Solar eclipse of July 9, 1945
Map
Type of eclipse
NatureTotal
Gamma0.7356
Magnitude1.018
Maximum eclipse
Duration75 sec (1 m 15 s)
Coordinates70°00′N 17°12′W / 70°N 17.2°W / 70; -17.2
Max. width of band92 km (57 mi)
Times (UTC)
Greatest eclipse13:27:46
References
Saros145 (18 of 77)
Catalog # (SE5000)9387

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 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
115August 12, 1942

Partial
120February 4, 1943

Total
125August 1, 1943

Annular
130January 25, 1944

Total
135July 20, 1944

Annular
140January 14, 1945

Annular
145July 9, 1945

Total
150January 3, 1946

Partial
155June 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

  1. 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

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