Solar eclipse of November 21, 1938

Last updated
Solar eclipse of November 21, 1938
SE1938Nov21P.png
Map
Type of eclipse
NaturePartial
Gamma 1.1077
Magnitude 0.7781
Maximum eclipse
Coordinates 68°54′N162°00′W / 68.9°N 162°W / 68.9; -162
Times (UTC)
Greatest eclipse23:52:25
References
Saros 151 (10 of 72)
Catalog # (SE5000) 9372

A partial solar eclipse occurred at the Moon's ascending node of orbit between Monday, November 21 and Tuesday, November 22, 1938, [1] with a magnitude of 0.7781. 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 Northeast Asia, Hawaii, and western North 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]

November 21, 1938 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact1938 November 21 at 21:45:25.1 UTC
Equatorial Conjunction1938 November 21 at 23:36:56.9 UTC
Greatest Eclipse1938 November 21 at 23:52:25.0 UTC
Ecliptic Conjunction1938 November 22 at 00:05:04.6 UTC
Last Penumbral External Contact1938 November 22 at 01:59:37.3 UTC
November 21, 1938 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.77807
Eclipse Obscuration0.70163
Gamma1.10769
Sun Right Ascension15h47m12.0s
Sun Declination-19°56'42.7"
Sun Semi-Diameter16'11.6"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension15h47m43.3s
Moon Declination-18°55'45.4"
Moon Semi-Diameter15'08.6"
Moon Equatorial Horizontal Parallax0°55'34.7"
ΔT24.0 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 November 1938
November 7
Descending node (full moon)
November 21
Ascending node (new moon)
Lunar eclipse chart close-1938Nov07.png SE1938Nov21P.png
Total lunar eclipse
Lunar Saros 125
Partial solar eclipse
Solar Saros 151

Eclipses in 1938

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 151

Inex

Triad

Solar eclipses of 1935–1938

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 February 3, 1935 and July 30, 1935 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 1935 to 1938
Ascending node Descending node
SarosMapGammaSarosMapGamma
111 January 5, 1935
SE1935Jan05P.png
Partial
−1.5381116 June 30, 1935
SE1935Jun30P.png
Partial
1.3623
121 December 25, 1935
SE1935Dec25A.png
Annular
−0.9228126 June 19, 1936
SE1936Jun19T.png
Total
0.5389
131 December 13, 1936
SE1936Dec13A.png
Annular
−0.2493136
Kanton total eclipse June8, 1937.jpg
Totality in Kanton Island,
Kiribati
June 8, 1937
SE1937Jun08T.png
Total
−0.2253
141 December 2, 1937
SE1937Dec02A.png
Annular
0.4389146 May 29, 1938
SE1938May29T.png
Total
−0.9607
151 November 21, 1938
SE1938Nov21P.png
Partial
1.1077

Saros 151

This eclipse is a part of Saros series 151, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on August 14, 1776. It contains annular eclipses from February 28, 2101 through April 23, 2191; a hybrid eclipse on May 5, 2209; and total eclipses from May 16, 2227 through July 6, 2912. The series ends at member 72 as a partial eclipse on October 1, 3056. 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 19 at 2 minutes, 44 seconds on February 28, 2101, and the longest duration of totality will be produced by member 60 at 5 minutes, 41 seconds on May 22, 2840. All eclipses in this series occur at the Moon’s ascending node of orbit. [4]

Series members 3–24 occur between 1801 and 2200:
345
SE1812Sep05P.gif
September 5, 1812
SE1830Sep17P.gif
September 17, 1830
SE1848Sep27P.gif
September 27, 1848
678
SE1866Oct08P.gif
October 8, 1866
SE1884Oct19P.gif
October 19, 1884
SE1902Oct31P.png
October 31, 1902
91011
SE1920Nov10P.png
November 10, 1920
SE1938Nov21P.png
November 21, 1938
SE1956Dec02P.png
December 2, 1956
121314
SE1974Dec13P.png
December 13, 1974
SE1992Dec24P.png
December 24, 1992
SE2011Jan04P.png
January 4, 2011
151617
SE2029Jan14P.png
January 14, 2029
SE2047Jan26P.png
January 26, 2047
SE2065Feb05P.png
February 5, 2065
181920
SE2083Feb16P.png
February 16, 2083
SE2101Feb28A.png
February 28, 2101
Saros151 20van72 SE2119Mar11A.jpg
March 11, 2119
212223
Saros151 21van72 SE2137Mar21A.jpg
March 21, 2137
SE2155Apr02A.png
April 2, 2155
Saros151 23van72 SE2173Apr12A.jpg
April 12, 2173
24
SE2191Apr23A.png
April 23, 2191

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 1982
SE1807Nov29H.gif
November 29, 1807
(Saros 139)
SE1818Oct29T.gif
October 29, 1818
(Saros 140)
SE1829Sep28A.gif
September 28, 1829
(Saros 141)
SE1840Aug27T.gif
August 27, 1840
(Saros 142)
SE1851Jul28T.png
July 28, 1851
(Saros 143)
SE1862Jun27P.gif
June 27, 1862
(Saros 144)
SE1873May26P.gif
May 26, 1873
(Saros 145)
SE1884Apr25P.gif
April 25, 1884
(Saros 146)
SE1895Mar26P.gif
March 26, 1895
(Saros 147)
SE1906Feb23P.png
February 23, 1906
(Saros 148)
SE1917Jan23P.png
January 23, 1917
(Saros 149)
SE1927Dec24P.png
December 24, 1927
(Saros 150)
SE1938Nov21P.png
November 21, 1938
(Saros 151)
SE1949Oct21P.png
October 21, 1949
(Saros 152)
SE1960Sep20P.png
September 20, 1960
(Saros 153)
SE1971Aug20P.png
August 20, 1971
(Saros 154)
SE1982Jul20P.png
July 20, 1982
(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 2200
SE1823Feb11P.gif
February 11, 1823
(Saros 147)
SE1852Jan21P.png
January 21, 1852
(Saros 148)
SE1880Dec31P.gif
December 31, 1880
(Saros 149)
SE1909Dec12P.png
December 12, 1909
(Saros 150)
SE1938Nov21P.png
November 21, 1938
(Saros 151)
SE1967Nov02T.png
November 2, 1967
(Saros 152)
SE1996Oct12P.png
October 12, 1996
(Saros 153)
SE2025Sep21P.png
September 21, 2025
(Saros 154)
SE2054Sep02P.png
September 2, 2054
(Saros 155)
SE2083Aug13P.png
August 13, 2083
(Saros 156)
Saros157 04van70 SE2112Jul23P.jpg
July 23, 2112
(Saros 157)
Saros158 05van70 SE2141Jul03P.jpg
July 3, 2141
(Saros 158)
Saros159 03van70 SE2170Jun14P.jpg
June 14, 2170
(Saros 159)
Saros160 02van71 SE2199May24P.jpg
May 24, 2199
(Saros 160)

Notes

  1. "November 21–22, 1938 Partial Solar Eclipse". timeanddate. Retrieved 3 August 2024.
  2. "Partial Solar Eclipse of 1938 Nov 21". EclipseWise.com. Retrieved 3 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 151". eclipse.gsfc.nasa.gov.

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References