Solar eclipse of August 20, 1952

20th-century annular solar eclipse
21°42′S 64°06′W / 21.7°S 64.1°W / -21.7; -64.1Max. width of band264 km (164 mi)Times (UTC)Greatest eclipse15:13:35ReferencesSaros144 (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.

Related eclipses

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 to 1953
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
119
1950 March 18
Annular (non-central)
-0.99880 124
1950 September 12
Total
0.89030
129
1951 March 7
Annular
-0.24196 134
1951 September 1
Annular
0.15570
139
1952 February 25
Total
0.46973 144
1952 August 20
Annular
-0.61023
149
1953 February 14
Partial
1.13308 154
1953 August 9
Partial
-1.34403
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.

Series members 11–21 occur between 1901 and 2100:
11 12 13

Jul 30, 1916

Aug 10, 1934

Aug 20, 1952
14 15 16

Aug 31, 1970

Sep 11, 1988

Sep 22, 2006
17 18 19

Oct 2, 2024

Oct 14, 2042

Oct 24, 2060
20 21

Nov 4, 2078

Nov 15, 2096

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

  • Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
    • Google interactive map
    • Besselian elements
  • v
  • t
  • e
FeaturesLists of eclipses
By era
Saros series (list)
Visibility
Historical
21 August 2017 total solar eclipse
Total/hybrid eclipses
next total/hybrid
10 May 2013 annular eclipse
Annular eclipses
next annular
23 October 2014 partial eclipse
Partial eclipses
next partial
Other bodiesRelated
  • Astronomy portal
  • Solar System portal
  • Category
Stub icon

This solar eclipse–related article is a stub. You can help Wikipedia by expanding it.

  • v
  • t
  • e