Solar eclipse of April 28, 1949

Last updated
Solar eclipse of April 28, 1949
SE1949Apr28P.png
Map
Type of eclipse
NaturePartial
Gamma 1.2068
Magnitude 0.6092
Maximum eclipse
Coordinates 61°54′N55°42′W / 61.9°N 55.7°W / 61.9; -55.7
Times (UTC)
Greatest eclipse7:48:53
References
Saros 147 (19 of 80)
Catalog # (SE5000) 9396

A partial solar eclipse occurred at the Moon's ascending node of orbit on Thursday, April 28, 1949, [1] with a magnitude of 0.6092. 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 North Africa, Europe, the Soviet Union, Greenland, and northern 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]

April 28, 1949 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact1949 April 28 at 05:52:15.3 UTC
Greatest Eclipse1949 April 28 at 07:48:53.1 UTC
Ecliptic Conjunction1949 April 28 at 08:02:42.0 UTC
Equatorial Conjunction1949 April 28 at 08:53:20.8 UTC
Last Penumbral External Contact1949 April 28 at 09:45:01.2 UTC
April 28, 1949 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.60918
Eclipse Obscuration0.50435
Gamma1.20682
Sun Right Ascension02h21m19.3s
Sun Declination+14°04'51.6"
Sun Semi-Diameter15'52.9"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension02h19m26.3s
Moon Declination+15°04'38.0"
Moon Semi-Diameter14'52.8"
Moon Equatorial Horizontal Parallax0°54'36.6"
ΔT28.9 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 April 1949
April 13
Descending node (full moon)
April 28
Ascending node (new moon)
Lunar eclipse chart close-1949Apr13.png SE1949Apr28P.png
Total lunar eclipse
Lunar Saros 121
Partial solar eclipse
Solar Saros 147

Eclipses in 1949

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 147

Inex

Triad

Solar eclipses of 1946–1949

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 January 3, 1946 and June 29, 1946 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 1946 to 1949
Ascending node Descending node
SarosMapGammaSarosMapGamma
117 May 30, 1946
SE1946May30P.png
Partial
−1.0711122 November 23, 1946
SE1946Nov23P.png
Partial
1.105
127 May 20, 1947
SE1947May20T.png
Total
−0.3528132 November 12, 1947
SE1947Nov12A.png
Annular
0.3743
137 May 9, 1948
SE1948May09A.png
Annular
0.4133142 November 1, 1948
SE1948Nov01T.png
Total
−0.3517
147 April 28, 1949
SE1949Apr28P.png
Partial
1.2068152 October 21, 1949
SE1949Oct21P.png
Partial
−1.027

Saros 147

This eclipse is a part of Saros series 147, repeating every 18 years, 11 days, and containing 80 events. The series started with a partial solar eclipse on October 12, 1624. It contains annular eclipses from May 31, 2003 through July 31, 2706. There are no hybrid or total eclipses in this set. The series ends at member 80 as a partial eclipse on February 24, 3049. 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 38 at 9 minutes, 41 seconds on November 21, 2291. All eclipses in this series occur at the Moon’s ascending node of orbit. [4]

Series members 11–32 occur between 1801 and 2200:
111213
SE1805Jan30P.gif
January 30, 1805
SE1823Feb11P.gif
February 11, 1823
SE1841Feb21P.gif
February 21, 1841
141516
SE1859Mar04P.gif
March 4, 1859
SE1877Mar15P.gif
March 15, 1877
SE1895Mar26P.gif
March 26, 1895
171819
SE1913Apr06P.png
April 6, 1913
SE1931Apr18P.png
April 18, 1931
SE1949Apr28P.png
April 28, 1949
202122
SE1967May09P.png
May 9, 1967
SE1985May19P.png
May 19, 1985
SE2003May31A.png
May 31, 2003
232425
SE2021Jun10A.png
June 10, 2021
SE2039Jun21A.png
June 21, 2039
SE2057Jul01A.png
July 1, 2057
262728
SE2075Jul13A.png
July 13, 2075
SE2093Jul23A.png
July 23, 2093
SE2111Aug04A.png
August 4, 2111
293031
SE2129Aug15A.png
August 15, 2129
Saros147 30van80 SE2147Aug26A.jpg
August 26, 2147
Saros147 31van80 SE2165Sep05A.jpg
September 5, 2165
32
Saros147 32van80 SE2183Sep16A.jpg
September 16, 2183

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.

22 eclipse events between December 2, 1880 and July 9, 1964
December 2–3September 20–21July 9–10April 26–28February 13–14
111113115117119
SE1880Dec02P.gif
December 2, 1880
SE1888Jul09P.gif
July 9, 1888
SE1892Apr26T.gif
April 26, 1892
SE1896Feb13A.png
February 13, 1896
121123125127129
SE1899Dec03A.gif
December 3, 1899
SE1903Sep21T.png
September 21, 1903
SE1907Jul10A.png
July 10, 1907
SE1911Apr28T.png
April 28, 1911
SE1915Feb14A.png
February 14, 1915
131133135137139
SE1918Dec03A.png
December 3, 1918
SE1922Sep21T.png
September 21, 1922
SE1926Jul09A.png
July 9, 1926
SE1930Apr28H.png
April 28, 1930
SE1934Feb14T.png
February 14, 1934
141143145147149
SE1937Dec02A.png
December 2, 1937
SE1941Sep21T.png
September 21, 1941
SE1945Jul09T.png
July 9, 1945
SE1949Apr28P.png
April 28, 1949
SE1953Feb14P.png
February 14, 1953
151153155
SE1956Dec02P.png
December 2, 1956
SE1960Sep20P.png
September 20, 1960
SE1964Jul09P.png
July 9, 1964

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 eclipses on November 16, 2134 (part of Saros 164) and October 16, 2145 (part of Saros 165) are also a part of this series but are not included in the table below.

Series members between 1801 and 2069
SE1807Jun06H.png
June 6, 1807
(Saros 134)
SE1818May05A.gif
May 5, 1818
(Saros 135)
SE1829Apr03T.gif
April 3, 1829
(Saros 136)
SE1840Mar04A.png
March 4, 1840
(Saros 137)
SE1851Feb01A.gif
February 1, 1851
(Saros 138)
SE1861Dec31T.gif
December 31, 1861
(Saros 139)
SE1872Nov30H.gif
November 30, 1872
(Saros 140)
SE1883Oct30A.gif
October 30, 1883
(Saros 141)
SE1894Sep29T.gif
September 29, 1894
(Saros 142)
SE1905Aug30T.png
August 30, 1905
(Saros 143)
SE1916Jul30A.png
July 30, 1916
(Saros 144)
SE1927Jun29T.png
June 29, 1927
(Saros 145)
SE1938May29T.png
May 29, 1938
(Saros 146)
SE1949Apr28P.png
April 28, 1949
(Saros 147)
SE1960Mar27P.png
March 27, 1960
(Saros 148)
SE1971Feb25P.png
February 25, 1971
(Saros 149)
SE1982Jan25P.png
January 25, 1982
(Saros 150)
SE1992Dec24P.png
December 24, 1992
(Saros 151)
SE2003Nov23T.png
November 23, 2003
(Saros 152)
SE2014Oct23P.png
October 23, 2014
(Saros 153)
SE2025Sep21P.png
September 21, 2025
(Saros 154)
SE2036Aug21P.png
August 21, 2036
(Saros 155)
SE2047Jul22P.png
July 22, 2047
(Saros 156)
SE2058Jun21P.png
June 21, 2058
(Saros 157)
SE2069May20P.png
May 20, 2069
(Saros 158)

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
SE1804Aug05T.gif
August 5, 1804
(Saros 142)
SE1833Jul17T.gif
July 17, 1833
(Saros 143)
SE1862Jun27P.gif
June 27, 1862
(Saros 144)
SE1891Jun06A.gif
June 6, 1891
(Saros 145)
SE1920May18P.png
May 18, 1920
(Saros 146)
SE1949Apr28P.png
April 28, 1949
(Saros 147)
SE1978Apr07P.png
April 7, 1978
(Saros 148)
SE2007Mar19P.png
March 19, 2007
(Saros 149)
SE2036Feb27P.png
February 27, 2036
(Saros 150)
SE2065Feb05P.png
February 5, 2065
(Saros 151)
SE2094Jan16T.png
January 16, 2094
(Saros 152)
Saros153 15van70 SE2122Dec28A.jpg
December 28, 2122
(Saros 153)
Saros154 14van71 SE2151Dec08A.jpg
December 8, 2151
(Saros 154)
Saros155 15van71 SE2180Nov17T.jpg
November 17, 2180
(Saros 155)

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References

  1. "April 28, 1949 Partial Solar Eclipse". timeanddate. Retrieved 4 August 2024.
  2. "Partial Solar Eclipse of 1949 Apr 28". 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 147". eclipse.gsfc.nasa.gov.