Solar eclipse of June 1, 2087
{{short description|Future partial solar eclipse}}
{{Infobox solar eclipse|2087Jun01
| previous = Solar eclipse of May 2, 2087
| next = Solar eclipse of October 26, 2087
}}
A partial solar eclipse will occur at the Moon's descending node of orbit on Sunday, June 1, 2087,{{cite web|title=June 1, 2087 Partial Solar Eclipse|url=https://www.timeanddate.com/eclipse/solar/2087-june-1|publisher=timeanddate|access-date=24 August 2024}} 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
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.{{cite web|title=Partial Solar Eclipse of 2087 Jun 01|url=https://eclipsewise.com/solar/SEprime/2001-2100/SE2087Jun01Pprime.html|publisher=EclipseWise.com|access-date=24 August 2024}}
| class="wikitable" align="{{{align|left}}}" style="margin:{{#ifeq:{{{align}}}|left|0 0 0.5em 1em|0 1em 0.5em 0}}"
|+June 1, 2087 Solar Eclipse Times ! 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 |
| class="wikitable" align="{{{align|right}}}" style="margin:{{#ifeq:{{{align}}}|right|0 0 0.5em 1em|0 1em 0.5em 0}}"
|+June 1, 2087 Solar Eclipse Parameters ! 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 |
{{clear}}
Eclipse season
{{See also|Eclipse cycle}}
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.
| class="wikitable"
|+ Eclipse season of May–June 2087 ! May 2 | ||
| 200px | 200px | 200px |
| align=center
| Partial solar eclipse | Total lunar eclipse Lunar Saros 132 | Partial solar eclipse Solar Saros 158 |
Related eclipses
= Eclipses in 2087 =
- 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 =
- Preceded by: Solar eclipse of August 13, 2083
= Tzolkinex =
- Followed by: Solar eclipse of July 12, 2094
= Half-Saros =
- Followed by: Lunar eclipse of June 6, 2096
= Tritos =
- Preceded by: Solar eclipse of July 1, 2076
= Solar Saros 158 =
- Preceded by: Solar eclipse of May 20, 2069
- Followed by: Solar eclipse of June 12, 2105
= Inex =
- Preceded by: Solar eclipse of June 21, 2058
= Triad =
- Preceded by: Solar eclipse of July 31, 2000
- Followed by: Solar eclipse of April 1, 2174
= Solar eclipses of 2083–2087 =
{{Solar eclipse set 2083–2087}}
= Saros 158 =
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.{{Cite web|url=https://eclipse.gsfc.nasa.gov/SEsaros/SEsaros158.html|title=NASA - Catalog of Solar Eclipses of Saros 158|website=eclipse.gsfc.nasa.gov}}
| class="wikitable mw-collapsible mw-collapsed"
!colspan=3|Series members 1–8 occur between 2069 and 2200: |
| 1
!2 !3 |
|---|
| style="text-align:center;"
|150px |150px |
| 4
!5 !6 |
| style="text-align:center;"
|150px |150px |150px |
| 7
!8 |
| style="text-align:center;"
|150px |150px |
= Metonic series =
{{Solar Metonic series 2011–2098}}
= Tritos series =
{{Solar Tritos series 2000 February 5}}
= Inex series =
{{Solar Inex series 2000 July 31}}
References
{{reflist}}
External links
{{Solar eclipse NASA reference|2051/SE2087Jun01P|20870601}}
{{Solar eclipses}}