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Solar eclipse of May 29, 1938

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Solar eclipse of May 29, 1938
Map
Type of eclipse
NatureTotal
Gamma−0.9607
Magnitude1.0552
Maximum eclipse
Duration245 s (4 min 5 s)
Coordinates52°42′S 22°00′W / 52.7°S 22°W / -52.7; -22
Max. width of band675 km (419 mi)
Times (UTC)
Greatest eclipse13:50:19
References
Saros146 (23 of 76)
Catalog # (SE5000)9371

A total solar eclipse occurred on May 29, 1938. 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 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]

The partial solar eclipses on February 3, 1935 and July 30, 1935 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 1935 to 1938
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
111 January 5, 1935

Partial
−1.5381 116 June 30, 1935

Partial
1.3623
121 December 25, 1935

Annular
−0.9228 126 June 19, 1936

Total
0.5389
131 December 13, 1936

Annular
−0.2493 136

Totality in Kanton Island,
Kiribati
June 8, 1937

Total
−0.2253
141 December 2, 1937

Annular
0.4389 146 May 29, 1938

Total
−0.9607
151 November 21, 1938

Partial
1.1077

References

  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.