Solar eclipse of June 10, 1964

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Solar eclipse of June 10, 1964
Partial eclipse
Gamma−1.1393
Magnitude0.7545
Maximum eclipse
CoordinatesLua error: callParserFunction: function "#coordinates" was not found.
Times (UTC)
Greatest eclipse4:34:07
References
Saros117 (66 of 71)
Catalog # (SE5000)9430

A partial solar eclipse occurred at the Moon's ascending node of orbit on Wednesday, June 10, 1964,[1] with a magnitude of 0.7545. 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 was the second of four partial solar eclipses in 1964, with the others occurring on January 14, July 9, and December 4.

A partial eclipse was visible for parts of Australia and western Oceania.

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]

June 10, 1964 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 1964 June 10 at 02:49:28.6 UTC
Equatorial Conjunction 1964 June 10 at 04:13:17.5 UTC
Ecliptic Conjunction 1964 June 10 at 04:22:52.0 UTC
Greatest Eclipse 1964 June 10 at 04:34:07.0 UTC
Last Penumbral External Contact 1964 June 10 at 06:18:54.5 UTC
June 10, 1964 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.75455
Eclipse Obscuration 0.70285
Gamma −1.13926
Sun Right Ascension 05h13m32.2s
Sun Declination +23°00'50.0"
Sun Semi-Diameter 15'45.1"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 05h14m24.9s
Moon Declination +21°52'09.4"
Moon Semi-Diameter 16'43.2"
Moon Equatorial Horizontal Parallax 1°01'21.8"
ΔT 35.3 s

Eclipse season

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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 June–July 1964
June 10
Ascending node (new moon)
June 25
Descending node (full moon)
July 9
Ascending node (new moon)
File:SE1964Jun10P.png File:Lunar eclipse chart close-1964Jun25.png File:SE1964Jul09P.png
Partial solar eclipse
Solar Saros 117
Total lunar eclipse
Lunar Saros 129
Partial solar eclipse
Solar Saros 155
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Eclipses in 1964

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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 117

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Triad

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Solar eclipses of 1964–1967

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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 January 14, 1964 and July 9, 1964 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 1964 to 1967
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
117 June 10, 1964
File:SE1964Jun10P.png
Partial
−1.1393 122 December 4, 1964
File:SE1964Dec04P.png
Partial
1.1193
127 May 30, 1965
File:SE1965May30T.png
Total
−0.4225 132 November 23, 1965
File:SE1965Nov23A.png
Annular
0.3906
137 May 20, 1966
File:SE1966May20A.png
Annular
0.3467 142 November 12, 1966
File:SE1966Nov12T.png
Total
−0.33
147 May 9, 1967
File:SE1967May09P.png
Partial
1.1422 152 November 2, 1967
File:SE1967Nov02T.png
Total (non-central)
1.0007

Saros 117

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This eclipse is a part of Saros series 117, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on June 24, 792 AD. It contains annular eclipses from September 18, 936 AD through May 14, 1333; hybrid eclipses from May 25, 1351 through July 8, 1423; and total eclipses from July 18, 1441 through May 19, 1928. The series ends at member 71 as a partial eclipse on August 3, 2054. 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 was produced by member 16 at 9 minutes, 26 seconds on December 3, 1062, and the longest duration of totality was produced by member 62 at 4 minutes, 19 seconds on April 26, 1892. All eclipses in this series occur at the Moon’s ascending 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 ascending node.

20 eclipse events between June 10, 1964 and August 21, 2036
June 10–11 March 28–29 January 14–16 November 3 August 21–22
117 119 121 123 125
File:SE1964Jun10P.png
June 10, 1964
File:SE1968Mar28P.png
March 28, 1968
File:SE1972Jan16A.png
January 16, 1972
File:SE1975Nov03P.png
November 3, 1975
File:SE1979Aug22A.png
August 22, 1979
127 129 131 133 135
File:SE1983Jun11T.png
June 11, 1983
File:SE1987Mar29H.png
March 29, 1987
File:SE1991Jan15A.png
January 15, 1991
File:SE1994Nov03T.png
November 3, 1994
File:SE1998Aug22A.png
August 22, 1998
137 139 141 143 145
File:SE2002Jun10A.png
June 10, 2002
File:SE2006Mar29T.png
March 29, 2006
File:SE2010Jan15A.png
January 15, 2010
File:SE2013Nov03H.png
November 3, 2013
File:SE2017Aug21T.png
August 21, 2017
147 149 151 153 155
File:SE2021Jun10A.png
June 10, 2021
File:SE2025Mar29P.png
March 29, 2025
File:SE2029Jan14P.png
January 14, 2029
File:SE2032Nov03P.png
November 3, 2032
File:SE2036Aug21P.png
August 21, 2036

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 1866 and 2200
File:SE1866Mar16P.gif
March 16, 1866
(Saros 108)
File:SE1898Dec13P.gif
December 13, 1898
(Saros 111)
File:SE1931Sep12P.png
September 12, 1931
(Saros 114)
File:SE1942Aug12P.png
August 12, 1942
(Saros 115)
File:SE1953Jul11P.png
July 11, 1953
(Saros 116)
File:SE1964Jun10P.png
June 10, 1964
(Saros 117)
File:SE1975May11P.png
May 11, 1975
(Saros 118)
File:SE1986Apr09P.png
April 9, 1986
(Saros 119)
File:SE1997Mar09T.png
March 9, 1997
(Saros 120)
File:SE2008Feb07A.png
February 7, 2008
(Saros 121)
File:SE2019Jan06P.png
January 6, 2019
(Saros 122)
File:SE2029Dec05P.png
December 5, 2029
(Saros 123)
File:SE2040Nov04P.png
November 4, 2040
(Saros 124)
File:SE2051Oct04P.png
October 4, 2051
(Saros 125)
File:SE2062Sep03P.png
September 3, 2062
(Saros 126)
File:SE2073Aug03T.png
August 3, 2073
(Saros 127)
File:SE2084Jul03A.png
July 3, 2084
(Saros 128)
File:SE2095Jun02T.png
June 2, 2095
(Saros 129)
File:SE2106May03T.png
May 3, 2106
(Saros 130)
File:SE2117Apr02A.png
April 2, 2117
(Saros 131)
File:SE2128Mar01A.png
March 1, 2128
(Saros 132)
File:SE2139Jan30T.png
January 30, 2139
(Saros 133)
File:SE2149Dec30A.png
December 30, 2149
(Saros 134)
File:SE2160Nov27A.png
November 27, 2160
(Saros 135)
File:SE2171Oct29T.png
October 29, 2171
(Saros 136)
File:SE2182Sep27A.png
September 27, 2182
(Saros 137)
File:SE2193Aug26A.png
August 26, 2193
(Saros 138)

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.

Series members between 1801 and 2200
File:SE1819Sep19Pe.gif
September 19, 1819
(Saros 112)
File:SE1848Aug28P.gif
August 28, 1848
(Saros 113)
File:SE1877Aug09P.gif
August 9, 1877
(Saros 114)
File:SE1906Jul21P.png
July 21, 1906
(Saros 115)
File:SE1935Jun30P.png
June 30, 1935
(Saros 116)
File:SE1964Jun10P.png
June 10, 1964
(Saros 117)
File:SE1993May21P.png
May 21, 1993
(Saros 118)
File:SE2022Apr30P.png
April 30, 2022
(Saros 119)
File:SE2051Apr11P.png
April 11, 2051
(Saros 120)
File:SE2080Mar21P.png
March 21, 2080
(Saros 121)
File:Saros122 63van70 SE2109Mar01P.jpg
March 1, 2109
(Saros 122)
File:Saros123 60van70 SE2138Feb09P.jpg
February 9, 2138
(Saros 123)
File:Saros124 63van73 SE2167Jan21P.jpg
January 21, 2167
(Saros 124)
File:Saros125 64van73 SE2195Dec31P.jpg
December 31, 2195
(Saros 125)

References

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  1. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
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