Solar eclipse of November 12, 1928
Solar eclipse of November 12, 1928 | |
---|---|
Type of eclipse | |
Nature | Partial |
Gamma | 1.0861 |
Magnitude | 0.8078 |
Maximum eclipse | |
Coordinates | 62°36′N 81°06′E / 62.6°N 81.1°E |
Times (UTC) | |
Greatest eclipse | 9:48:24 |
References | |
Saros | 122 (53 of 70) |
Catalog # (SE5000) | 9348 |
A partial solar eclipse occurred at the Moon's descending node of orbit on Monday, November 12, 1928, with a magnitude of 0.8078. 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.
Related eclipses[edit]
Eclipses in 1928[edit]
- A total solar eclipse on May 19, 1928.
- A total lunar eclipse on June 3, 1928.
- A partial solar eclipse on June 17, 1928.
- A partial solar eclipse on November 12, 1928.
- A total lunar eclipse on November 27, 1928.
Metonic[edit]
- Preceded by: Solar eclipse of January 24, 1925
- Followed by: Solar eclipse of August 31, 1932
Tzolkinex[edit]
- Preceded by: Solar eclipse of October 1, 1921
- Followed by: Solar eclipse of December 25, 1935
Half-Saros[edit]
- Preceded by: Lunar eclipse of November 7, 1919
- Followed by: Lunar eclipse of November 18, 1937
Tritos[edit]
- Preceded by: Solar eclipse of December 14, 1917
- Followed by: Solar eclipse of October 12, 1939
Solar Saros 122[edit]
- Preceded by: Solar eclipse of November 2, 1910
- Followed by: Solar eclipse of November 23, 1946
Inex[edit]
- Preceded by: Solar eclipse of December 3, 1899
- Followed by: Solar eclipse of October 23, 1957
Triad[edit]
- Preceded by: Solar eclipse of January 11, 1842
- Followed by: Solar eclipse of September 13, 2015
Solar eclipses of 1928–1931[edit]
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.[1]
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 122[edit]
This eclipse is a part of Saros series 122, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on April 17, 991 AD. It contains total eclipses from July 12, 1135 through August 3, 1171; hybrid eclipses on August 13, 1189 and August 25, 1207; and annular eclipses from September 4, 1225 through October 10, 1874. The series ends at member 70 as a partial eclipse on May 17, 2235. 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 was produced by member 9 at 1 minutes, 25 seconds on July 12, 1135, and the longest duration of annularity was produced by member 50 at 6 minutes, 28 seconds on October 10, 1874. All eclipses in this series occur at the Moon’s descending node of orbit.[2]
Series members 46–68 occur between 1801 and 2200: | ||
---|---|---|
46 | 47 | 48 |
August 28, 1802 |
September 7, 1820 |
September 18, 1838 |
49 | 50 | 51 |
September 29, 1856 |
October 10, 1874 |
October 20, 1892 |
52 | 53 | 54 |
November 2, 1910 |
November 12, 1928 |
November 23, 1946 |
55 | 56 | 57 |
December 4, 1964 |
December 15, 1982 |
December 25, 2000 |
58 | 59 | 60 |
January 6, 2019 |
January 16, 2037 |
January 27, 2055 |
61 | 62 | 63 |
February 7, 2073 |
February 18, 2091 |
March 1, 2109 |
64 | 65 | 66 |
March 13, 2127 |
March 23, 2145 |
April 3, 2163 |
67 | 68 | |
April 14, 2181 |
April 25, 2199 |
Metonic series[edit]
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).
22 eclipse events, progressing from north to south between April 8, 1902 and August 31, 1989: | ||||
---|---|---|---|---|
April 7–8 | January 24–25 | November 12 | August 31-September 1 | June 19–20 |
108 | 114 | 116 | ||
April 8, 1902 |
August 31, 1913 |
June 19, 1917 | ||
118 | 120 | 122 | 124 | 126 |
April 8, 1921 |
January 24, 1925 |
November 12, 1928 |
August 31, 1932 |
June 19, 1936 |
128 | 130 | 132 | 134 | 136 |
April 7, 1940 |
January 25, 1944 |
November 12, 1947 |
September 1, 1951 |
June 20, 1955 |
138 | 140 | 142 | 144 | 146 |
April 8, 1959 |
January 25, 1963 |
November 12, 1966 |
August 31, 1970 |
June 20, 1974 |
148 | 150 | 152 | 154 | |
April 7, 1978 |
January 25, 1982 |
November 12, 1985 |
August 31, 1989 |
References[edit]
- ^ 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 122". eclipse.gsfc.nasa.gov.
External links[edit]
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC