Solar eclipse of May 29, 1938

Last updated
Solar eclipse of May 29, 1938
SE1938May29T.png
Map
Type of eclipse
NatureTotal
Gamma -0.9607
Magnitude 1.0552
Maximum eclipse
Duration245 sec (4 m 5 s)
Coordinates 52°42′S22°00′W / 52.7°S 22°W / -52.7; -22
Max. width of band675 km (419 mi)
Times (UTC)
Greatest eclipse13:50:19
References
Saros 146 (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.

Contents

This was the first of 41 umbral eclipses of Solar Saros 146. The first was in 1938 and the last will be in 2659. The total duration is 721 years.

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 1935–1938
Ascending node Descending node
111 January 5, 1935
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Partial
116 June 30, 1935
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Partial
121 December 25, 1935
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Annular
126 June 19, 1936
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Total
131 December 13, 1936
SE1936Dec13A.png
Annular
136 June 8, 1937
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Total
141 December 2, 1937
SE1937Dec02A.png
Annular
146 May 29, 1938
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Total
151 November 21, 1938
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Partial

Saros 146

It is a part of Saros cycle 146, repeating every 18 years, 11 days, containing 76 events. The series started with partial solar eclipse on September 19, 1541. It contains total eclipses from May 29, 1938 through October 7, 2154, hybrid eclipses from October 17, 2172 through November 20, 2226, and annular eclipses from December 1, 2244 through August 10, 2659. The series ends at member 76 as a partial eclipse on December 29, 2893. The longest duration of totality was 5 minutes, 21 seconds on June 30, 1992.

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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.