Solar eclipse of January 3, 1946

Last updated
Solar eclipse of January 3, 1946
SE1946Jan03P.png
Map
Type of eclipse
NaturePartial
Gamma −1.2392
Magnitude 0.5529
Maximum eclipse
Coordinates 67°06′S177°36′E / 67.1°S 177.6°E / -67.1; 177.6
Times (UTC)
Greatest eclipse12:16:11
References
Saros 150 (13 of 71)
Catalog # (SE5000) 9388

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.

Contents

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
EventTime (UTC)
First Penumbral External Contact1946 January 03 at 10:25:50.6 UTC
Greatest Eclipse1946 January 03 at 12:16:10.7 UTC
Equatorial Conjunction1946 January 03 at 12:16:37.9 UTC
Ecliptic Conjunction1946 January 03 at 12:30:05.5 UTC
Last Penumbral External Contact1946 January 03 at 14:06:25.7 UTC
January 3, 1946 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.55294
Eclipse Obscuration0.43993
Gamma−1.23918
Sun Right Ascension18h54m29.6s
Sun Declination-22°51'18.5"
Sun Semi-Diameter16'15.9"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension18h54m28.6s
Moon Declination-23°59'55.4"
Moon Semi-Diameter15'07.7"
Moon Equatorial Horizontal Parallax0°55'31.2"
ΔT27.3 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 1945–January 1946
December 19
Ascending node (full moon)
January 3
Descending node (new moon)
Lunar eclipse chart close-1945Dec19.png SE1946Jan03P.png
Total lunar eclipse
Lunar Saros 124
Partial solar eclipse
Solar Saros 150

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
SarosMapGammaSarosMapGamma
115 August 12, 1942
SE1942Aug12P.png
Partial
−1.5244120 February 4, 1943
SE1943Feb04T.png
Total
0.8734
125 August 1, 1943
SE1943Aug01A.png
Annular
−0.8041130 January 25, 1944
SE1944Jan25T.png
Total
0.2025
135 July 20, 1944
SE1944Jul20A.png
Annular
−0.0314140 January 14, 1945
SE1945Jan14A.png
Annular
−0.4937
145 July 9, 1945
1945Jul09T.png
Total
0.7356150 January 3, 1946
SE1946Jan03P.png
Partial
−1.2392
155 June 29, 1946
SE1946Jun29P.png
Partial
1.4361

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 16, 1866 and August 9, 1953
March 16–17January 1–3October 20–22August 9–10May 27–29
108110112114116
SE1866Mar16P.gif
March 16, 1866
SE1877Aug09P.gif
August 9, 1877
SE1881May27P.gif
May 27, 1881
118120122124126
SE1885Mar16A.gif
March 16, 1885
SE1889Jan01T.png
January 1, 1889
SE1892Oct20P.gif
October 20, 1892
SE1896Aug09T.png
August 9, 1896
SE1900May28T.png
May 28, 1900
128130132134136
SE1904Mar17A.png
March 17, 1904
SE1908Jan03T.png
January 3, 1908
SE1911Oct22A.png
October 22, 1911
SE1915Aug10A.png
August 10, 1915
SE1919May29T.png
May 29, 1919
138140142144146
SE1923Mar17A.png
March 17, 1923
SE1927Jan03A.png
January 3, 1927
SE1930Oct21T.png
October 21, 1930
SE1934Aug10A.png
August 10, 1934
SE1938May29T.png
May 29, 1938
148150152154
SE1942Mar16P.png
March 16, 1942
SE1946Jan03P.png
January 3, 1946
SE1949Oct21P.png
October 21, 1949
SE1953Aug09P.png
August 9, 1953

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 October 24, 2098 (part of Saros 164) is also a part of this series but is not included in the table below.

Series members between 1801 and 2011
SE1804Feb11H.png
February 11, 1804
(Saros 137)
SE1815Jan10A.png
January 10, 1815
(Saros 138)
SE1825Dec09H.png
December 9, 1825
(Saros 139)
SE1836Nov09T.png
November 9, 1836
(Saros 140)
SE1847Oct09A.png
October 9, 1847
(Saros 141)
SE1858Sep07T.png
September 7, 1858
(Saros 142)
SE1869Aug07T.png
August 7, 1869
(Saros 143)
SE1880Jul07A.png
July 7, 1880
(Saros 144)
SE1891Jun06A.png
June 6, 1891
(Saros 145)
SE1902May07P.png
May 7, 1902
(Saros 146)
SE1913Apr06P.png
April 6, 1913
(Saros 147)
SE1924Mar05P.png
March 5, 1924
(Saros 148)
SE1935Feb03P.png
February 3, 1935
(Saros 149)
SE1946Jan03P.png
January 3, 1946
(Saros 150)
SE1956Dec02P.png
December 2, 1956
(Saros 151)
SE1967Nov02T.png
November 2, 1967
(Saros 152)
SE1978Oct02P.png
October 2, 1978
(Saros 153)
SE1989Aug31P.png
August 31, 1989
(Saros 154)
SE2000Jul31P.png
July 31, 2000
(Saros 155)
SE2011Jul01P.png
July 1, 2011
(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
SE1801Apr13P.png
April 13, 1801
(Saros 145)
SE1830Mar24P.gif
March 24, 1830
(Saros 146)
SE1859Mar04P.gif
March 4, 1859
(Saros 147)
SE1888Feb11P.gif
February 11, 1888
(Saros 148)
SE1917Jan23P.png
January 23, 1917
(Saros 149)
SE1946Jan03P.png
January 3, 1946
(Saros 150)
SE1974Dec13P.png
December 13, 1974
(Saros 151)
SE2003Nov23T.png
November 23, 2003
(Saros 152)
SE2032Nov03P.png
November 3, 2032
(Saros 153)
SE2061Oct13A.png
October 13, 2061
(Saros 154)
SE2090Sep23T.png
September 23, 2090
(Saros 155)
Saros156 07van69 SE2119Sep05P.jpg
September 5, 2119
(Saros 156)
Saros157 06van70 SE2148Aug14P.jpg
August 14, 2148
(Saros 157)
Saros158 07van70 SE2177Jul25P.jpg
July 25, 2177
(Saros 158)

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References

  1. "January 3, 1946 Partial Solar Eclipse". timeanddate. Retrieved 4 August 2024.
  2. "Partial Solar Eclipse of 1946 Jan 03". EclipseWise.com. Retrieved 4 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.