Solar eclipse of March 16, 1942

Last updated
Solar eclipse of March 16, 1942
SE1942Mar16P.png
Map
Type of eclipse
NaturePartial
Gamma −1.1908
Magnitude 0.6393
Maximum eclipse
Coordinates 72°12′S76°48′W / 72.2°S 76.8°W / -72.2; -76.8
Times (UTC)
Greatest eclipse23:37:07
References
Saros 148 (17 of 75)
Catalog # (SE5000) 9379

A partial solar eclipse occurred at the Moon's descending node of orbit between Monday, March 16 and Tuesday, March 17, 1942, [1] with a magnitude of 0.6393. 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 Antarctica and southern Oceania.

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]

March 16, 1942 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact1942 March 16 at 21:44:48.6 UTC
Equatorial Conjunction1942 March 16 at 22:54:14.8 UTC
Greatest Eclipse1942 March 16 at 23:37:06.8 UTC
Ecliptic Conjunction1942 March 16 at 23:50:18.2 UTC
Last Penumbral External Contact1942 March 17 at 01:29:50.5 UTC
March 16, 1942 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.63936
Eclipse Obscuration0.54379
Gamma−1.19082
Sun Right Ascension23h44m24.0s
Sun Declination-01°41'22.1"
Sun Semi-Diameter16'04.3"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension23h45m46.3s
Moon Declination-02°45'29.1"
Moon Semi-Diameter15'26.7"
Moon Equatorial Horizontal Parallax0°56'41.2"
ΔT25.4 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 March 1942
March 3
Ascending node (full moon)
March 16
Descending node (new moon)
Lunar eclipse chart close-1942Mar03.png SE1942Mar16P.png
Total lunar eclipse
Lunar Saros 122
Partial solar eclipse
Solar Saros 148

Eclipses in 1942

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 148

Inex

Triad

Solar eclipses of 1939–1942

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 August 12, 1942 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 1939 to 1942
Descending node Ascending node
SarosMapGammaSarosMapGamma
118 April 19, 1939
SE1939Apr19A.png
Annular
0.9388123 October 12, 1939
SE1939Oct12T.png
Total
−0.9737
128 April 7, 1940
SE1940Apr07A.png
Annular
0.219133 October 1, 1940
SE1940Oct01T.png
Total
−0.2573
138 March 27, 1941
SE1941Mar27A.png
Annular
−0.5025143 September 21, 1941
SE1941Sep21T.png
Total
0.4649
148 March 16, 1942
SE1942Mar16P.png
Partial
−1.1908153 September 10, 1942
SE1942Sep10P.png
Partial
1.2571

Saros 148

This eclipse is a part of Saros series 148, repeating every 18 years, 11 days, and containing 75 events. The series started with a partial solar eclipse on September 21, 1653. It contains annular eclipses on April 29, 2014 and May 9, 2032; a hybrid eclipse on May 20, 2050; and total eclipses from May 31, 2068 through August 3, 2771. The series ends at member 75 as a partial eclipse on December 12, 2987. 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 22 at 22 seconds (by default) on May 9, 2032, and the longest duration of totality will be produced by member 54 at 5 minutes, 23 seconds on April 26, 2609. All eclipses in this series occur at the Moon’s descending node of orbit. [4]

Series members 10–31 occur between 1801 and 2200:
101112
SE1815Dec30P.gif
December 30, 1815
SE1834Jan09P.gif
January 9, 1834
SE1852Jan21P.gif
January 21, 1852
131415
SE1870Jan31P.gif
January 31, 1870
SE1888Feb11P.gif
February 11, 1888
SE1906Feb23P.png
February 23, 1906
161718
SE1924Mar05P.png
March 5, 1924
SE1942Mar16P.png
March 16, 1942
SE1960Mar27P.png
March 27, 1960
192021
SE1978Apr07P.png
April 7, 1978
SE1996Apr17P.png
April 17, 1996
SE2014Apr29A.png
April 29, 2014
222324
SE2032May09A.png
May 9, 2032
SE2050May20H.png
May 20, 2050
SE2068May31T.png
May 31, 2068
252627
SE2086Jun11T.png
June 11, 2086
Saros148 26van75 SE2104Jun22T.jpg
June 22, 2104
Saros148 27van75 SE2122Jul04T.jpg
July 4, 2122
282930
Saros148 28van75 SE2140Jul14T.jpg
July 14, 2140
SE2158Jul25T.png
July 25, 2158
Saros148 30van75 SE2176Aug04T.jpg
August 4, 2176
31
Saros148 31van75 SE2194Aug16T.jpg
August 16, 2194

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 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
SE1826Jun05P.gif
June 5, 1826
(Saros 144)
SE1855May16P.gif
May 16, 1855
(Saros 145)
SE1884Apr25P.gif
April 25, 1884
(Saros 146)
SE1913Apr06P.png
April 6, 1913
(Saros 147)
SE1942Mar16P.png
March 16, 1942
(Saros 148)
SE1971Feb25P.png
February 25, 1971
(Saros 149)
SE2000Feb05P.png
February 5, 2000
(Saros 150)
SE2029Jan14P.png
January 14, 2029
(Saros 151)
SE2057Dec26T.png
December 26, 2057
(Saros 152)
SE2086Dec06P.png
December 6, 2086
(Saros 153)
Saros154 12van71 SE2115Nov16A.jpg
November 16, 2115
(Saros 154)
Saros155 13van71 SE2144Oct26T.jpg
October 26, 2144
(Saros 155)
Saros156 10van69 SE2173Oct07A.jpg
October 7, 2173
(Saros 156)

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References

  1. "March 16–17, 1942 Partial Solar Eclipse". timeanddate. Retrieved 4 August 2024.
  2. "Partial Solar Eclipse of 1942 Mar 16". 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 148". eclipse.gsfc.nasa.gov.