Solar eclipse of June 22, 2085

Last updated
Solar eclipse of June 22, 2085
SE2085Jun22A.png
Map
Type of eclipse
NatureAnnular
Gamma 0.0452
Magnitude 0.9704
Maximum eclipse
Duration209 s (3 min 29 s)
Coordinates 26°12′N131°18′E / 26.2°N 131.3°E / 26.2; 131.3
Max. width of band106 km (66 mi)
Times (UTC)
Greatest eclipse3:21:16
References
Saros 138 (35 of 70)
Catalog # (SE5000) 9699

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]

Contents

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]

June 22, 2085 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2085 June 22 at 00:21:14.2 UTC
First Umbral External Contact2085 June 22 at 01:24:22.9 UTC
First Central Line2085 June 22 at 01:25:50.9 UTC
First Umbral Internal Contact2085 June 22 at 01:27:19.0 UTC
First Penumbral Internal Contact2085 June 22 at 02:30:35.9 UTC
Greatest Duration2085 June 22 at 03:17:43.0 UTC
Equatorial Conjunction2085 June 22 at 03:20:41.0 UTC
Ecliptic Conjunction2085 June 22 at 03:20:44.5 UTC
Greatest Eclipse2085 June 22 at 03:21:15.9 UTC
Last Penumbral Internal Contact2085 June 22 at 04:11:55.8 UTC
Last Umbral Internal Contact2085 June 22 at 05:15:11.5 UTC
Last Central Line2085 June 22 at 05:16:42.0 UTC
Last Umbral External Contact2085 June 22 at 05:18:12.5 UTC
Last Penumbral External Contact2085 June 22 at 06:21:23.2 UTC
June 22, 2085 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.97041
Eclipse Obscuration0.94170
Gamma0.04525
Sun Right Ascension06h06m22.6s
Sun Declination+23°25'12.0"
Sun Semi-Diameter15'44.3"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension06h06m23.8s
Moon Declination+23°27'40.5"
Moon Semi-Diameter15'02.4"
Moon Equatorial Horizontal Parallax0°55'11.8"
ΔT110.1 s

Eclipse season

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.

Eclipse season of June–July 2085
June 8
Ascending node (full moon)
 June 22
Descending node (new moon)
 July 7
Ascending node (full moon)
SE2085Jun22A.png
Penumbral lunar eclipse
Lunar Saros 112		 Annular solar eclipse
Solar Saros 138		 Penumbral lunar eclipse
Lunar Saros 150

Eclipses in 2085

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 138

Inex

Triad

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
SarosMapGammaSarosMapGamma
118 July 15, 2083
SE2083Jul15P.png
Partial		1.5465123 January 7, 2084
SE2084Jan07P.png
Partial		−1.0715
128 July 3, 2084
SE2084Jul03A.png
Annular		0.8208133 December 27, 2084
SE2084Dec27T.png
Total		−0.4094
138 June 22, 2085
SE2085Jun22A.png
Annular		0.0452143 December 16, 2085
SE2085Dec16A.png
Annular		0.2786
148 June 11, 2086
SE2086Jun11T.png
Total		−0.7215153 December 6, 2086
SE2086Dec06P.png
Partial		1.0194
158 June 1, 2087
SE2087Jun01P.png
Partial		−1.4186

Saros 138

This eclipse is a part of Saros series 138, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on June 6, 1472. It contains annular eclipses from August 31, 1598 through February 18, 2482; a hybrid eclipse on March 1, 2500; and total eclipses from March 12, 2518 through April 3, 2554. The series ends at member 70 as a partial eclipse on July 11, 2716. 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 annularity was produced by member 23 at 8 minutes, 2 seconds on February 11, 1869, and the longest duration of totality will be produced by member 61 at 56 seconds on April 3, 2554. All eclipses in this series occur at the Moon’s descending node of orbit. [5]

Series members 20–41 occur between 1801 and 2200:
202122
SE1815Jan10A.png
January 10, 1815		 SE1833Jan20A.png
January 20, 1833		 SE1851Feb01A.png
February 1, 1851
232425
SE1869Feb11A.png
February 11, 1869		 SE1887Feb22A.png
February 22, 1887		 SE1905Mar06A.png
March 6, 1905
262728
SE1923Mar17A.png
March 17, 1923 		SE1941Mar27A.png
March 27, 1941 		SE1959Apr08A.png
April 8, 1959
293031
SE1977Apr18A.png
April 18, 1977 		SE1995Apr29A.png
April 29, 1995 		SE2013May10A.png
May 10, 2013
323334
SE2031May21A.png
May 21, 2031 		SE2049May31A.png
May 31, 2049 		SE2067Jun11A.png
June 11, 2067
353637
SE2085Jun22A.png
June 22, 2085 		SE2103Jul04A.png
July 4, 2103		 SE2121Jul14A.png
July 14, 2121
383940
SE2139Jul25A.png
July 25, 2139		 SE2157Aug05A.png
August 5, 2157		 SE2175Aug16A.png
August 16, 2175
41
SE2193Aug26A.png
August 26, 2193

Metonic series

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.

22 eclipse events between June 23, 2047 and November 16, 2134
June 22–23April 10–11January 27–29November 15–16September 3–5
118120122124126
SE2047Jun23P.png
June 23, 2047 		SE2051Apr11P.png
April 11, 2051 		SE2055Jan27P.png
January 27, 2055 		SE2058Nov16P.png
November 16, 2058 		SE2062Sep03P.png
September 3, 2062
128130132134136
SE2066Jun22A.png
June 22, 2066 		SE2070Apr11T.png
April 11, 2070 		SE2074Jan27A.png
January 27, 2074 		SE2077Nov15A.png
November 15, 2077 		SE2081Sep03T.png
September 3, 2081
138140142144146
SE2085Jun22A.png
June 22, 2085 		SE2089Apr10A.png
April 10, 2089 		SE2093Jan27T.png
January 27, 2093 		SE2096Nov15A.png
November 15, 2096 		SE2100Sep04T.png
September 4, 2100
148150152154156
SE2104Jun22T.png
June 22, 2104		 SE2108Apr11P.gif
April 11, 2108		 Saros152 18van70 SE2112Jan29T.jpg
January 29, 2112		 SE2115Nov16A.png
November 16, 2115		 Saros156 07van69 SE2119Sep05P.jpg
September 5, 2119
158160162164
Saros158 04van70 SE2123Jun23P.jpg
June 23, 2123		 Saros164 03van80 SE2134Nov16P.jpg
November 16, 2134

Tritos series

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 1801 and 2200
SE1801Sep08P.png
September 8, 1801
(Saros 112)		 SE1812Aug07P.gif
August 7, 1812
(Saros 113)		 SE1823Jul08P.gif
July 8, 1823
(Saros 114)		 SE1834Jun07P.gif
June 7, 1834
(Saros 115)		 SE1845May06An.gif
May 6, 1845
(Saros 116)
SE1856Apr05T.gif
April 5, 1856
(Saros 117)		 SE1867Mar06A.gif
March 6, 1867
(Saros 118)		 SE1878Feb02A.gif
February 2, 1878
(Saros 119)		 SE1889Jan01T.png
January 1, 1889
(Saros 120)		 SE1899Dec03A.png
December 3, 1899
(Saros 121)
SE1910Nov02P.png
November 2, 1910
(Saros 122)		 SE1921Oct01T.png
October 1, 1921
(Saros 123)		 SE1932Aug31T.png
August 31, 1932
(Saros 124)		 SE1943Aug01A.png
August 1, 1943
(Saros 125)		 SE1954Jun30T.png
June 30, 1954
(Saros 126)
SE1965May30T.png
May 30, 1965
(Saros 127)		 SE1976Apr29A.png
April 29, 1976
(Saros 128)		 SE1987Mar29H.png
March 29, 1987
(Saros 129)		 SE1998Feb26T.png
February 26, 1998
(Saros 130)		 SE2009Jan26A.png
January 26, 2009
(Saros 131)
SE2019Dec26A.png
December 26, 2019
(Saros 132)		 SE2030Nov25T.png
November 25, 2030
(Saros 133)		 SE2041Oct25A.png
October 25, 2041
(Saros 134)		 SE2052Sep22A.png
September 22, 2052
(Saros 135)		 SE2063Aug24T.png
August 24, 2063
(Saros 136)
SE2074Jul24A.png
July 24, 2074
(Saros 137)		 SE2085Jun22A.png
June 22, 2085
(Saros 138)		 SE2096May22T.png
May 22, 2096
(Saros 139)		 SE2107Apr23A.png
April 23, 2107
(Saros 140)		 SE2118Mar22A.png
March 22, 2118
(Saros 141)
SE2129Feb18T.png
February 18, 2129
(Saros 142)		 SE2140Jan20A.png
January 20, 2140
(Saros 143)		 SE2150Dec19A.png
December 19, 2150
(Saros 144)		 SE2161Nov17T.png
November 17, 2161
(Saros 145)		 SE2172Oct17H.png
October 17, 2172
(Saros 146)
Saros147 32van80 SE2183Sep16A.jpg
September 16, 2183
(Saros 147)		 Saros148 31van75 SE2194Aug16T.jpg
August 16, 2194
(Saros 148)

Inex series

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
SE1824Dec20Am.gif
December 20, 1824
(Saros 129)		 SE1853Nov30T.png
November 30, 1853
(Saros 130)		 SE1882Nov10A.gif
November 10, 1882
(Saros 131)
SE1911Oct22A.png
October 22, 1911
(Saros 132)		 SE1940Oct01T.png
October 1, 1940
(Saros 133)		 SE1969Sep11A.png
September 11, 1969
(Saros 134)
SE1998Aug22A.png
August 22, 1998
(Saros 135)		 SE2027Aug02T.png
August 2, 2027
(Saros 136)		 SE2056Jul12A.png
July 12, 2056
(Saros 137)
SE2085Jun22A.png
June 22, 2085
(Saros 138)		 SE2114Jun03T.png
June 3, 2114
(Saros 139)		 SE2143May14A.png
May 14, 2143
(Saros 140)
SE2172Apr23A.png
April 23, 2172
(Saros 141)

Notes

  1. ↑ "June 22, 2085 Annular Solar Eclipse". timeanddate. Retrieved 23 August 2024.
  2. ↑ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 23 August 2024.
  3. ↑ "Annular Solar Eclipse of 2085 Jun 22". EclipseWise.com. Retrieved 23 August 2024.
  4. ↑ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
  5. ↑ "NASA - Catalog of Solar Eclipses of Saros 138". eclipse.gsfc.nasa.gov.

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References

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