Solar eclipse of July 9, 1945
A total solar eclipse occurred on July 9, 1945. 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 northern North America, across Greenland and into Scandinavia, the western Soviet Union, and central Asia.
| Solar eclipse of July 9, 1945 | |
|---|---|
|  Map | |
| Type of eclipse | |
| Nature | Total | 
| Gamma | 0.7356 | 
| Magnitude | 1.018 | 
| Maximum eclipse | |
| Duration | 75 sec (1 m 15 s) | 
| Coordinates | 70°N 17.2°W | 
| Max. width of band | 92 km (57 mi) | 
| Times (UTC) | |
| Greatest eclipse | 13:27:46 | 
| References | |
| Saros | 145 (18 of 77) | 
| Catalog # (SE5000) | 9387 | 
Related eclipses
    
    Solar eclipses 1942–1946
    
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]
Note: The partial solar eclipse on September 10, 1942 occurs in the previous lunar year eclipse set.
| Solar eclipse series sets from 1942–1946 | ||||
|---|---|---|---|---|
| Ascending node | Descending node | |||
| 115 | August 12, 1942  Partial | 120 | February 4, 1943  Total | |
| 125 | August 1, 1943  Annular | 130 | January 25, 1944  Total | |
| 135 | July 20, 1944  Annular | 140 | January 14, 1945  Annular | |
| 145 | July 9, 1945  Total | 150 | January 3, 1946  Partial | |
| 155 | June 29, 1946  Partial | |||
Saros 145
    
This solar eclipse is a part of Saros cycle 145, repeating every 18 years, 11 days, 8 hours, containing 77 events. The series started with a partial solar eclipse on January 4, 1639, and reached a first annular eclipse on June 6, 1891. It was a hybrid event on June 17, 1909, and total eclipses from June 29, 1927, through September 9, 2648. The series ends at member 77 as a partial eclipse on April 17, 3009. The longest eclipse will occur on June 25, 2522, with a maximum duration of totality of 7 minutes, 12 seconds. All eclipses in this series occurs at the Moon's ascending node.
| Series members 10–32 occur between 1801 and 2359 | ||
|---|---|---|
| 10 | 11 | 12 | 
|  April 13, 1801 |  April 24, 1819 |  May 4, 1837 | 
| 13 | 14 | 15 | 
|  May 16, 1855 |  May 26, 1873 |  June 6, 1891 | 
| 16 | 17 | 18 | 
|  June 17, 1909 |  June 29, 1927 |  July 9, 1945 | 
| 19 | 20 | 21 | 
|  July 20, 1963 |  July 31, 1981 |  August 11, 1999 | 
| 22 | 23 | 24 | 
|  August 21, 2017 |  September 2, 2035 |  September 12, 2053 | 
| 25 | 26 | 27 | 
|  September 23, 2071 |  October 4, 2089 |  October 16, 2107 | 
| 28 | 29 | 30 | 
|  October 26, 2125 |  November 7, 2143 |  November 17, 2161 | 
| 31 | 32 | 33 | 
|  November 28, 2179 |  December 9, 2197 |  December 21, 2215 | 
| 34 | 35 | 36 | 
|  December 31, 2233 |  January 12, 2252 |  January 22, 2270 | 
| 37 | 38 | 39 | 
|  February 2, 2288 |  February 14, 2306 |  February 25, 2324 | 
| 40 | ||
|  March 8, 2342 | ||
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
- Вьюшков П.В. (1945). Солнечное затмение 9 июля 1945 года [Solar eclipse of July 9, 1945] (PDF) (in Russian). Saratov: Saratov State University.

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