Solar eclipse of February 14, 1953

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Template:Short description Script error: No such module "Solar eclipse". 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.

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

In Asia, the date of the eclipse, February 14, was the exact day of the Lunar New Year, celebrated in multiple countries.

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
Event Time (UTC)
First Penumbral External Contact 1953 February 13 at 23:12:27.3 UTC
Greatest Eclipse 1953 February 14 at 00:59:29.8 UTC
Ecliptic Conjunction 1953 February 14 at 01:10:45.7 UTC
Equatorial Conjunction 1953 February 14 at 01:54:08.7 UTC
Last Penumbral External Contact 1953 February 14 at 02:46:08.9 UTC
February 14, 1953 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.75964
Eclipse Obscuration 0.70380
Gamma 1.13308
Sun Right Ascension 21h49m19.4s
Sun Declination -13°10'35.4"
Sun Semi-Diameter 16'11.6"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 21h47m19.1s
Moon Declination -12°07'43.4"
Moon Semi-Diameter 16'43.4"
Moon Equatorial Horizontal Parallax 1°01'22.7"
ΔT 30.4 s

Eclipse season

Script error: No such module "Labelled list hatnote". 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)
File:Lunar eclipse chart close-1953Jan29.png File:SE1953Feb14P.png
Total lunar eclipse
Lunar Saros 123
Partial solar eclipse
Solar Saros 149

Related eclipses

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
Saros Map Gamma Saros Map Gamma
119 March 18, 1950
File:SE1950Mar18A.png
Annular (non-central)
0.9988 124 September 12, 1950
File:SE1950Sep12T.png
Total
0.8903
129 March 7, 1951
File:SE1951Mar07A.png
Annular
−0.242 134 September 1, 1951
File:SE1951Sep01A.png
Annular
0.1557
139 February 25, 1952
File:SE1952Feb25T.png
Total
0.4697 144 August 20, 1952
File:SE1952Aug20A.png
Annular
−0.6102
149 February 14, 1953
File:SE1953Feb14P.png
Partial
1.1331 154 August 9, 1953
File:SE1953Aug09P.png
Partial
−1.344

Saros 149

Template:Solar Saros series 149

Metonic series

Template:Solar Metonic series 1880–1964

Tritos series

Template:Solar Tritos series 2007 September 11

Inex series

Template:Solar Inex series 2011 January 4

References

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External links

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