Solar eclipse of August 20, 1952
Map
Type of eclipse
NatureAnnular
Gamma−0.6102
Magnitude0.942
Maximum eclipse
Duration400 sec (6 m 40 s)
Coordinates21°42′S 64°06′W / 21.7°S 64.1°W / -21.7; -64.1
Max. width of band264 km (164 mi)
Times (UTC)
Greatest eclipse15:13:35
References
Saros144 (13 of 70)
Catalog # (SE5000)9403

An annular solar eclipse occurred on August 20, 1952. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Annularity was visible from Peru including the capital city Lima, northeastern Chile, Bolivia including the constitutional capital Sucre and seat of government La Paz, Argentina, Paraguay, southern Brazil and Uruguay.

Solar eclipses of 1950–1953

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 1950–1953
Ascending node   Descending node
SarosMap SarosMap
119
1950 March 18
Annular (non-central)		 124
1950 September 12
Total
129
1951 March 7
Annular		 134
1951 September 1
Annular
139
1952 February 25
Total		 144
1952 August 20
Annular
149
1953 February 14
Partial		 154
1953 August 9
Partial
Solar eclipse of July 11, 1953 belongs to the next lunar year set

Saros 144

It is a part of Saros cycle 144, repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on April 11, 1736. It contains annular eclipses from July 7, 1880, through August 27, 2565. There are no total eclipses in the series. The series ends at member 70 as a partial eclipse on May 5, 2980. The longest duration of annularity will be 9 minutes, 52 seconds on December 29, 2168.

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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