Solar eclipse of January 3, 1946

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Template:Short description Script error: No such module "Solar eclipse". A partial solar eclipse occurred at the Moon's descending node of orbit on Thursday, January 3, 1946,[1] with a magnitude of 0.5529. 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 first of four partial solar eclipses in 1946, with the others occurring on May 30, June 29, and November 23.

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 3, 1946 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 1946 January 3 at 10:25:50.6 UTC
Greatest Eclipse 1946 January 3 at 12:16:10.7 UTC
Equatorial Conjunction 1946 January 3 at 12:16:37.9 UTC
Ecliptic Conjunction 1946 January 3 at 12:30:05.5 UTC
Last Penumbral External Contact 1946 January 3 at 14:06:25.7 UTC
January 3, 1946 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.55294
Eclipse Obscuration 0.43993
Gamma −1.23918
Sun Right Ascension 18h54m29.6s
Sun Declination -22°51'18.5"
Sun Semi-Diameter 16'15.9"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 18h54m28.6s
Moon Declination -23°59'55.4"
Moon Semi-Diameter 15'07.7"
Moon Equatorial Horizontal Parallax 0°55'31.2"
ΔT 27.3 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 December 1945–January 1946
December 19
Ascending node (full moon)
January 3
Descending node (new moon)
File:Lunar eclipse chart close-1945Dec19.png File:SE1946Jan03P.png
Total lunar eclipse
Lunar Saros 124
Partial solar eclipse
Solar Saros 150

Related eclipses

Eclipses in 1946

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 150

Inex

Triad

Solar eclipses of 1942–1946

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 March 16, 1942 and September 10, 1942 occur in the previous lunar year eclipse set, and the partial solar eclipses on May 30, 1946 and November 23, 1946 occur in the next lunar year eclipse set.

Solar eclipse series sets from 1942 to 1946
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
115 August 12, 1942
File:SE1942Aug12P.png
Partial
−1.5244 120 February 4, 1943
File:SE1943Feb04T.png
Total
0.8734
125 August 1, 1943
File:SE1943Aug01A.png
Annular
−0.8041 130 January 25, 1944
File:SE1944Jan25T.png
Total
0.2025
135 July 20, 1944
File:SE1944Jul20A.png
Annular
−0.0314 140 January 14, 1945
File:SE1945Jan14A.png
Annular
−0.4937
145 July 9, 1945
File:1945Jul09T.png
Total
0.7356 150 January 3, 1946
File:SE1946Jan03P.png
Partial
−1.2392
155 June 29, 1946
File:SE1946Jun29P.png
Partial
1.4361

Saros 150

Template:Solar Saros series 150

Metonic series

Template:Solar Metonic series 1866–1953

Tritos series

Template:Solar Tritos series 2000 July 31

Inex series

Template:Solar Inex series 2003 November 23

References

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External links


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