Solar eclipse of March 5, 1924

Last updated
Solar eclipse of March 5, 1924
SE1924Mar05P.png
Map
Type of eclipse
NaturePartial
Gamma −1.2232
Magnitude 0.5819
Maximum eclipse
Coordinates 71°54′S55°36′E / 71.9°S 55.6°E / -71.9; 55.6
Times (UTC)
Greatest eclipse15:44:20
References
Saros 148 (16 of 75)
Catalog # (SE5000) 9336

A partial solar eclipse occurred at the Moon's descending node of orbit on Wednesday, March 5, 1924, [1] with a magnitude of 0.5819. 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 Africa.

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 5, 1924 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact1924 March 05 at 13:55:48.0 UTC
Equatorial Conjunction1924 March 05 at 15:01:55.2 UTC
Greatest Eclipse1924 March 05 at 15:44:20.0 UTC
Ecliptic Conjunction1924 March 05 at 15:57:55.9 UTC
Last Penumbral External Contact1924 March 05 at 17:33:17.1 UTC
March 5, 1924 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.58196
Eclipse Obscuration0.47664
Gamma−1.22320
Sun Right Ascension23h04m03.9s
Sun Declination-05°58'59.1"
Sun Semi-Diameter16'07.1"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension23h05m25.5s
Moon Declination-07°04'53.3"
Moon Semi-Diameter15'24.0"
Moon Equatorial Horizontal Parallax0°56'31.1"
ΔT23.5 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.

Eclipse season of February–March 1924
February 20
Ascending node (full moon)
March 5
Descending node (new moon)
Lunar eclipse chart close-1924Feb20.png SE1924Mar05P.png
Total lunar eclipse
Lunar Saros 122
Partial solar eclipse
Solar Saros 148

Eclipses in 1924

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 148

Inex

Triad

Solar eclipses of 1921–1924

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 July 31, 1924 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 1921 to 1924
Descending node Ascending node
SarosMapGammaSarosMapGamma
118 April 8, 1921
SE1921Apr08A.png
Annular
0.8869123 October 1, 1921
SE1921Oct01T.png
Total
−0.9383
128 March 28, 1922
SE1922Mar28A.png
Annular
0.1711133 September 21, 1922
SE1922Sep21T.png
Total
−0.213
138 March 17, 1923
SE1923Mar17A.png
Annular
−0.5438143 September 10, 1923
SE1923Sep10T.png
Total
0.5149
148 March 5, 1924
SE1924Mar05P.png
Partial
−1.2232153 August 30, 1924
SE1924Aug30P.png
Partial
1.3123

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 5, 1848 and July 30, 1935
March 5–6December 22–24October 9–11July 29–30May 17–18
108110112114116
SE1848Mar05P.gif
March 5, 1848
SE1859Jul29P.gif
July 29, 1859
SE1863May17P.gif
May 17, 1863
118120122124126
SE1867Mar06A.gif
March 6, 1867
SE1870Dec22T.png
December 22, 1870
SE1874Oct10An.gif
October 10, 1874
SE1878Jul29T.png
July 29, 1878
SE1882May17T.png
May 17, 1882
128130132134136
SE1886Mar05A.gif
March 5, 1886
SE1889Dec22T.png
December 22, 1889
SE1893Oct09A.png
October 9, 1893
SE1897Jul29A.png
July 29, 1897
SE1901May18T.png
May 18, 1901
138140142144146
SE1905Mar06A.png
March 6, 1905
SE1908Dec23H.png
December 23, 1908
SE1912Oct10T.png
October 10, 1912
SE1916Jul30A.png
July 30, 1916
SE1920May18P.png
May 18, 1920
148150152154
SE1924Mar05P.png
March 5, 1924
SE1927Dec24P.png
December 24, 1927
SE1931Oct11P.png
October 11, 1931
SE1935Jul30P.png
July 30, 1935

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
SE1808May25P.gif
May 25, 1808
(Saros 144)
SE1837May04P.gif
May 4, 1837
(Saros 145)
SE1866Apr15P.gif
April 15, 1866
(Saros 146)
SE1895Mar26P.gif
March 26, 1895
(Saros 147)
SE1924Mar05P.png
March 5, 1924
(Saros 148)
SE1953Feb14P.png
February 14, 1953
(Saros 149)
SE1982Jan25P.png
January 24, 1982
(Saros 150)
SE2011Jan04P.png
January 4, 2011
(Saros 151)
SE2039Dec15T.png
December 15, 2039
(Saros 152)
SE2068Nov24P.png
November 24, 2068
(Saros 153)
SE2097Nov04A.png
November 4, 2097
(Saros 154)
Saros155 12van71 SE2126Oct16T.jpg
October 16, 2126
(Saros 155)
Saros156 09van69 SE2155Sep26A.jpg
September 26, 2155
(Saros 156)
Saros157 08van70 SE2184Sep04A.jpg
September 4, 2184
(Saros 157)

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References

  1. "March 5, 1924 Partial Solar Eclipse". timeanddate. Retrieved 2 August 2024.
  2. "Partial Solar Eclipse of 1924 Mar 05". EclipseWise.com. Retrieved 2 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.