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Solar eclipse of July 15, 2083

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Solar eclipse of July 15, 2083
Map
Type of eclipse
NaturePartial
Gamma1.5465
Magnitude0.0168
Maximum eclipse
Coordinates64°00′N 37°42′W / 64°N 37.7°W / 64; -37.7
Times (UTC)
Greatest eclipse0:14:23
References
Saros118 (72 of 72)
Catalog # (SE5000)9695

A partial solar eclipse will occur at the Moon's descending node of orbit on Thursday, July 15, 2083, with a magnitude of 0.0168. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth. This will be the 72nd and final event from Solar Saros 118.

Related eclipses[edit]

Eclipses in 2083[edit]

Metonic[edit]

Tzolkinex[edit]

Half-Saros[edit]

Tritos[edit]

Solar Saros 118[edit]

Inex[edit]

Triad[edit]

Solar eclipses of 2083–2087[edit]

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

Saros 118[edit]

This eclipse is a part of Saros series 118, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on May 24, 803 AD. It contains total eclipses from August 19, 947 AD through October 25, 1650; hybrid eclipses on November 4, 1668 and November 15, 1686; and annular eclipses from November 27, 1704 through April 30, 1957. The series ends at member 72 as a partial eclipse on July 15, 2083. 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 totality was produced by member 34 at 6 minutes, 59 seconds on May 16, 1398, and the longest duration of annularity was produced by member 59 at 1 minutes, 58 seconds on February 23, 1849. All eclipses in this series occur at the Moon’s descending node of orbit.[2]

References[edit]

  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. ^ "NASA - Catalog of Solar Eclipses of Saros 118". eclipse.gsfc.nasa.gov.

External links[edit]