Solar eclipse of July 1, 2076

Solar eclipse of July 1, 2076
Solar eclipse of July 1, 2076
	Map
Type of eclipse
Nature	Partial
Gamma	1.4005
Magnitude	0.2746
Maximum eclipse
Coordinates	67°00′N 98°06′W / 67°N 98.1°W
Times (UTC)
Greatest eclipse	6:50:43
References
Saros	157 (2 of 70)
Catalog # (SE5000)	9678

A partial solar eclipse will occur at the Moon's ascending node of orbit on Wednesday, July 1, 2076, with a magnitude of 0.2746. 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 third of four solar eclipses in 2076, with the others occurring on January 6, June 1, and November 26.

Related eclipses

Eclipses in 2076

Solar eclipses of 2073–2076

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 June 1, 2076 and November 26, 2076 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2073 to 2076
Descending node			Ascending node
Saros	Map	Gamma	Saros	Map	Gamma
122	February 7, 2073 Partial	1.1651	127	August 3, 2073 Total	−0.8763
132	January 27, 2074 Annular	0.4251	137	July 24, 2074 Annular	−0.1242
142	January 16, 2075 Total	−0.2799	147	July 13, 2075 Annular	0.6583
152	January 6, 2076 Total	−0.9373	157	July 1, 2076 Partial	1.4005

Saros 157

This eclipse is a part of Saros series 157, repeating every 18 years, 11 days, and containing 70 events. The series will start with a partial solar eclipse on June 21, 2058. It contains annular eclipses from August 25, 2166 through March 10, 2491; hybrid eclipses from March 22, 2509 through April 12, 2545; and total eclipses from April 24, 2563 through April 21, 3158. The series ends at member 70 as a partial eclipse on July 17, 3302. 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 15 at 4 minutes, 16 seconds on November 22, 2310, and the longest duration of totality will be produced by member 38 at 5 minutes, 57 seconds on July 31, 2725. All eclipses in this series occur at the Moon’s ascending node of orbit.^[2]

Series members 1–8 occur between 2058 and 2200:
1	2	3
June 21, 2058	July 1, 2076	July 12, 2094
4	5	6
July 23, 2112	August 4, 2130	August 14, 2148
7	8
August 25, 2166	September 4, 2184

Metonic series

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 ascending node.

21 eclipse events between July 1, 2000 and July 1, 2076
July 1–2	April 19–20	February 5–7	November 24–25	September 12–13
117	119	121	123	125
July 1, 2000	April 19, 2004	February 7, 2008	November 25, 2011	September 13, 2015
127	129	131	133	135
July 2, 2019	April 20, 2023	February 6, 2027	November 25, 2030	September 12, 2034
137	139	141	143	145
July 2, 2038	April 20, 2042	February 5, 2046	November 25, 2049	September 12, 2053
147	149	151	153	155
July 1, 2057	April 20, 2061	February 5, 2065	November 24, 2068	September 12, 2072
157
July 1, 2076

Tritos series

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 2087
August 17, 1803 (Saros 132)	July 17, 1814 (Saros 133)	June 16, 1825 (Saros 134)	May 15, 1836 (Saros 135)	April 15, 1847 (Saros 136)
March 15, 1858 (Saros 137)	February 11, 1869 (Saros 138)	January 11, 1880 (Saros 139)	December 12, 1890 (Saros 140)	November 11, 1901 (Saros 141)
October 10, 1912 (Saros 142)	September 10, 1923 (Saros 143)	August 10, 1934 (Saros 144)	July 9, 1945 (Saros 145)	June 8, 1956 (Saros 146)
May 9, 1967 (Saros 147)	April 7, 1978 (Saros 148)	March 7, 1989 (Saros 149)	February 5, 2000 (Saros 150)	January 4, 2011 (Saros 151)
December 4, 2021 (Saros 152)	November 3, 2032 (Saros 153)	October 3, 2043 (Saros 154)	September 2, 2054 (Saros 155)	August 2, 2065 (Saros 156)
July 1, 2076 (Saros 157)	June 1, 2087 (Saros 158)

Inex series

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 30, 1815 (Saros 148)	December 9, 1844 (Saros 149)	November 20, 1873 (Saros 150)
October 31, 1902 (Saros 151)	October 11, 1931 (Saros 152)	September 20, 1960 (Saros 153)
August 31, 1989 (Saros 154)	August 11, 2018 (Saros 155)	July 22, 2047 (Saros 156)
July 1, 2076 (Saros 157)	June 12, 2105 (Saros 158)	May 23, 2134 (Saros 159)
	April 12, 2192 (Saros 161)