Wikipedia

Solar eclipse of July 3, 2065

A partial solar eclipse will occur at the Moon's descending node of orbit on Friday, July 3, 2065,[1] 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.

Solar eclipse of July 3, 2065
Map
Type of eclipse
NaturePartial
Gamma1.4619
Magnitude0.1638
Maximum eclipse
Coordinates64°48′N 71°54′E / 64.8°N 71.9°E / 64.8; 71.9
Times (UTC)
Greatest eclipse17:33:52
References
Saros118 (71 of 72)
Catalog # (SE5000)9654

This will be the second of four partial solar eclipses in 2065, with the others occurring on February 5, August 2, and December 27.

The partial solar eclipse will be visible for parts of Northern Europe and northern Russia.

Eclipse details

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Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.[2]

July 3, 2065 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 2065 July 03 at 16:32:44.5 UTC
Equatorial Conjunction 2065 July 03 at 17:01:37.1 UTC
Ecliptic Conjunction 2065 July 03 at 17:17:29.5 UTC
Greatest Eclipse 2065 July 03 at 17:33:52.5 UTC
Last Penumbral External Contact 2065 July 03 at 18:35:10.0 UTC
July 3, 2065 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.16388
Eclipse Obscuration 0.07678
Gamma 1.46186
Sun Right Ascension 06h53m43.9s
Sun Declination +22°51'26.7"
Sun Semi-Diameter 15'43.9"
Sun Equatorial Horizontal Parallax 08.6"
Moon Right Ascension 06h54m50.6s
Moon Declination +24°10'43.8"
Moon Semi-Diameter 15'05.3"
Moon Equatorial Horizontal Parallax 0°55'22.6"
ΔT 94.2 s

Eclipse season

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See also: Eclipse cycle

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight. The first and last eclipse in this sequence is separated by one synodic month.

Eclipse season of July–August 2065
July 3
Descending node (new moon)
 July 17
Ascending node (full moon)
 August 2
Descending node (new moon)
     
Partial solar eclipse
Solar Saros 118		 Total lunar eclipse
Lunar Saros 130		 Partial solar eclipse
Solar Saros 156
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Eclipses in 2065

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Solar Saros 118

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Inex

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Triad

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Solar eclipses of 2065–2069

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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.[3]

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

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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.[4]

Metonic series

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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

Tritos series

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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 2054 and 2200
 
August 3, 2054
(Saros 117) 		 
July 3, 2065
(Saros 118) 		 
June 1, 2076
(Saros 119) 		 
May 2, 2087
(Saros 120) 		 
April 1, 2098
(Saros 121)
 
March 1, 2109
(Saros 122) 		 
January 30, 2120
(Saros 123) 		 
December 30, 2130
(Saros 124) 		 
November 28, 2141
(Saros 125) 		 
October 28, 2152
(Saros 126)
 
September 28, 2163
(Saros 127) 		 
August 27, 2174
(Saros 128) 		 
July 26, 2185
(Saros 129) 		 
June 26, 2196
(Saros 130)

Inex series

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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.

The partial solar eclipses on January 1, 1805 (part of Saros 109) and November 21, 1862 (part of Saros 111) are also a part of this series but are not included in the table below.

Series members between 2036 and 2200
 
July 23, 2036
(Saros 117) 		 
July 3, 2065
(Saros 118) 		 
June 13, 2094
(Saros 119)
 
May 25, 2123
(Saros 120) 		 
May 4, 2152
(Saros 121) 		 
April 14, 2181
(Saros 122)

References

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  1. ^ "July 3, 2065 Partial Solar Eclipse". timeanddate. Retrieved 19 August 2024.
  2. ^ "Partial Solar Eclipse of 2065 Jul 03". EclipseWise.com. Retrieved 19 August 2024.
  3. ^ 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.
  4. ^ "NASA - Catalog of Solar Eclipses of Saros 118". eclipse.gsfc.nasa.gov.
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