Solar eclipse of September 12, 1950
Solar eclipse of September 12, 1950 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | 0.8903 |
Magnitude | 1.0182 |
Maximum eclipse | |
Duration | 74 s (1 min 14 s) |
Coordinates | 54°48′N 172°18′E / 54.8°N 172.3°E |
Max. width of band | 134 km (83 mi) |
Times (UTC) | |
Greatest eclipse | 3:38:47 |
References | |
Saros | 124 (51 of 73) |
Catalog # (SE5000) | 9399 |
A total solar eclipse occurred at the Moon's descending node of orbit on Tuesday, September 12, 1950, with a magnitude of 1.0182. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Totality was visible from eastern Soviet Union (today's Russia) on September 12 local time and the whole Semichi Islands in Alaska on September 11 local time.
Related eclipses[edit]
Eclipses in 1950[edit]
- An annular solar eclipse on March 18, 1950.
- A total lunar eclipse on April 2, 1950.
- A total solar eclipse on September 12, 1950.
- A total lunar eclipse on September 26, 1950.
Metonic[edit]
- Preceded by: Solar eclipse of November 23, 1946
- Followed by: Solar eclipse of June 30, 1954
Tzolkinex[edit]
- Preceded by: Solar eclipse of August 1, 1943
- Followed by: Solar eclipse of October 23, 1957
Half-Saros[edit]
- Preceded by: Lunar eclipse of September 5, 1941
- Followed by: Lunar eclipse of September 17, 1959
Tritos[edit]
- Preceded by: Solar eclipse of October 12, 1939
- Followed by: Solar eclipse of August 11, 1961
Solar Saros 124[edit]
- Preceded by: Solar eclipse of August 31, 1932
- Followed by: Solar eclipse of September 22, 1968
Inex[edit]
- Preceded by: Solar eclipse of October 1, 1921
- Followed by: Solar eclipse of August 22, 1979
Triad[edit]
- Preceded by: Solar eclipse of November 11, 1863
- Followed by: Solar eclipse of July 13, 2037
Solar eclipses of 1950–1953[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 July 11, 1953 occurs in the next lunar year eclipse set.
Solar eclipse series sets from 1950 to 1953 | ||||||
---|---|---|---|---|---|---|
Ascending node | Descending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
119 | March 18, 1950![]() Annular (non-central) |
0.9988 | 124 | September 12, 1950![]() Total |
0.8903 | |
129 | March 7, 1951![]() Annular |
−0.242 | 134 | September 1, 1951![]() Annular |
0.1557 | |
139 | February 25, 1952![]() Total |
0.4697 | 144 | August 20, 1952![]() Annular |
−0.6102 | |
149 | February 14, 1953![]() Partial |
1.1331 | 154 | August 9, 1953![]() Partial |
−1.344 |
Saros 124[edit]
This eclipse is a part of Saros series 124, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on March 6, 1049. It contains total eclipses from June 12, 1211 through September 22, 1968, and a hybrid eclipse on October 3, 1986. There are no annular eclipses in this set. The series ends at member 73 as a partial eclipse on May 11, 2347. 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 39 at 5 minutes, 46 seconds on May 3, 1734. All eclipses in this series occur at the Moon’s descending node of orbit.[2]
Series members 43–64 occur between 1801 and 2200: | ||
---|---|---|
43 | 44 | 45 |
![]() June 16, 1806 |
![]() June 26, 1824 |
![]() July 8, 1842 |
46 | 47 | 48 |
![]() July 18, 1860 |
![]() July 29, 1878 |
![]() August 9, 1896 |
49 | 50 | 51 |
![]() August 21, 1914 |
![]() August 31, 1932 |
![]() September 12, 1950 |
52 | 53 | 54 |
![]() September 22, 1968 |
![]() October 3, 1986 |
![]() October 14, 2004 |
55 | 56 | 57 |
![]() October 25, 2022 |
![]() November 4, 2040 |
![]() November 16, 2058 |
58 | 59 | 60 |
![]() November 26, 2076 |
![]() December 7, 2094 |
![]() December 19, 2112 |
61 | 62 | 63 |
![]() December 30, 2130 |
![]() January 9, 2149 |
![]() January 21, 2167 |
64 | ||
![]() January 31, 2185 |
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). All eclipses in this table occur at the Moon's descending node.
22 eclipse events between September 12, 1931 and July 1, 2011. | ||||
---|---|---|---|---|
September 11-12 | June 30-July 1 | April 17-19 | February 4-5 | November 22-23 |
114 | 116 | 118 | 120 | 122 |
![]() September 12, 1931 |
![]() June 30, 1935 |
![]() April 19, 1939 |
![]() February 4, 1943 |
![]() November 23, 1946 |
124 | 126 | 128 | 130 | 132 |
![]() September 12, 1950 |
![]() June 30, 1954 |
![]() April 19, 1958 |
![]() February 5, 1962 |
![]() November 23, 1965 |
134 | 136 | 138 | 140 | 142 |
![]() September 11, 1969 |
![]() June 30, 1973 |
![]() April 18, 1977 |
![]() February 4, 1981 |
![]() November 22, 1984 |
144 | 146 | 148 | 150 | 152 |
![]() September 11, 1988 |
![]() June 30, 1992 |
![]() April 17, 1996 |
![]() February 5, 2000 |
![]() November 23, 2003 |
154 | 156 | |||
![]() September 11, 2007 |
![]() July 1, 2011 |
Notes[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 124". eclipse.gsfc.nasa.gov.
References[edit]
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC