Solar eclipse of June 11, 2086

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Solar eclipse of June 11, 2086
SE2086Jun11T.png
Map
Type of eclipse
NatureTotal
Gamma-0.7215
Magnitude1.0174
Maximum eclipse
Duration108 sec (1 m 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 on June 11, 2086. 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.

Related eclipses

Solar eclipses 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.[1]

Solar eclipse series sets from 2083–2087
Descending node   Ascending node
118 July 15, 2083
SE2083Jul15P.png
Partial
123 January 7, 2084
SE2084Jan07P.png
Partial
128 July 3, 2084
SE2084Jul03A.png
Annular
133 December 27, 2084
SE2084Dec27T.png
Total
138 June 22, 2085
SE2085Jun22A.png
Annular
143 December 16, 2085
SE2085Dec16A.png
Annular
148 June 11, 2086
SE2086Jun11T.png
Total
153 December 6, 2086
SE2086Dec06P.png
Partial
158 June 1, 2087
SE2087Jun01P.png
Partial

Saros 148

Solar saros 148, repeating every about 18 years and 11 days, contains 75 events. The series started with a partial solar eclipse on September 21, 1653. It has annular eclipses on April 29, 2014, and May 9, 2032, and a hybrid eclipse on May 20, 2050. It has total eclipses from May 31, 2068, to August 3, 2771. The series ends at member 75 as a partial eclipse on December 12, 2987. The longest total eclipse will be on April 26, 2609, at 5 minutes and 23 seconds.[2]

Series members 15–25 occur between 1901 and 2100:
15 16 17
SE1906Feb23P.png
February 23, 1906
SE1924Mar05P.png
March 5, 1924
SE1942Mar16P.png
March 16, 1942
18 19 20
SE1960Mar27P.png
March 27, 1960
SE1978Apr07P.png
April 7, 1978
SE1996Apr17P.png
April 17, 1996
21 22 23
SE2014Apr29A.png
April 29, 2014
SE2032May09A.png
May 9, 2032
SE2050May20H.png
May 20, 2050
24 25
SE2068May31T.png
May 31, 2068
SE2086Jun11T.png
June 11, 2086

Metonic cycle

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).

Notes

  1. ^ 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.
  2. ^ Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site.

References