Solar eclipse of June 22, 2085
Template:Short description Script error: No such module "Solar eclipse". An annular solar eclipse will occur at the Moon's descending node of orbit on Friday, June 22, 2085,[1] with a magnitude of 0.9704. 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 4.6 days before apogee (on June 26, 2085, at 16:30 UTC), the Moon's apparent diameter will be smaller.[2]
The path of annularity will be visible from parts of India, Myanmar, China, the Ryukyu Islands (including Okinawa), the Marshall Islands, and Kiribati. A partial solar eclipse will also be visible for parts of South Asia, Southeast Asia, East Asia, Oceania, and Hawaii.
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 | 2085 June 22 at 00:21:14.2 UTC |
| First Umbral External Contact | 2085 June 22 at 01:24:22.9 UTC |
| First Central Line | 2085 June 22 at 01:25:50.9 UTC |
| First Umbral Internal Contact | 2085 June 22 at 01:27:19.0 UTC |
| First Penumbral Internal Contact | 2085 June 22 at 02:30:35.9 UTC |
| Greatest Duration | 2085 June 22 at 03:17:43.0 UTC |
| Equatorial Conjunction | 2085 June 22 at 03:20:41.0 UTC |
| Ecliptic Conjunction | 2085 June 22 at 03:20:44.5 UTC |
| Greatest Eclipse | 2085 June 22 at 03:21:15.9 UTC |
| Last Penumbral Internal Contact | 2085 June 22 at 04:11:55.8 UTC |
| Last Umbral Internal Contact | 2085 June 22 at 05:15:11.5 UTC |
| Last Central Line | 2085 June 22 at 05:16:42.0 UTC |
| Last Umbral External Contact | 2085 June 22 at 05:18:12.5 UTC |
| Last Penumbral External Contact | 2085 June 22 at 06:21:23.2 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.97041 |
| Eclipse Obscuration | 0.94170 |
| Gamma | 0.04525 |
| Sun Right Ascension | 06h06m22.6s |
| Sun Declination | +23°25'12.0" |
| Sun Semi-Diameter | 15'44.3" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 06h06m23.8s |
| Moon Declination | +23°27'40.5" |
| Moon Semi-Diameter | 15'02.4" |
| Moon Equatorial Horizontal Parallax | 0°55'11.8" |
| ΔT | 110.1 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. The first and last eclipse in this sequence is separated by one synodic month.
| June 8 Ascending node (full moon) |
June 22 Descending node (new moon) |
July 7 Ascending node (full moon) |
|---|---|---|
| File:SE2085Jun22A.png | ||
| Penumbral lunar eclipse Lunar Saros 112 |
Annular solar eclipse Solar Saros 138 |
Penumbral lunar eclipse Lunar Saros 150 |
Related eclipses
Eclipses in 2085
- A penumbral lunar eclipse on January 10.
- A penumbral lunar eclipse on June 8.
- An annular solar eclipse on June 22.
- A penumbral lunar eclipse on July 7.
- A penumbral lunar eclipse on December 1.
- An annular solar eclipse on December 16.
Metonic
- Preceded by: Solar eclipse of September 3, 2081
- Followed by: Solar eclipse of April 10, 2089
Tzolkinex
- Preceded by: Solar eclipse of May 11, 2078
- Followed by: Solar eclipse of August 3, 2092
Half-Saros
- Preceded by: Lunar eclipse of June 17, 2076
- Followed by: Lunar eclipse of June 28, 2094
Tritos
- Preceded by: Solar eclipse of July 24, 2074
- Followed by: Solar eclipse of May 22, 2096
Solar Saros 138
- Preceded by: Solar eclipse of June 11, 2067
- Followed by: Solar eclipse of July 4, 2103
Inex
- Preceded by: Solar eclipse of July 12, 2056
- Followed by: Solar eclipse of June 3, 2114
Triad
- Preceded by: Solar eclipse of August 22, 1998
- Followed by: Solar eclipse of April 23, 2172
Solar eclipses of 2083–2087
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 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 138
Template:Solar Saros series 138
Metonic series
Template:Solar Metonic series 2047–2134
Tritos series
Template:Solar Tritos series 2009 January 26
Inex series
Template:Solar Inex series 2027 August 2
Notes
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References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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