Solar eclipse of October 1, 1940

Solar eclipse of October 1, 1940
Map
Type of eclipse
Nature Total
Gamma -0.2573
Magnitude 1.0645
Maximum eclipse
Duration 335 sec (5 m 35 s)
Coordinates 17°30′S 18°12′W / 17.5°S 18.2°W / -17.5; -18.2
Max. width of band 218 km (135 mi)
Times (UTC)
Greatest eclipse 12:44:06
References
Saros 133 (41 of 72)
Catalog # (SE5000) 9376

A total solar eclipse occurred on October 1, 1940. 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.

Solar eclipses 1939-1942

Each member 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.

Solar eclipse series sets from 1939-1942
Descending node   Ascending node
SarosMap SarosMap
118April 19, 1939

Annular
123October 12, 1939

Total
128April 7, 1940

Annular
133October 1, 1940

Total
138March 27, 1941

Annular
143September 21, 1941

Total
148March 16, 1942

Partial
153September 10, 1942

Partial
The partial solar eclipse on August 12, 1942 occurs in the next lunar year eclipse set.

Saros 133

Solar Saros 133, repeating every 18 years, 11 days, contains 72 events. The series started with a partial solar eclipse on July 13, 1219. It contains annular eclipses from November 20, 1435, through January 13, 1526, with a hybrid eclipse on January 24, 1544. It has total eclipses from February 3, 1562, through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. The longest duration of totality was 6 minutes, 50 seconds on August 7, 1850.[1] The total eclipses of this saros series are getting shorter and farther south with each iteration.

Notes

References

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