A partial solar eclipse occurred at the Moon's descending node of orbit on Sunday, October 11, 1931,[1] with a magnitude of 0.9005. 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.
| Solar eclipse of October 11, 1931 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Partial |
| Gamma | −1.0607 |
| Magnitude | 0.9005 |
| Maximum eclipse | |
| Coordinates | 61°12′S 119°30′W / 61.2°S 119.5°W |
| Times (UTC) | |
| Greatest eclipse | 12:55:40 |
| References | |
| Saros | 152 (8 of 70) |
| Catalog # (SE5000) | 9354 |
A partial eclipse was visible for parts of southern and central South America and Antarctica.
Eclipse details
editShown 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 | 1931 October 11 at 11:01:29.3 UTC |
| Greatest Eclipse | 1931 October 11 at 12:55:39.8 UTC |
| Ecliptic Conjunction | 1931 October 11 at 13:06:15.3 UTC |
| Equatorial Conjunction | 1931 October 11 at 13:53:48.2 UTC |
| Last Penumbral External Contact | 1931 October 11 at 14:49:27.7 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.90054 |
| Eclipse Obscuration | 0.88440 |
| Gamma | −1.06069 |
| Sun Right Ascension | 13h03m34.8s |
| Sun Declination | -06°46'31.5" |
| Sun Semi-Diameter | 16'01.4" |
| Sun Equatorial Horizontal Parallax | 08.8" |
| Moon Right Ascension | 13h01m31.6s |
| Moon Declination | -07°43'48.4" |
| Moon Semi-Diameter | 16'43.0" |
| Moon Equatorial Horizontal Parallax | 1°01'21.2" |
| ΔT | 23.9 s |
Eclipse season
editThis 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.
| September 12 Descending node (new moon) |
September 26 Ascending node (full moon) |
October 11 Descending node (new moon) |
|---|---|---|
| Partial solar eclipse Solar Saros 114 |
Total lunar eclipse Lunar Saros 126 |
Partial solar eclipse Solar Saros 152 |
Related eclipses
editEclipses in 1931
edit- A total lunar eclipse on April 2.
- A partial solar eclipse on April 18.
- A partial solar eclipse on September 12.
- A total lunar eclipse on September 26.
- A partial solar eclipse on October 11.
Metonic
edit- Preceded by: Solar eclipse of December 24, 1927
- Followed by: Solar eclipse of July 30, 1935
Tzolkinex
edit- Preceded by: Solar eclipse of August 30, 1924
- Followed by: Solar eclipse of November 21, 1938
Half-Saros
edit- Preceded by: Lunar eclipse of October 6, 1922
- Followed by: Lunar eclipse of October 16, 1940
Tritos
edit- Preceded by: Solar eclipse of November 10, 1920
- Followed by: Solar eclipse of September 10, 1942
Solar Saros 152
edit- Preceded by: Solar eclipse of September 30, 1913
- Followed by: Solar eclipse of October 21, 1949
Inex
edit- Preceded by: Solar eclipse of October 31, 1902
- Followed by: Solar eclipse of September 20, 1960
Triad
edit- Preceded by: Solar eclipse of December 9, 1844
- Followed by: Solar eclipse of August 11, 2018
Solar eclipses of 1928–1931
editThis 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 June 17, 1928 occurs in the previous lunar year eclipse set, and the partial solar eclipse on September 12, 1931 occurs in the next lunar year eclipse set.
| Solar eclipse series sets from 1928 to 1931 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 117 | May 19, 1928 Total (non-central) |
1.0048 | 122 | November 12, 1928 Partial |
1.0861 | |
| 127 | May 9, 1929 Total |
−0.2887 | 132 | November 1, 1929 Annular |
0.3514 | |
| 137 | April 28, 1930 Hybrid |
0.473 | 142 | October 21, 1930 Total |
−0.3804 | |
| 147 | April 18, 1931 Partial |
1.2643 | 152 | October 11, 1931 Partial |
−1.0607 | |
Saros 152
editThis eclipse is a part of Saros series 152, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on July 26, 1805. It contains total eclipses from November 2, 1967 through September 14, 2490; hybrid eclipses from September 26, 2508 through October 17, 2544; and annular eclipses from October 29, 2562 through June 16, 2941. The series ends at member 70 as a partial eclipse on August 20, 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 totality will be produced by member 30 at 5 minutes, 16 seconds on June 9, 2328, and the longest duration of annularity will be produced by member 53 at 5 minutes, 20 seconds on February 16, 2743. All eclipses in this series occur at the Moon’s descending node of orbit.[4]
| Series members 1–22 occur between 1805 and 2200: | ||
|---|---|---|
| 1 | 2 | 3 |
| July 26, 1805 |
August 6, 1823 |
August 16, 1841 |
| 4 | 5 | 6 |
| August 28, 1859 |
September 7, 1877 |
September 18, 1895 |
| 7 | 8 | 9 |
| September 30, 1913 |
October 11, 1931 |
October 21, 1949 |
| 10 | 11 | 12 |
| November 2, 1967 |
November 12, 1985 |
November 23, 2003 |
| 13 | 14 | 15 |
| December 4, 2021 |
December 15, 2039 |
December 26, 2057 |
| 16 | 17 | 18 |
| January 6, 2076 |
January 16, 2094 |
January 29, 2112 |
| 19 | 20 | 21 |
| February 8, 2130 |
February 19, 2148 |
March 2, 2166 |
| 22 | ||
| March 12, 2184 | ||
Metonic series
editThe 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 5–6 | December 22–24 | October 9–11 | July 29–30 | May 17–18 |
| 108 | 110 | 112 | 114 | 116 |
| March 5, 1848 |
July 29, 1859 |
May 17, 1863 | ||
| 118 | 120 | 122 | 124 | 126 |
| March 6, 1867 |
December 22, 1870 |
October 10, 1874 |
July 29, 1878 |
May 17, 1882 |
| 128 | 130 | 132 | 134 | 136 |
| March 5, 1886 |
December 22, 1889 |
October 9, 1893 |
July 29, 1897 |
May 18, 1901 |
| 138 | 140 | 142 | 144 | 146 |
| March 6, 1905 |
December 23, 1908 |
October 10, 1912 |
July 30, 1916 |
May 18, 1920 |
| 148 | 150 | 152 | 154 | |
| March 5, 1924 |
December 24, 1927 |
October 11, 1931 |
July 30, 1935 | |
Tritos series
editThis 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 1964 | ||||
|---|---|---|---|---|
| September 17, 1811 (Saros 141) |
August 16, 1822 (Saros 142) |
July 17, 1833 (Saros 143) |
June 16, 1844 (Saros 144) |
May 16, 1855 (Saros 145) |
| April 15, 1866 (Saros 146) |
March 15, 1877 (Saros 147) |
February 11, 1888 (Saros 148) |
January 11, 1899 (Saros 149) |
December 12, 1909 (Saros 150) |
| November 10, 1920 (Saros 151) |
October 11, 1931 (Saros 152) |
September 10, 1942 (Saros 153) |
August 9, 1953 (Saros 154) |
July 9, 1964 (Saros 155) |
Inex series
editThis 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 | ||
|---|---|---|
| December 30, 1815 (Saros 148) |
December 9, 1844 (Saros 149) |
November 20, 1873 (Saros 150) |
| October 31, 1902 (Saros 151) |
October 11, 1931 (Saros 152) |
September 20, 1960 (Saros 153) |
| August 31, 1989 (Saros 154) |
August 11, 2018 (Saros 155) |
July 22, 2047 (Saros 156) |
| July 1, 2076 (Saros 157) |
June 12, 2105 (Saros 158) |
May 23, 2134 (Saros 159) |
| April 12, 2192 (Saros 161) |
||
Notes
edit- ^ "October 11, 1931 Partial Solar Eclipse". timeanddate. Retrieved 3 August 2024.
- ^ "Partial Solar Eclipse of 1931 Oct 11". EclipseWise.com. Retrieved 3 August 2024.
- ^ 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.
- ^ "NASA - Catalog of Solar Eclipses of Saros 152". eclipse.gsfc.nasa.gov.
References
edit- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
