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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 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.

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]

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

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.

References