Solar eclipse of June 19, 1936
Solar eclipse of June 19, 1936 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | 0.5389 |
Magnitude | 1.0329 |
Maximum eclipse | |
Duration | 151 s (2 min 31 s) |
Coordinates | 56°06′N 104°42′E / 56.1°N 104.7°E |
Max. width of band | 132 km (82 mi) |
Times (UTC) | |
Greatest eclipse | 5:20:31 |
References | |
Saros | 126 (43 of 72) |
Catalog # (SE5000) | 9367 |
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A total solar eclipse occurred on June 19, 1936. 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. The path of totality crossed Europe and Asia. The full phase can be seen in Greece, Turkey, USSR, China and Japan. The maximum eclipse was near Bratsk and lasts about 2.5 minutes.
Related eclipses
Solar eclipses 1935-1938
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]
Solar eclipse series sets from 1935 to 1938 | ||||
---|---|---|---|---|
Ascending node | Descending node | |||
111 | January 5, 1935![]() Partial |
116 | June 30, 1935![]() Partial | |
121 | December 25, 1935![]() Annular |
126 | June 19, 1936![]() Total | |
131 | December 13, 1936![]() Annular |
136 | June 8, 1937![]() Total | |
141 | December 2, 1937![]() Annular |
146 | May 29, 1938![]() Total | |
151 | November 21, 1938![]() Partial |
Saros 126
It is a part of Saros cycle 126, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on March 10, 1179. It contains annular eclipses from June 4, 1323 through April 4, 1810, hybrid eclipses from April 14, 1828 through May 6, 1864 and total eclipses from May 17, 1882 through August 23, 2044. The series ends at member 72 as a partial eclipse on May 3, 2459. The longest duration of central eclipse (annular or total) was 6 minutes, 30 seconds of annularity on June 26, 1359. The longest duration of totality was 2 minutes, 36 seconds on July 10, 1972. All eclipses in this series occurs at the Moon’s descending node.
Series members 42–52 occur between 1901 and 2100 | ||
---|---|---|
42 | 43 | 44 |
![]() June 8, 1918 |
![]() June 19, 1936 |
![]() June 30, 1954 |
45 | 46 | 47 |
![]() July 10, 1972 |
![]() July 22, 1990 |
![]() August 1, 2008 |
48 | 49 | 50 |
![]() August 12, 2026 |
![]() August 23, 2044 |
![]() September 3, 2062 |
51 | 52 | |
![]() September 13, 2080 |
![]() September 25, 2098 |
Notes
- ^ 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.
References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
- Solar eclipse of June 19, 1936 in Russia
- Images of solar eclipse of June 19, 1936
- Map Kazakhstan
- Observing in Moscow
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