Solar eclipse of June 29, 1946

Last updated
Solar eclipse of June 29, 1946
SE1946Jun29P.png
Map
Type of eclipse
NaturePartial
Gamma 1.4361
Magnitude 0.1802
Maximum eclipse
Coordinates 66°36′N50°48′W / 66.6°N 50.8°W / 66.6; -50.8
Times (UTC)
Greatest eclipse3:51:58
References
Saros 155 (2 of 71)
Catalog # (SE5000) 9389

A partial solar eclipse occurred at the Moon's ascending node of orbit on Saturday, June 29, 1946, [1] with a magnitude of 0.1802. 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 third of four partial solar eclipses in 1946, with the others occurring on January 3, May 30, and November 23.

A partial eclipse was visible for parts of Northern Europe, Greenland, and Canada.

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]

June 29, 1946 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact1946 June 29 at 02:57:15.1 UTC
Greatest Eclipse1946 June 29 at 03:51:57.7 UTC
Equatorial Conjunction1946 June 29 at 03:58:28.2 UTC
Ecliptic Conjunction1946 June 29 at 04:06:09.4 UTC
Last Penumbral External Contact1946 June 29 at 04:46:39.5 UTC
June 29, 1946 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.18018
Eclipse Obscuration0.09049
Gamma1.43612
Sun Right Ascension06h29m37.9s
Sun Declination+23°16'18.2"
Sun Semi-Diameter15'43.9"
Sun Equatorial Horizontal Parallax08.6"
Moon Right Ascension06h29m21.1s
Moon Declination+24°43'20.8"
Moon Semi-Diameter16'34.1"
Moon Equatorial Horizontal Parallax1°00'48.5"
ΔT27.5 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. The first and last eclipse in this sequence is separated by one synodic month.

Eclipse season of May–June 1946
May 30
Ascending node (new moon)
June 14
Descending node (full moon)
June 29
Ascending node (new moon)
SE1946May30P.png Lunar eclipse chart close-1946Jun14.png SE1946Jun29P.png
Partial solar eclipse
Solar Saros 117
Total lunar eclipse
Lunar Saros 129
Partial solar eclipse
Solar Saros 155

Eclipses in 1946

Metonic

Tzolkinex

Tritos

Solar Saros 155

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 155

This eclipse is a part of Saros series 155, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on June 17, 1928. It contains total eclipses from September 12, 2072 through August 30, 2649; hybrid eclipses from September 10, 2667 through October 2, 2703; and annular eclipses from October 13, 2721 through May 8, 3064. The series ends at member 71 as a partial eclipse on July 24, 3190. 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 14 at 4 minutes, 5 seconds on November 6, 2162, and the longest duration of annularity will be produced by member 63 at 5 minutes, 31 seconds on April 28, 3046. All eclipses in this series occur at the Moon’s ascending node of orbit. [4]

Series members 1–16 occur between 1928 and 2200:
123
SE1928Jun17P.png
June 17, 1928
SE1946Jun29P.png
June 29, 1946
SE1964Jul09P.png
July 9, 1964
456
SE1982Jul20P.png
July 20, 1982
SE2000Jul31P.png
July 31, 2000
SE2018Aug11P.png
August 11, 2018
789
SE2036Aug21P.png
August 21, 2036
SE2054Sep02P.png
September 2, 2054
SE2072Sep12T.png
September 12, 2072
101112
SE2090Sep23T.png
September 23, 2090
Saros155 11van71 SE2108Oct05T.jpg
October 5, 2108
Saros155 12van71 SE2126Oct16T.jpg
October 16, 2126
131415
Saros155 13van71 SE2144Oct26T.jpg
October 26, 2144
Saros155 14van71 SE2162Nov07T.jpg
November 7, 2162
Saros155 15van71 SE2180Nov17T.jpg
November 17, 2180
16
Saros155 16van71 SE2198Nov28T.jpg
November 28, 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 ascending node.

23 eclipse events between February 3, 1859 and June 29, 1946
February 1–3November 21–22September 8–10June 28–29April 16–18
109111113115117
SE1859Feb03P.png
February 3, 1859
SE1862Nov21P.gif
November 21, 1862
SE1870Jun28P.gif
June 28, 1870
SE1874Apr16T.gif
April 16, 1874
119121123125127
SE1878Feb02A.gif
February 2, 1878
SE1881Nov21A.gif
November 21, 1881
SE1885Sep08T.png
September 8, 1885
SE1889Jun28A.png
June 28, 1889
SE1893Apr16T.png
April 16, 1893
129131133135137
SE1897Feb01A.gif
February 1, 1897
SE1900Nov22A.gif
November 22, 1900
SE1904Sep09T.png
September 9, 1904
SE1908Jun28A.png
June 28, 1908
SE1912Apr17H.png
April 17, 1912
139141143145147
SE1916Feb03T.png
February 3, 1916
SE1919Nov22A.png
November 22, 1919
SE1923Sep10T.png
September 10, 1923
SE1927Jun29T.png
June 29, 1927
SE1931Apr18P.png
April 18, 1931
149151153155
SE1935Feb03P.png
February 3, 1935
SE1938Nov21P.png
November 21, 1938
SE1942Sep10P.png
September 10, 1942
SE1946Jun29P.png
June 29, 1946

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.

Series members between 1801 and 1946
SE1804Aug05T.gif
August 5, 1804
(Saros 142)
SE1815Jul06T.gif
July 6, 1815
(Saros 143)
SE1826Jun05P.gif
June 5, 1826
(Saros 144)
SE1837May04P.gif
May 4, 1837
(Saros 145)
SE1848Apr03P.png
April 3, 1848
(Saros 146)
SE1859Mar04P.gif
March 4, 1859
(Saros 147)
SE1870Jan31P.gif
January 31, 1870
(Saros 148)
SE1880Dec31P.gif
December 31, 1880
(Saros 149)
SE1891Dec01P.gif
December 1, 1891
(Saros 150)
SE1902Oct31P.png
October 31, 1902
(Saros 151)
SE1913Sep30P.png
September 30, 1913
(Saros 152)
SE1924Aug30P.png
August 30, 1924
(Saros 153)
SE1935Jul30P.png
July 30, 1935
(Saros 154)
SE1946Jun29P.png
June 29, 1946
(Saros 155)

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 1946
SE1801Oct07P.png
October 7, 1801
(Saros 150)
SE1830Sep17P.gif
September 17, 1830
(Saros 151)
SE1859Aug28P.gif
August 28, 1859
(Saros 152)
SE1888Aug07P.gif
August 7, 1888
(Saros 153)
SE1917Jul19P.png
July 19, 1917
(Saros 154)
SE1946Jun29P.png
June 29, 1946
(Saros 155)

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References

  1. "June 29, 1946 Partial Solar Eclipse". timeanddate. Retrieved 4 August 2024.
  2. "Partial Solar Eclipse of 1946 Jun 29". 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 155". eclipse.gsfc.nasa.gov.