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Solar eclipse of June 11, 2086

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Solar eclipse of June 11, 2086
Map
Type of eclipse
NatureTotal
Gamma−0.7215
Magnitude1.0174
Maximum eclipse
Duration108 s (1 min 48 s)
Coordinates23°12′S 12°30′E / 23.2°S 12.5°E / -23.2; 12.5
Max. width of band86 km (53 mi)
Times (UTC)
Greatest eclipse11:07:14
References
Saros148 (25 of 75)
Catalog # (SE5000)9701

A total solar eclipse will occur at the Moon's descending node of orbit on Tuesday, June 11, 2086,[1] with a magnitude of 1.0174. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 4.4 days after perigee (on June 7, 2086, at 2:30 UTC), the Moon's apparent diameter will be larger.[2]

The path of totality will be visible from parts of Namibia, Botswana, and South Africa. A partial solar eclipse will also be visible for parts of eastern Brazil, Southern Africa, and Central Africa.

Eclipse details

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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 11, 2086 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 2086 June 11 at 08:38:38.2 UTC
First Umbral External Contact 2086 June 11 at 09:51:48.2 UTC
First Central Line 2086 June 11 at 09:52:03.8 UTC
First Umbral Internal Contact 2086 June 11 at 09:52:19.5 UTC
Greatest Duration 2086 June 11 at 11:05:08.5 UTC
Greatest Eclipse 2086 June 11 at 11:07:13.9 UTC
Equatorial Conjunction 2086 June 11 at 11:09:41.4 UTC
Ecliptic Conjunction 2086 June 11 at 11:15:00.5 UTC
Last Umbral Internal Contact 2086 June 11 at 12:22:09.7 UTC
Last Central Line 2086 June 11 at 12:22:22.6 UTC
Last Umbral External Contact 2086 June 11 at 12:22:35.5 UTC
Last Penumbral External Contact 2086 June 11 at 13:35:54.0 UTC
June 11, 2086 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 1.01736
Eclipse Obscuration 1.03502
Gamma −0.72150
Sun Right Ascension 05h20m59.8s
Sun Declination +23°07'28.2"
Sun Semi-Diameter 15'45.2"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 05h20m54.1s
Moon Declination +22°25'37.5"
Moon Semi-Diameter 15'51.0"
Moon Equatorial Horizontal Parallax 0°58'10.3"
ΔT 110.9 s

Eclipse season

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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.

Eclipse season of May–June 2086
May 28
Ascending node (full moon)
June 11
Descending node (new moon)
Partial lunar eclipse
Lunar Saros 122
Total solar eclipse
Solar Saros 148
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Eclipses in 2086

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Solar Saros 148

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Inex

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Triad

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Solar eclipses of 2083–2087

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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

Partial
1.5465 123 January 7, 2084

Partial
−1.0715
128 July 3, 2084

Annular
0.8208 133 December 27, 2084

Total
−0.4094
138 June 22, 2085

Annular
0.0452 143 December 16, 2085

Annular
0.2786
148 June 11, 2086

Total
−0.7215 153 December 6, 2086

Partial
1.0194
158 June 1, 2087

Partial
−1.4186

Saros 148

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This eclipse is a part of Saros series 148, repeating every 18 years, 11 days, and containing 75 events. The series started with a partial solar eclipse on September 21, 1653. It contains annular eclipses on April 29, 2014 and May 9, 2032; a hybrid eclipse on May 20, 2050; and total eclipses from May 31, 2068 through August 3, 2771. The series ends at member 75 as a partial eclipse on December 12, 2987. 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 will be produced by member 22 at 22 seconds (by default) on May 9, 2032, and the longest duration of totality will be produced by member 54 at 5 minutes, 23 seconds on April 26, 2609. All eclipses in this series occur at the Moon’s descending node of orbit.[5]

Series members 10–31 occur between 1801 and 2200:
10 11 12

December 30, 1815

January 9, 1834

January 21, 1852
13 14 15

January 31, 1870

February 11, 1888

February 23, 1906
16 17 18

March 5, 1924

March 16, 1942

March 27, 1960
19 20 21

April 7, 1978

April 17, 1996

April 29, 2014
22 23 24

May 9, 2032

May 20, 2050

May 31, 2068
25 26 27

June 11, 2086

June 22, 2104

July 4, 2122
28 29 30

July 14, 2140

July 25, 2158

August 4, 2176
31

August 16, 2194

Metonic series

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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 12, 2029 and November 4, 2116
June 11–12 March 30–31 January 16 November 4–5 August 23–24
118 120 122 124 126

June 12, 2029

March 30, 2033

January 16, 2037

November 4, 2040

August 23, 2044
128 130 132 134 136

June 11, 2048

March 30, 2052

January 16, 2056

November 5, 2059

August 24, 2063
138 140 142 144 146

June 11, 2067

March 31, 2071

January 16, 2075

November 4, 2078

August 24, 2082
148 150 152 154 156

June 11, 2086

March 31, 2090

January 16, 2094

November 4, 2097

August 24, 2101
158 160 162 164

June 12, 2105

November 4, 2116

Tritos series

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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

August 28, 1802
(Saros 122)

July 27, 1813
(Saros 123)

June 26, 1824
(Saros 124)

May 27, 1835
(Saros 125)

April 25, 1846
(Saros 126)

March 25, 1857
(Saros 127)

February 23, 1868
(Saros 128)

January 22, 1879
(Saros 129)

December 22, 1889
(Saros 130)

November 22, 1900
(Saros 131)

October 22, 1911
(Saros 132)

September 21, 1922
(Saros 133)

August 21, 1933
(Saros 134)

July 20, 1944
(Saros 135)

June 20, 1955
(Saros 136)

May 20, 1966
(Saros 137)

April 18, 1977
(Saros 138)

March 18, 1988
(Saros 139)

February 16, 1999
(Saros 140)

January 15, 2010
(Saros 141)

December 14, 2020
(Saros 142)

November 14, 2031
(Saros 143)

October 14, 2042
(Saros 144)

September 12, 2053
(Saros 145)

August 12, 2064
(Saros 146)

July 13, 2075
(Saros 147)

June 11, 2086
(Saros 148)

May 11, 2097
(Saros 149)

April 11, 2108
(Saros 150)

March 11, 2119
(Saros 151)

February 8, 2130
(Saros 152)

January 8, 2141
(Saros 153)

December 8, 2151
(Saros 154)

November 7, 2162
(Saros 155)

October 7, 2173
(Saros 156)

September 4, 2184
(Saros 157)

August 5, 2195
(Saros 158)

Inex series

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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

December 9, 1825
(Saros 139)

November 20, 1854
(Saros 140)

October 30, 1883
(Saros 141)

October 10, 1912
(Saros 142)

September 21, 1941
(Saros 143)

August 31, 1970
(Saros 144)

August 11, 1999
(Saros 145)

July 22, 2028
(Saros 146)

July 1, 2057
(Saros 147)

June 11, 2086
(Saros 148)

May 24, 2115
(Saros 149)

May 3, 2144
(Saros 150)

April 12, 2173
(Saros 151)

Notes

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  1. ^ "June 11, 2086 Total Solar Eclipse". timeanddate. Retrieved 24 August 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 24 August 2024.
  3. ^ "Total Solar Eclipse of 2086 Jun 11". EclipseWise.com. Retrieved 24 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 148". eclipse.gsfc.nasa.gov.

References

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