
| Sun Declination | +22°03'32.2" |
| Sun Semi-Diameter | 15'46.5" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 04h37m20.9s |
| Moon Declination | +20°37'32.1" |
| Moon Semi-Diameter | 16'34.5" |
| Moon Equatorial Horizontal Parallax | 1°00'49.8" |
| ΔT | 111.8 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.
| May 2 Descending node (new moon) |
May 17 Ascending node (full moon) |
June 1 Descending node (new moon) |
|---|---|---|
| File:SE2087May02P.png | File:Lunar eclipse chart close-2087May17.png | File:SE2087Jun01P.png |
| Partial solar eclipse Solar Saros 120 |
Total lunar eclipse Lunar Saros 132 |
Partial solar eclipse Solar Saros 158 |
Related eclipses
[edit | edit source]Eclipses in 2087
[edit | edit source]- A partial solar eclipse on May 2.
- A total lunar eclipse on May 17.
- A partial solar eclipse on June 1.
- A partial solar eclipse on October 26.
- A total lunar eclipse on November 10.
Metonic
[edit | edit source]- Preceded by: Solar eclipse of August 13, 2083
Tzolkinex
[edit | edit source]- Followed by: Solar eclipse of July 12, 2094
Half-Saros
[edit | edit source]- Followed by: Lunar eclipse of June 6, 2096
Tritos
[edit | edit source]- Preceded by: Solar eclipse of July 1, 2076
Solar Saros 158
[edit | edit source]- Preceded by: Solar eclipse of May 20, 2069
- Followed by: Solar eclipse of June 12, 2105
Inex
[edit | edit source]- Preceded by: Solar eclipse of June 21, 2058
Triad
[edit | edit source]- Preceded by: Solar eclipse of July 31, 2000
- Followed by: Solar eclipse of April 1, 2174
Solar eclipses of 2083–2087
[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 February 16, 2083 and August 13, 2083 occur in the previous lunar year eclipse set, and the partial solar eclipses on May 2, 2087 and October 26, 2087 occur in the next lunar year eclipse set.
| Solar eclipse series sets from 2083 to 2087 | ||||||
|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 118 | July 15, 2083 File:SE2083Jul15P.png Partial |
1.5465 | 123 | January 7, 2084 File:SE2084Jan07P.png Partial |
−1.0715 | |
| 128 | July 3, 2084 File:SE2084Jul03A.png Annular |
0.8208 | 133 | December 27, 2084 File:SE2084Dec27T.png Total |
−0.4094 | |
| 138 | June 22, 2085 File:SE2085Jun22A.png Annular |
0.0452 | 143 | December 16, 2085 File:SE2085Dec16A.png Annular |
0.2786 | |
| 148 | June 11, 2086 File:SE2086Jun11T.png Total |
−0.7215 | 153 | December 6, 2086 File:SE2086Dec06P.png Partial |
1.0194 | |
| 158 | June 1, 2087 File:SE2087Jun01P.png Partial |
−1.4186 | ||||
Saros 158
[edit | edit source]This eclipse is a part of Saros series 158, repeating every 18 years, 11 days, and containing 70 events. The series will start with a partial solar eclipse on May 20, 2069. It contains total eclipses from August 5, 2195 through August 13, 2808; hybrid eclipses on August 24, 2826 and September 3, 2844; and annular eclipses from September 15, 2862 through February 27, 3133. The series ends at member 70 as a partial eclipse on June 16, 3313. 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 will be produced by member 10 at 4 minutes, 43 seconds on August 28, 2231, and the longest duration of annularity will be produced by member 57 at 6 minutes, 7 seconds on January 25, 3079. All eclipses in this series occur at the Moon’s descending node of orbit.[4]
| Series members 1–8 occur between 2069 and 2200: | ||
|---|---|---|
| 1 | 2 | 3 |
| File:SE2069May20P.png May 20, 2069 |
File:SE2087Jun01P.png June 1, 2087 |
File:Saros158 03van70 SE2105Jun12P.jpg June 12, 2105 |
| 4 | 5 | 6 |
| File:Saros158 04van70 SE2123Jun23P.jpg June 23, 2123 |
File:Saros158 05van70 SE2141Jul03P.jpg July 3, 2141 |
File:Saros158 06van70 SE2159Jul15P.jpg July 15, 2159 |
| 7 | 8 | |
| File:Saros158 07van70 SE2177Jul25P.jpg July 25, 2177 |
File:Saros158 08van70 SE2195Aug05T.jpg August 5, 2195 | |
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 descending 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.
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 1801 and 2200 | ||
|---|---|---|
| File:SE1826Nov29P.gif November 29, 1826 (Saros 149) |
File:SE1855Nov09P.png November 9, 1855 (Saros 150) |
File:SE1884Oct19P.gif October 19, 1884 (Saros 151) |
| File:SE1913Sep30P.png September 30, 1913 (Saros 152) |
File:SE1942Sep10P.png September 10, 1942 (Saros 153) |
File:SE1971Aug20P.png August 20, 1971 (Saros 154) |
| File:SE2000Jul31P.png July 31, 2000 (Saros 155) |
File:SE2029Jul11P.png July 11, 2029 (Saros 156) |
File:SE2058Jun21P.png June 21, 2058 (Saros 157) |
| File:SE2087Jun01P.png June 1, 2087 (Saros 158) |
||
| File:Saros161 01van72 SE2174Apr01P.jpg April 1, 2174 (Saros 161) |
||
References
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- ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
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- ^ 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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