Solar eclipse of August 30, 1924

Last updated
Solar eclipse of August 30, 1924
SE1924Aug30P.png
Map
Type of eclipse
NaturePartial
Gamma 1.3123
Magnitude 0.4245
Maximum eclipse
Coordinates 71°30′N172°54′E / 71.5°N 172.9°E / 71.5; 172.9
Times (UTC)
Greatest eclipse8:23:00
References
Saros 153 (4 of 70)
Catalog # (SE5000) 9337

A partial solar eclipse occurred at the Moon's ascending node of orbit on Saturday, August 30, 1924, [1] with a magnitude of 0.4245. 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 Greenland, the Russian SFSR, and Northeast Asia.

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]

August 30, 1924 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact1924 August 30 at 06:50:49.9 UTC
Equatorial Conjunction1924 August 30 at 07:40:15.6 UTC
Greatest Eclipse1924 August 30 at 08:23:00.2 UTC
Ecliptic Conjunction1924 August 30 at 08:37:02.6 UTC
Last Penumbral External Contact1924 August 30 at 09:55:25.5 UTC
August 30, 1924 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.42450
Eclipse Obscuration0.30793
Gamma1.31228
Sun Right Ascension10h33m37.7s
Sun Declination+09°04'07.2"
Sun Semi-Diameter15'50.6"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension10h35m02.3s
Moon Declination+10°15'33.7"
Moon Semi-Diameter15'29.6"
Moon Equatorial Horizontal Parallax0°56'51.5"
ΔT23.6 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 July–August 1924
July 31
Ascending node (new moon)
August 14
Descending node (full moon)
August 30
Ascending node (new moon)
SE1924Jul31P.png Lunar eclipse chart close-1924Aug14.png SE1924Aug30P.png
Partial solar eclipse
Solar Saros 115
Total lunar eclipse
Lunar Saros 127
Partial solar eclipse
Solar Saros 153

Eclipses in 1924

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 153

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 153

This eclipse is a part of Saros series 153, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on July 28, 1870. It contains annular eclipses from December 17, 2104 through May 26, 2970. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on August 22, 3114. 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 7 minutes, 1 seconds on September 5, 2537. All eclipses in this series occur at the Moon’s ascending node of orbit. [4]

Series members 1–19 occur between 1870 and 2200:
123
SE1870Jul28Pb.gif
July 28, 1870
SE1888Aug07P.gif
August 7, 1888
SE1906Aug20P.png
August 20, 1906
456
SE1924Aug30P.png
August 30, 1924
SE1942Sep10P.png
September 10, 1942
SE1960Sep20P.png
September 20, 1960
789
SE1978Oct02P.png
October 2, 1978
SE1996Oct12P.png
October 12, 1996
SE2014Oct23P.png
October 23, 2014
101112
SE2032Nov03P.png
November 3, 2032
SE2050Nov14P.png
November 14, 2050
SE2068Nov24P.png
November 24, 2068
131415
SE2086Dec06P.png
December 6, 2086
Saros153 14van70 SE2104Dec17A.jpg
December 17, 2104
Saros153 15van70 SE2122Dec28A.jpg
December 28, 2122
161718
Saros153 16van70 SE2141Jan08A.jpg
January 8, 2141
Saros153 17van70 SE2159Jan19A.jpg
January 19, 2159
Saros153 18van70 SE2177Jan29A.jpg
January 29, 2177
19
Saros153 19van70 SE2195Feb10A.jpg
February 10, 2195

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.

25 eclipse events between April 5, 1837 and June 17, 1928
April 5–6January 22–23November 10–11August 28–30June 17–18
107109111113115
SE1837Apr05P.png
April 5, 1837
SE1841Jan22P.gif
January 22, 1841
SE1844Nov10P.gif
November 10, 1844
SE1848Aug28P.gif
August 28, 1848
SE1852Jun17P.gif
June 17, 1852
117119121123125
SE1856Apr05T.gif
April 5, 1856
SE1860Jan23A.gif
January 23, 1860
SE1863Nov11A.gif
November 11, 1863
SE1867Aug29T.gif
August 29, 1867
SE1871Jun18A.gif
June 18, 1871
127129131133135
SE1875Apr06T.gif
April 6, 1875
SE1879Jan22A.gif
January 22, 1879
SE1882Nov10A.gif
November 10, 1882
SE1886Aug29T.png
August 29, 1886
SE1890Jun17A.gif
June 17, 1890
137139141143145
SE1894Apr06H.gif
April 6, 1894
SE1898Jan22T.png
January 22, 1898
SE1901Nov11A.png
November 11, 1901
SE1905Aug30T.png
August 30, 1905
SE1909Jun17H.png
June 17, 1909
147149151153155
SE1913Apr06P.png
April 6, 1913
SE1917Jan23P.png
January 23, 1917
SE1920Nov10P.png
November 10, 1920
SE1924Aug30P.png
August 30, 1924
SE1928Jun17P.png
June 17, 1928

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 2069
SE1808Nov18P.gif
November 18, 1808
(Saros 149)
SE1837Oct29P.gif
October 29, 1837
(Saros 150)
SE1866Oct08P.gif
October 8, 1866
(Saros 151)
SE1895Sep18P.gif
September 18, 1895
(Saros 152)
SE1924Aug30P.png
August 30, 1924
(Saros 153)
SE1953Aug09P.png
August 9, 1953
(Saros 154)
SE1982Jul20P.png
July 20, 1982
(Saros 155)
SE2011Jul01P.png
July 1, 2011
(Saros 156)
SE2069May20P.png
May 20, 2069
(Saros 158)

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References

  1. "August 30, 1924 Partial Solar Eclipse". timeanddate. Retrieved 2 August 2024.
  2. "Partial Solar Eclipse of 1924 Aug 30". 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 153". eclipse.gsfc.nasa.gov.