Solar eclipse of February 14, 1953

Last updated
Solar eclipse of February 14, 1953
SE1953Feb14P.png
Map
Type of eclipse
NaturePartial
Gamma 1.1331
Magnitude 0.7596
Maximum eclipse
Coordinates 61°54′N104°54′E / 61.9°N 104.9°E / 61.9; 104.9
Times (UTC)
Greatest eclipse0:59:30
References
Saros 149 (17 of 71)
Catalog # (SE5000) 9404

A partial solar eclipse occurred at the Moon's ascending node of orbit between Friday, February 13 and Saturday, February 14, 1953, [1] with a magnitude of 0.7596. 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

A partial eclipse was visible for parts of East Asia, Northeast Asia, and Alaska.

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]

February 14, 1953 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact1953 February 13 at 23:12:27.3 UTC
Greatest Eclipse1953 February 14 at 00:59:29.8 UTC
Ecliptic Conjunction1953 February 14 at 01:10:45.7 UTC
Equatorial Conjunction1953 February 14 at 01:54:08.7 UTC
Last Penumbral External Contact1953 February 14 at 02:46:08.9 UTC
February 14, 1953 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.75964
Eclipse Obscuration0.70380
Gamma1.13308
Sun Right Ascension21h49m19.4s
Sun Declination-13°10'35.4"
Sun Semi-Diameter16'11.6"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension21h47m19.1s
Moon Declination-12°07'43.4"
Moon Semi-Diameter16'43.4"
Moon Equatorial Horizontal Parallax1°01'22.7"
ΔT30.4 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 January–February 1953
January 29
Descending node (full moon)
February 14
Ascending node (new moon)
Lunar eclipse chart close-1953Jan29.png SE1953Feb14P.png
Total lunar eclipse
Lunar Saros 123
Partial solar eclipse
Solar Saros 149

Eclipses in 1953

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 149

Inex

Triad

Solar eclipses of 1950–1953

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 eclipse on July 11, 1953 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 1950 to 1953
Ascending node Descending node
SarosMapGammaSarosMapGamma
119 March 18, 1950
SE1950Mar18A.png
Annular (non-central)
0.9988124 September 12, 1950
SE1950Sep12T.png
Total
0.8903
129 March 7, 1951
SE1951Mar07A.png
Annular
−0.242134 September 1, 1951
SE1951Sep01A.png
Annular
0.1557
139 February 25, 1952
SE1952Feb25T.png
Total
0.4697144 August 20, 1952
SE1952Aug20A.png
Annular
−0.6102
149 February 14, 1953
SE1953Feb14P.png
Partial
1.1331154 August 9, 1953
SE1953Aug09P.png
Partial
−1.344

Saros 149

This eclipse is a part of Saros series 149, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on August 21, 1664. It contains total eclipses from April 9, 2043 through October 2, 2331; hybrid eclipses from October 13, 2349 through November 3, 2385; and annular eclipses from November 15, 2403 through July 13, 2800. The series ends at member 71 as a partial eclipse on September 28, 2926. 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 will be produced by member 31 at 4 minutes, 10 seconds on July 17, 2205, and the longest duration of annularity will be produced by member 62 at 5 minutes, 6 seconds on June 21, 2764. All eclipses in this series occur at the Moon’s ascending node of orbit. [4]

Series members 9–30 occur between 1801 and 2200:
91011
SE1808Nov18P.gif
November 18, 1808
SE1826Nov29P.gif
November 29, 1826
SE1844Dec09P.gif
December 9, 1844
121314
SE1862Dec21P.gif
December 21, 1862
SE1880Dec31P.gif
December 31, 1880
SE1899Jan11P.gif
January 11, 1899
151617
SE1917Jan23P.png
January 23, 1917
SE1935Feb03P.png
February 3, 1935
SE1953Feb14P.png
February 14, 1953
181920
SE1971Feb25P.png
February 25, 1971
SE1989Mar07P.png
March 7, 1989
SE2007Mar19P.png
March 19, 2007
212223
SE2025Mar29P.png
March 29, 2025
SE2043Apr09T.png
April 9, 2043
SE2061Apr20T.png
April 20, 2061
242526
SE2079May01T.png
May 1, 2079
SE2097May11T.png
May 11, 2097
SE2115May24T.png
May 24, 2115
272829
SE2133Jun03T.png
June 3, 2133
Saros149 28van71 SE2151Jun14T.jpg
June 14, 2151
SE2169Jun25T.png
June 25, 2169
30
Saros149 30van71 SE2187Jul06T.jpg
July 6, 2187

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 ascending node.

22 eclipse events between December 2, 1880 and July 9, 1964
December 2–3September 20–21July 9–10April 26–28February 13–14
111113115117119
SE1880Dec02P.gif
December 2, 1880
SE1888Jul09P.gif
July 9, 1888
SE1892Apr26T.gif
April 26, 1892
SE1896Feb13A.png
February 13, 1896
121123125127129
SE1899Dec03A.gif
December 3, 1899
SE1903Sep21T.png
September 21, 1903
SE1907Jul10A.png
July 10, 1907
SE1911Apr28T.png
April 28, 1911
SE1915Feb14A.png
February 14, 1915
131133135137139
SE1918Dec03A.png
December 3, 1918
SE1922Sep21T.png
September 21, 1922
SE1926Jul09A.png
July 9, 1926
SE1930Apr28H.png
April 28, 1930
SE1934Feb14T.png
February 14, 1934
141143145147149
SE1937Dec02A.png
December 2, 1937
SE1941Sep21T.png
September 21, 1941
SE1945Jul09T.png
July 9, 1945
SE1949Apr28P.png
April 28, 1949
SE1953Feb14P.png
February 14, 1953
151153155
SE1956Dec02P.png
December 2, 1956
SE1960Sep20P.png
September 20, 1960
SE1964Jul09P.png
July 9, 1964

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
SE1808May25P.gif
May 25, 1808
(Saros 144)
SE1837May04P.gif
May 4, 1837
(Saros 145)
SE1866Apr15P.gif
April 15, 1866
(Saros 146)
SE1895Mar26P.gif
March 26, 1895
(Saros 147)
SE1924Mar05P.png
March 5, 1924
(Saros 148)
SE1953Feb14P.png
February 14, 1953
(Saros 149)
SE1982Jan25P.png
January 24, 1982
(Saros 150)
SE2011Jan04P.png
January 4, 2011
(Saros 151)
SE2039Dec15T.png
December 15, 2039
(Saros 152)
SE2068Nov24P.png
November 24, 2068
(Saros 153)
SE2097Nov04A.png
November 4, 2097
(Saros 154)
Saros155 12van71 SE2126Oct16T.jpg
October 16, 2126
(Saros 155)
Saros156 09van69 SE2155Sep26A.jpg
September 26, 2155
(Saros 156)
Saros157 08van70 SE2184Sep04A.jpg
September 4, 2184
(Saros 157)

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References

  1. "February 13–14, 1953 Partial Solar Eclipse". timeanddate. Retrieved 5 August 2024.
  2. "Partial Solar Eclipse of 1953 Feb 14". EclipseWise.com. Retrieved 5 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 149". eclipse.gsfc.nasa.gov.