Solar eclipse of August 10, 1934

20th-century annular solar eclipse
24°30′S 34°36′E / 24.5°S 34.6°E / -24.5; 34.6Max. width of band280 km (170 mi)Times (UTC)Greatest eclipse8:37:48ReferencesSaros144 (12 of 70)Catalog # (SE5000)9361

An annular solar eclipse occurred on August 10, 1934, with an eclipse magnitude of 0.9436. 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.

Related eclipses

Solar eclipses 1931–1935

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 1931 to 1935
Descending node   Ascending node
114 September 12, 1931

Partial
119 March 7, 1932

Annular
124 August 31, 1932

Total
129 February 24, 1933

Annular
134 August 21, 1933

Annular
139 February 14, 1934

Total
144 August 10, 1934

Annular
149 February 3, 1935

Partial
154 July 30, 1935

Partial

Inex series

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings. In the 19th century:

  • Solar saros 140: total solar eclipse of October 29, 1818
  • Solar saros 141: annular solar eclipse of October 9, 1847
  • Solar saros 142: total solar eclipse of September 17, 1876
Inex series members between 1901 and 2100:

August 30, 1905
(Saros 143)

August 10, 1934
(Saros 144)

July 20, 1963
(Saros 145)

June 30, 1992
(Saros 146)

June 10, 2021
(Saros 147)

May 20, 2050
(Saros 148)

May 1, 2079
(Saros 149)

In the 22nd century:

  • Solar saros 150: partial solar eclipse of April 11, 2108
  • Solar saros 151: annular solar eclipse of March 21, 2137
  • Solar saros 152: total solar eclipse of March 2, 2166
  • Solar saros 153: annular solar eclipse of February 10, 2195

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 October 6, 2018.

References

  • Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
    • Google interactive map
    • Besselian elements
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