Solar eclipse of August 20, 1952

Last updated
Solar eclipse of August 20, 1952
SE1952Aug20A.png
Map
Type of eclipse
NatureAnnular
Gamma -0.6102
Magnitude 0.942
Maximum eclipse
Duration400 sec (6 m 40 s)
Coordinates 21°42′S64°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
Saros 144 (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.

Contents

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
SarosMapSarosMap
119 SE1950Mar18A.png
1950 March 18
Annular (non-central)
124 SE1950Sep12T.png
1950 September 12
Total
129 SE1951Mar07A.png
1951 March 7
Annular
134 SE1951Sep01A.png
1951 September 1
Annular
139 SE1952Feb25T.png
1952 February 25
Total
144 SE1952Aug20A.png
1952 August 20
Annular
149 SE1953Feb14P.png
1953 February 14
Partial
154 SE1953Aug09P.png
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.

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References