Solar eclipse of August 13, 2083

Solar eclipse of August 13, 2083
Solar eclipse of August 13, 2083
	Map
Type of eclipse
Nature	Partial
Gamma	−1.2064
Magnitude	0.6146
Maximum eclipse
Coordinates	62°06′S 67°30′W / 62.1°S 67.5°W
Times (UTC)
Greatest eclipse	12:34:41
References
Saros	156 (5 of 69)
Catalog # (SE5000)	9694

A partial solar eclipse will occur at the Moon's descending node of orbit on Friday, August 13, 2083, with a magnitude of 0.6146. 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.

Related eclipses[edit]

Solar eclipses 2080–2083[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 eclipse on July 15, 2083 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 2080 to 2083
Ascending node			Descending node
Saros	Map	Gamma	Saros	Map	Gamma
121	March 21, 2080 Partial	−1.0578	126	September 13, 2080 Partial	1.0723
131	March 10, 2081 Annular	−0.3653	136	September 3, 2081 Total	0.3378
141	February 27, 2082 Annular	0.3361	146	August 24, 2082 Total	−0.4004
151	February 16, 2083 Partial	1.017	156	August 13, 2083 Partial	−1.2064

Saros 156[edit]

This eclipse is a part of Saros series 156, repeating every 18 years, 11 days, and containing 69 events. The series started with a partial solar eclipse on July 1, 2011. It contains annular eclipses from September 26, 2155 through April 7, 3075. There are no hybrid or total eclipses in this set. The series ends at member 69 as a partial eclipse on July 14, 3237. 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 29 at 8 minutes, 28 seconds on May 3, 2516. All eclipses in this series occur at the Moon’s descending node of orbit.^[2]

Series members 1–11 occur between 2011 and 2200:
1	2	3
July 1, 2011	July 11, 2029	July 22, 2047
4	5	6
August 2, 2065	August 13, 2083	August 24, 2101
7	8	9
September 5, 2119	September 15, 2137	September 26, 2155
10	11
October 7, 2173	October 18, 2191

Metonic series[edit]

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.

21 eclipse events between June 1, 2011 and June 1, 2087
May 31 – June 1	March 19–20	January 5–6	October 24–25	August 12–13
118	120	122	124	126
June 1, 2011	March 20, 2015	January 6, 2019	October 25, 2022	August 12, 2026
128	130	132	134	136
June 1, 2030	March 20, 2034	January 5, 2038	October 25, 2041	August 12, 2045
138	140	142	144	146
May 31, 2049	March 20, 2053	January 5, 2057	October 24, 2060	August 12, 2064
148	150	152	154	156
May 31, 2068	March 19, 2072	January 6, 2076	October 24, 2079	August 13, 2083
158	160	162	164	166
June 1, 2087			October 24, 2098