Solar eclipse of August 30, 1924
Template:Short description Script error: No such module "Solar eclipse". 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.
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]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 1924 August 30 at 06:50:49.9 UTC |
| Equatorial Conjunction | 1924 August 30 at 07:40:15.6 UTC |
| Greatest Eclipse | 1924 August 30 at 08:23:00.2 UTC |
| Ecliptic Conjunction | 1924 August 30 at 08:37:02.6 UTC |
| Last Penumbral External Contact | 1924 August 30 at 09:55:25.5 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.42450 |
| Eclipse Obscuration | 0.30793 |
| Gamma | 1.31228 |
| Sun Right Ascension | 10h33m37.7s |
| Sun Declination | +09°04'07.2" |
| Sun Semi-Diameter | 15'50.6" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 10h35m02.3s |
| Moon Declination | +10°15'33.7" |
| Moon Semi-Diameter | 15'29.6" |
| Moon Equatorial Horizontal Parallax | 0°56'51.5" |
| ΔT | 23.6 s |
Eclipse season
Script error: No such module "Labelled list hatnote". 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.
| July 31 Ascending node (new moon) |
August 14 Descending node (full moon) |
August 30 Ascending node (new moon) |
|---|---|---|
| File:SE1924Jul31P.png | File:Lunar eclipse chart close-1924Aug14.png | File:SE1924Aug30P.png |
| Partial solar eclipse Solar Saros 115 |
Total lunar eclipse Lunar Saros 127 |
Partial solar eclipse Solar Saros 153 |
Related eclipses
Eclipses in 1924
- A total lunar eclipse on February 20.
- A partial solar eclipse on March 5.
- A partial solar eclipse on July 31.
- A total lunar eclipse on August 14.
- A partial solar eclipse on August 30.
Metonic
- Preceded by: Solar eclipse of November 10, 1920
- Followed by: Solar eclipse of June 17, 1928
Tzolkinex
- Preceded by: Solar eclipse of July 19, 1917
- Followed by: Solar eclipse of October 11, 1931
Half-Saros
- Preceded by: Lunar eclipse of August 24, 1915
- Followed by: Lunar eclipse of September 4, 1933
Tritos
- Preceded by: Solar eclipse of September 30, 1913
- Followed by: Solar eclipse of July 30, 1935
Solar Saros 153
- Preceded by: Solar eclipse of August 20, 1906
- Followed by: Solar eclipse of September 10, 1942
Inex
- Preceded by: Solar eclipse of September 18, 1895
- Followed by: Solar eclipse of August 9, 1953
Triad
- Preceded by: Solar eclipse of October 29, 1837
- Followed by: Solar eclipse of July 1, 2011
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 | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 118 | April 8, 1921 File:SE1921Apr08A.png Annular |
0.8869 | 123 | October 1, 1921 File:SE1921Oct01T.png Total |
−0.9383 | |
| 128 | March 28, 1922 File:SE1922Mar28A.png Annular |
0.1711 | 133 | September 21, 1922 File:SE1922Sep21T.png Total |
−0.213 | |
| 138 | March 17, 1923 File:SE1923Mar17A.png Annular |
−0.5438 | 143 | September 10, 1923 File:SE1923Sep10T.png Total |
0.5149 | |
| 148 | March 5, 1924 File:SE1924Mar05P.png Partial |
−1.2232 | 153 | August 30, 1924 File:SE1924Aug30P.png Partial |
1.3123 | |
Saros 153
Template:Solar Saros series 153
Metonic series
Template:Solar Metonic series 1837–1928
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 | ||||
|---|---|---|---|---|
| File:SE1804Aug05T.gif August 5, 1804 (Saros 142) |
File:SE1815Jul06T.gif July 6, 1815 (Saros 143) |
File:SE1826Jun05P.gif June 5, 1826 (Saros 144) |
File:SE1837May04P.gif May 4, 1837 (Saros 145) |
File:SE1848Apr03P.png April 3, 1848 (Saros 146) |
| File:SE1859Mar04P.gif March 4, 1859 (Saros 147) |
File:SE1870Jan31P.gif January 31, 1870 (Saros 148) |
File:SE1880Dec31P.gif December 31, 1880 (Saros 149) |
File:SE1891Dec01P.gif December 1, 1891 (Saros 150) |
File:SE1902Oct31P.png October 31, 1902 (Saros 151) |
| File:SE1913Sep30P.png September 30, 1913 (Saros 152) |
File:SE1924Aug30P.png August 30, 1924 (Saros 153) |
File:SE1935Jul30P.png July 30, 1935 (Saros 154) |
File:SE1946Jun29P.png June 29, 1946 (Saros 155) | |
Inex series
Template:Solar Inex series 2011 July 1
References
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External links
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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