Solar eclipse of June 11, 2067
{{short description|Future annular solar eclipse}}
{{Infobox solar eclipse|2067Jun11
| previous = Solar eclipse of December 17, 2066
| next = Solar eclipse of December 6, 2067
}}
An annular solar eclipse will occur at the Moon's descending node of orbit on Saturday, June 11, 2067,{{cite web|title=June 11, 2067 Annular Solar Eclipse|url=https://www.timeanddate.com/eclipse/solar/2067-june-11|publisher=timeanddate|access-date=19 August 2024}} with a magnitude of 0.967. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 4.3 days before apogee (on June 16, 2067, at 4:05 UTC), the Moon's apparent diameter will be smaller.{{cite web|title=Moon Distances for London, United Kingdom, England|url=https://www.timeanddate.com/astronomy/moon/distance.html?year=2067&n=136|publisher=timeanddate|access-date=19 August 2024}}
The path of annularity will be visible from parts of Kiribati, Ecuador, northern Peru, extreme southern Colombia, and extreme western Brazil. A partial solar eclipse will also be visible for parts of Oceania, Hawaii, southern North America, Central America, the Caribbean, and western South America.
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=Annular Solar Eclipse of 2067 Jun 11|url=https://eclipsewise.com/solar/SEprime/2001-2100/SE2067Jun11Aprime.html|publisher=EclipseWise.com|access-date=19 August 2024}}
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|+June 11, 2067 Solar Eclipse Times ! Event ! Time (UTC) |
First Penumbral External Contact
| 2067 June 11 at 17:41:42.1 UTC |
First Umbral External Contact
| 2067 June 11 at 18:45:02.0 UTC |
First Central Line
| 2067 June 11 at 18:46:37.3 UTC |
First Umbral Internal Contact
| 2067 June 11 at 18:48:12.5 UTC |
First Penumbral Internal Contact
| 2067 June 11 at 19:51:38.7 UTC |
Greatest Eclipse
| 2067 June 11 at 20:42:26.4 UTC |
Equatorial Conjunction
| 2067 June 11 at 20:42:35.2 UTC |
Ecliptic Conjunction
| 2067 June 11 at 20:42:53.4 UTC |
Greatest Duration
| 2067 June 11 at 20:43:57.1 UTC |
Last Penumbral Internal Contact
| 2067 June 11 at 21:33:13.1 UTC |
Last Umbral Internal Contact
| 2067 June 11 at 22:36:38.6 UTC |
Last Central Line
| 2067 June 11 at 22:38:16.2 UTC |
Last Umbral External Contact
| 2067 June 11 at 22:39:53.8 UTC |
Last Penumbral External Contact
| 2067 June 11 at 23:43:15.9 UTC |
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|+June 11, 2067 Solar Eclipse Parameters ! Parameter ! Value |
Eclipse Magnitude
| 0.96702 |
Eclipse Obscuration
| 0.93513 |
Gamma
| −0.03865 |
Sun Right Ascension
| 05h20m58.3s |
Sun Declination
| +23°07'36.6" |
Sun Semi-Diameter
| 15'45.1" |
Sun Equatorial Horizontal Parallax
| 08.7" |
Moon Right Ascension
| 05h20m58.0s |
Moon Declination
| +23°05'29.3" |
Moon Semi-Diameter
| 15'00.0" |
Moon Equatorial Horizontal Parallax
| 0°55'03.2" |
ΔT
| 95.6 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.
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|+ Eclipse season of May–June 2067 ! May 28 | ||
200px | 200px | |
align=center
| Penumbral lunar eclipse | Annular solar eclipse Solar Saros 138 | Penumbral lunar eclipse Lunar Saros 150 |
Related eclipses
= Eclipses in 2067 =
- A penumbral lunar eclipse on May 28.
- An annular solar eclipse on June 11.
- A penumbral lunar eclipse on June 27.
- A penumbral lunar eclipse on November 21.
- A hybrid solar eclipse on December 6.
= Metonic =
- Preceded by: Solar eclipse of August 24, 2063
- Followed by: Solar eclipse of March 31, 2071
= Tzolkinex =
- Preceded by: Solar eclipse of April 30, 2060
- Followed by: Solar eclipse of July 24, 2074
= Half-Saros =
- Preceded by: Lunar eclipse of June 6, 2058
- Followed by: Lunar eclipse of June 17, 2076
= Tritos =
- Preceded by: Solar eclipse of July 12, 2056
- Followed by: Solar eclipse of May 11, 2078
= Solar Saros 138 =
- Preceded by: Solar eclipse of May 31, 2049
- Followed by: Solar eclipse of June 22, 2085
= Inex =
- Preceded by: Solar eclipse of July 2, 2038
- Followed by: Solar eclipse of May 22, 2096
= Triad =
- Preceded by: Solar eclipse of August 10, 1980
- Followed by: Solar eclipse of April 12, 2154
= Solar eclipses of 2065–2069 =
{{Solar eclipse set 2065–2069}}
= Saros 138 =
{{Solar Saros series 138}}
= Metonic series =
{{Solar Metonic series 2029–2116}}
= Tritos series =
{{Solar Tritos series 2001 December 14}}
= Inex series =
{{Solar Inex series 2009 July 22}}
References
{{reflist}}
External links
{{Solar eclipse NASA reference|2051/SE2067Jun11A|20670511}}
{{Solar eclipses}}