Solar eclipse of July 3, 2065

Last updated
Solar eclipse of July 3, 2065
SE2065Jul03P.png
Map
Type of eclipse
NaturePartial
Gamma 1.4619
Magnitude 0.1638
Maximum eclipse
Coordinates 64°48′N71°54′E / 64.8°N 71.9°E / 64.8; 71.9
Times (UTC)
Greatest eclipse17:33:52
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, [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.

Contents

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

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
EventTime (UTC)
First Penumbral External Contact2065 July 03 at 16:32:44.5 UTC
Equatorial Conjunction2065 July 03 at 17:01:37.1 UTC
Ecliptic Conjunction2065 July 03 at 17:17:29.5 UTC
Greatest Eclipse2065 July 03 at 17:33:52.5 UTC
Last Penumbral External Contact2065 July 03 at 18:35:10.0 UTC
July 3, 2065 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.16388
Eclipse Obscuration0.07678
Gamma1.46186
Sun Right Ascension06h53m43.9s
Sun Declination+22°51'26.7"
Sun Semi-Diameter15'43.9"
Sun Equatorial Horizontal Parallax08.6"
Moon Right Ascension06h54m50.6s
Moon Declination+24°10'43.8"
Moon Semi-Diameter15'05.3"
Moon Equatorial Horizontal Parallax0°55'22.6"
ΔT94.2 s

Eclipse season

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)
SE2065Jul03P.png Lunar eclipse chart close-2065Jul17.png SE2065Aug02P.png
Partial solar eclipse
Solar Saros 118
Total lunar eclipse
Lunar Saros 130
Partial solar eclipse
Solar Saros 156

Eclipses in 2065

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 118

Inex

Triad

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. [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
SarosMapGammaSarosMapGamma
118 July 3, 2065
SE2065Jul03P.png
Partial
1.4619123 December 27, 2065
SE2065Dec27P.png
Partial
−1.0688
128 June 22, 2066
SE2066Jun22A.png
Annular
0.733133 December 17, 2066
SE2066Dec17T.png
Total
−0.4043
138 June 11, 2067
SE2067Jun11A.png
Annular
−0.0387143 December 6, 2067
SE2067Dec06H.png
Hybrid
0.2845
148 May 31, 2068
SE2068May31T.png
Total
−0.797153 November 24, 2068
SE2068Nov24P.png
Partial
1.0299
158 May 20, 2069
SE2069May20P.png
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. [4]

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 3–4April 21–23February 7–8November 26–27September 13–15
118120122124126
SE2065Jul03P.png
July 3, 2065
SE2069Apr21P.png
April 21, 2069
SE2073Feb07P.png
February 7, 2073
SE2076Nov26P.png
November 26, 2076
SE2080Sep13P.png
September 13, 2080
128130132134136
SE2084Jul03A.png
July 3, 2084
SE2088Apr21T.png
April 21, 2088
SE2092Feb07A.png
February 7, 2092
SE2095Nov27A.png
November 27, 2095
SE2099Sep14T.png
September 14, 2099
138140142144146
SE2103Jul04A.png
July 4, 2103
SE2107Apr23A.png
April 23, 2107
SE2111Feb08T.png
February 8, 2111
SE2114Nov27A.png
November 27, 2114
SE2118Sep15T.png
September 15, 2118
148150152154156
Saros148 27van75 SE2122Jul04T.jpg
July 4, 2122
Saros150 23van71 SE2126Apr22A.jpg
April 22, 2126
Saros152 19van70 SE2130Feb08T.jpg
February 8, 2130
Saros154 13van71 SE2133Nov26A.jpg
November 26, 2133
Saros156 08van69 SE2137Sep15P.jpg
September 15, 2137
158160162164
Saros158 05van70 SE2141Jul03P.jpg
July 3, 2141
Saros164 04van80 SE2152Nov26P.jpg
November 26, 2152

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 2054 and 2200
SE2054Aug03P.png
August 3, 2054
(Saros 117)
SE2065Jul03P.png
July 3, 2065
(Saros 118)
SE2076Jun01P.png
June 1, 2076
(Saros 119)
SE2087May02P.png
May 2, 2087
(Saros 120)
SE2098Apr01P.png
April 1, 2098
(Saros 121)
SE2109Mar01P.png
March 1, 2109
(Saros 122)
Saros123 59van70 SE2120Jan30P.jpg
January 30, 2120
(Saros 123)
Saros124 61van73 SE2130Dec30P.jpg
December 30, 2130
(Saros 124)
Saros125 61van73 SE2141Nov28P.jpg
November 28, 2141
(Saros 125)
Saros126 55van72 SE2152Oct28P.jpg
October 28, 2152
(Saros 126)
Saros127 66van82 SE2163Sep28P.jpg
September 28, 2163
(Saros 127)
Saros128 67van73 SE2174Aug27P.jpg
August 27, 2174
(Saros 128)
Saros129 61van80 SE2185Jul26T.jpg
July 26, 2185
(Saros 129)
SE2196Jun26T.png
June 26, 2196
(Saros 130)

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.

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
SE2036Jul23P.png
July 23, 2036
(Saros 117)
SE2065Jul03P.png
July 3, 2065
(Saros 118)
SE2094Jun13P.png
June 13, 2094
(Saros 119)
Saros120 67van71 SE2123May25P.jpg
May 25, 2123
(Saros 120)
Saros121 68van71 SE2152May04P.jpg
May 4, 2152
(Saros 121)
Saros122 67van70 SE2181Apr14P.jpg
April 14, 2181
(Saros 122)

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References

  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.