Solar eclipse of January 14, 1964

Last updated
Solar eclipse of January 14, 1964
SE1964Jan14P.png
Map
Type of eclipse
NaturePartial
Gamma −1.2354
Magnitude 0.5591
Maximum eclipse
Coordinates 68°12′S43°06′E / 68.2°S 43.1°E / -68.2; 43.1
Times (UTC)
Greatest eclipse20:30:08
References
Saros 150 (14 of 71)
Catalog # (SE5000) 9428

A partial solar eclipse occurred at the Moon's descending node of orbit on Tuesday, January 14, 1964, [1] with a magnitude of 0.5591. 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. Partial solar eclipses occur in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

Contents

This was the first of four partial solar eclipses in 1964, with the others occurring on June 10, July 9, and December 4.

A partial eclipse was visible for parts of Antarctica and extreme southern South America.

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]

January 14, 1964 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact1964 January 14 at 18:38:52.1 UTC
Equatorial Conjunction1964 January 14 at 20:19:20.3 UTC
Greatest Eclipse1964 January 14 at 20:30:08.2 UTC
Ecliptic Conjunction1964 January 14 at 20:44:03.6 UTC
Last Penumbral External Contact1964 January 14 at 22:21:24.3 UTC
January 14, 1964 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.55916
Eclipse Obscuration0.44651
Gamma−1.23541
Sun Right Ascension19h42m19.5s
Sun Declination-21°21'43.0"
Sun Semi-Diameter16'15.6"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension19h42m41.8s
Moon Declination-22°29'45.9"
Moon Semi-Diameter15'05.5"
Moon Equatorial Horizontal Parallax0°55'23.3"
ΔT35.1 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.

Eclipse season of December 1963–January 1964
December 30
Ascending node (full moon)
January 14
Descending node (new moon)
Lunar eclipse chart close-1963Dec30.png SE1964Jan14P.png
Total lunar eclipse
Lunar Saros 124
Partial solar eclipse
Solar Saros 150

Eclipses in 1964

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 150

Inex

Triad

Solar eclipses of 1961–1964

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 June 10, 1964 and December 4, 1964 occur in the next lunar year eclipse set.

Solar eclipse series sets from 1961 to 1964
Descending node Ascending node
SarosMapGammaSarosMapGamma
120
1961 Total Solar Eclipse.jpg
February 15, 1961
SE1961Feb15T.png
Total
0.883125 August 11, 1961
SE1961Aug11A.png
Annular
−0.8859
130 February 5, 1962
SE1962Feb05T.png
Total
0.2107135 July 31, 1962
SE1962Jul31A.png
Annular
−0.113
140 January 25, 1963
SE1963Jan25A.png
Annular
−0.4898145 July 20, 1963
SE1963Jul20T.png
Total
0.6571
150 January 14, 1964
SE1964Jan14P.png
Partial
−1.2354155 July 9, 1964
SE1964Jul09P.png
Partial
1.3623

Saros 150

This eclipse is a part of Saros series 150, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on August 24, 1729. It contains annular eclipses from April 22, 2126 through June 22, 2829. There are no hybrid or total eclipses in this set. The series ends at member 71 as a partial eclipse on September 29, 2991. 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 45 at 9 minutes, 58 seconds on December 19, 2522. All eclipses in this series occur at the Moon’s descending node of orbit. [4]

Series members 5–27 occur between 1801 and 2200:
567
SE1801Oct07P.png
October 7, 1801
SE1819Oct19P.gif
October 19, 1819
SE1837Oct29P.gif
October 29, 1837
8910
SE1855Nov09P.gif
November 9, 1855
SE1873Nov20P.gif
November 20, 1873
SE1891Dec01P.gif
December 1, 1891
111213
SE1909Dec12P.png
December 12, 1909
SE1927Dec24P.png
December 24, 1927
SE1946Jan03P.png
January 3, 1946
141516
SE1964Jan14P.png
January 14, 1964
SE1982Jan25P.png
January 25, 1982
SE2000Feb05P.png
February 5, 2000
171819
SE2018Feb15P.png
February 15, 2018
SE2036Feb27P.png
February 27, 2036
SE2054Mar09P.png
March 9, 2054
202122
SE2072Mar19P.png
March 19, 2072
SE2090Mar31P.png
March 31, 2090
SE2108Apr11P.gif
April 11, 2108
232425
Saros150 23van71 SE2126Apr22A.jpg
April 22, 2126
Saros150 24van71 SE2144May03A.jpg
May 3, 2144
Saros150 25van71 SE2162May14A.jpg
May 14, 2162
2627
Saros150 26van71 SE2180May24A.jpg
May 24, 2180
Saros150 27van71 SE2198Jun04A.jpg
June 4, 2198

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 March 27, 1884 and August 20, 1971
March 27–29January 14November 1–2August 20–21June 8
108110112114116
SE1884Mar27P.gif
March 27, 1884
SE1895Aug20P.gif
August 20, 1895
SE1899Jun08P.gif
June 8, 1899
118120122124126
SE1903Mar29A.png
March 29, 1903
SE1907Jan14T.png
January 14, 1907
SE1910Nov02P.png
November 2, 1910
SE1914Aug21T.png
August 21, 1914
SE1918Jun08T.png
June 8, 1918
128130132134136
SE1922Mar28A.png
March 28, 1922
SE1926Jan14T.png
January 14, 1926
SE1929Nov01A.png
November 1, 1929
SE1933Aug21A.png
August 21, 1933
SE1918Jun08T.png
June 8, 1937
138140142144146
SE1941Mar27A.png
March 27, 1941
SE1945Jan14A.png
January 14, 1945
SE1948Nov01T.png
November 1, 1948
SE1952Aug20A.png
August 20, 1952
SE1956Jun08T.png
June 8, 1956
148150152154
SE1960Mar27P.png
March 27, 1960
SE1964Jan14P.png
January 14, 1964
SE1967Nov02T.png
November 2, 1967
SE1971Aug20P.png
August 20, 1971

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.

The partial solar eclipse on November 4, 2116 (part of Saros 164) is also a part of this series but is not included in the table below.

Series members between 1801 and 2029
SE1811Mar24T.gif
March 24, 1811
(Saros 136)
SE1822Feb21A.gif
February 21, 1822
(Saros 137)
SE1833Jan20A.gif
January 20, 1833
(Saros 138)
SE1843Dec21T.gif
December 21, 1843
(Saros 139)
SE1854Nov20H.png
November 20, 1854
(Saros 140)
SE1865Oct19A.png
October 19, 1865
(Saros 141)
SE1876Sep17T.gif
September 17, 1876
(Saros 142)
SE1887Aug19T.png
August 19, 1887
(Saros 143)
SE1898Jul18A.gif
July 18, 1898
(Saros 144)
SE1909Jun17H.png
June 17, 1909
(Saros 145)
SE1920May18P.png
May 18, 1920
(Saros 146)
SE1931Apr18P.png
April 18, 1931
(Saros 147)
SE1942Mar16P.png
March 16, 1942
(Saros 148)
SE1953Feb14P.png
February 14, 1953
(Saros 149)
SE1964Jan14P.png
January 14, 1964
(Saros 150)
SE1974Dec13P.png
December 13, 1974
(Saros 151)
SE1985Nov12T.png
November 12, 1985
(Saros 152)
SE1996Oct12P.png
October 12, 1996
(Saros 153)
SE2007Sep11P.png
September 11, 2007
(Saros 154)
SE2018Aug11P.png
August 11, 2018
(Saros 155)
SE2029Jul11P.png
July 11, 2029
(Saros 156)

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
SE1819Apr24P.png
April 24, 1819
(Saros 145)
SE1848Apr03P.png
April 3, 1848
(Saros 146)
SE1877Mar15P.gif
March 15, 1877
(Saros 147)
SE1906Feb23P.png
February 23, 1906
(Saros 148)
SE1935Feb03P.png
February 3, 1935
(Saros 149)
SE1964Jan14P.png
January 14, 1964
(Saros 150)
SE1992Dec24P.png
December 24, 1992
(Saros 151)
SE2021Dec04T.png
December 4, 2021
(Saros 152)
SE2050Nov14P.png
November 14, 2050
(Saros 153)
SE2079Oct24A.png
October 24, 2079
(Saros 154)
Saros155 11van71 SE2108Oct05T.jpg
October 5, 2108
(Saros 155)
Saros156 08van69 SE2137Sep15P.jpg
September 15, 2137
(Saros 156)
Saros157 07van70 SE2166Aug25A.jpg
August 25, 2166
(Saros 157)
Saros158 08van70 SE2195Aug05T.jpg
August 5, 2195
(Saros 158)

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References

  1. "January 14, 1964 Partial Solar Eclipse". timeanddate. Retrieved 7 August 2024.
  2. "Partial Solar Eclipse of 1964 Jan 14". EclipseWise.com. Retrieved 7 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 150". eclipse.gsfc.nasa.gov.