Solar eclipse of July 3, 2065 | |
---|---|
Type of eclipse | |
Nature | Partial |
Gamma | 1.4619 |
Magnitude | 0.1638 |
Maximum eclipse | |
Coordinates | 64°48′N 71°54′E / 64.8°N 71.9°E |
Times (UTC) | |
Greatest eclipse | 17:33:52 |
References | |
Saros | 118 (71 of 72) |
Catalog # (SE5000) | 9654 |
A partial solar eclipse will occur at the Moon's descending node of orbit on Friday, July 3, 2065, with a magnitude of 0.1638. 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 second of four partial solar eclipses in 2065, with the others occurring on February 5, August 2, and December 27.
Related eclipses
Eclipses in 2065
- A total lunar eclipse on January 22, 2065.
- A partial solar eclipse on February 5, 2065.
- A partial solar eclipse on July 3, 2065.
- A total lunar eclipse on July 17, 2065.
- A partial solar eclipse on August 2, 2065.
- A partial solar eclipse on December 27, 2065.
Metonic
- Followed by: Solar eclipse of April 21, 2069
Tzolkinex
- Preceded by: Solar eclipse of May 22, 2058
Half-Saros
- Preceded by: Lunar eclipse of June 27, 2056
- Followed by: Lunar eclipse of July 8, 2074
Tritos
- Preceded by: Solar eclipse of August 3, 2054
- Followed by: Solar eclipse of June 1, 2076
Solar Saros 118
- Preceded by: Solar eclipse of June 23, 2047
- Followed by: Solar eclipse of July 15, 2083
Inex
- Preceded by: Solar eclipse of July 23, 2036
- Followed by: Solar eclipse of June 13, 2094
Triad
- Followed by: Solar eclipse of May 4, 2152
Solar eclipses of 2065–2069
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 5, 2065 and August 2, 2065 occur in the previous lunar year eclipse set, and the partial solar eclipses on April 21, 2069 and October 15, 2069 occur in the next lunar year eclipse set.
Solar eclipse series sets from 2065 to 2069 | ||||||
---|---|---|---|---|---|---|
Descending node | Ascending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
118 | July 3, 2065 Partial |
1.4619 | 123 | December 27, 2065 Partial |
−1.0688 | |
128 | June 22, 2066 Annular |
0.733 | 133 | December 17, 2066 Total |
−0.4043 | |
138 | June 11, 2067 Annular |
−0.0387 | 143 | December 6, 2067 Hybrid |
0.2845 | |
148 | May 31, 2068 Total |
−0.797 | 153 | November 24, 2068 Partial |
1.0299 | |
158 | May 20, 2069 Partial |
−1.4852 |
Saros 118
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]
Series members 57–72 occur between 1801 and 2083: | ||
---|---|---|
57 | 58 | 59 |
February 1, 1813 |
February 12, 1831 |
February 23, 1849 |
60 | 61 | 62 |
March 6, 1867 |
March 16, 1885 |
March 29, 1903 |
63 | 64 | 65 |
April 8, 1921 |
April 19, 1939 |
April 30, 1957 |
66 | 67 | 68 |
May 11, 1975 |
May 21, 1993 |
June 1, 2011 |
69 | 70 | 71 |
June 12, 2029 |
June 23, 2047 |
July 3, 2065 |
72 | ||
July 15, 2083 |
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 descending node.
22 eclipse events between July 3, 2065 and November 26, 2152 | ||||
---|---|---|---|---|
July 3–4 | April 21–23 | February 7–8 | November 26–27 | September 13–15 |
118 | 120 | 122 | 124 | 126 |
July 3, 2065 |
April 21, 2069 |
February 7, 2073 |
November 26, 2076 |
September 13, 2080 |
128 | 130 | 132 | 134 | 136 |
July 3, 2084 |
April 21, 2088 |
February 7, 2092 |
November 27, 2095 |
September 14, 2099 |
138 | 140 | 142 | 144 | 146 |
July 4, 2103 |
April 23, 2107 |
February 8, 2111 |
November 27, 2114 |
September 15, 2118 |
148 | 150 | 152 | 154 | 156 |
July 4, 2122 |
April 22, 2126 |
February 8, 2130 |
November 26, 2133 |
September 15, 2137 |
158 | 160 | 162 | 164 | |
July 3, 2141 |
November 26, 2152 |
References
- ^ 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.
- ^ "NASA - Catalog of Solar Eclipses of Saros 118". eclipse.gsfc.nasa.gov.
External links
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC