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Solar eclipse of January 5, 1935

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Solar eclipse of January 5, 1935
Map
Type of eclipse
NaturePartial
Gamma-1.5381
Magnitude0.0013
Maximum eclipse
Coordinates64°42′S 110°12′W / 64.7°S 110.2°W / -64.7; -110.2
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Times (UTC)
Greatest eclipse5:35:46
References
Saros111 (79 of 79)
Catalog # (SE5000)9363

A partial solar eclipse occurred on January 5, 1935 during summer. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

Description

It was one of five eclipses that took place that year, the next one was on February 3 and covered much of North America.

It was the last eclipse of solar saros 111 with the Moon's penumbra touching the Earth for just 10 minutes.[1] The next mini eclipse in 296 years, the last solar eclipse that was very short occurred on January 4, 1639 and had a magnitude of 0.0009 and lasted for about 7 minutes.

As is shown under 1% obscuration, the center of the Moon's shadow was missed by about 2,825 km above the area (64.7S) north of the Antarctic Circle.

The mini-eclipse took place hundreds of kilometers offshore from Antarctica in the Pacific Ocean, at the fifth minute, the greatest eclipse occurred at 5:35:45 UTC (22:45 local time) at 64.7S and 110.2 W.

As the Moon moved towards the right, in that part of Antarctica north of the South Pole at the 110th meridian west, it was seen as it was moved towards the right as the axis spun south of 66.5 S, the Antarctic Circle.

The eclipse was the shortest in the 20th century.

Related eclipses

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.[2]

Solar eclipse series sets from 1935–1938
Ascending node   Descending node
111 January 5, 1935

Partial
116 June 30, 1935

Partial
121 December 25, 1935

Annular
126 June 19, 1936

Total
131 December 13, 1936

Annular
136 June 8, 1937

Total
141 December 2, 1937

Annular
146 May 29, 1938

Total
151 November 21, 1938

Partial

Metonic series

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's ascending node.

22 eclipse events between January 5, 1935 and August 11, 2018
January 4-5 October 23-24 August 10-12 May 30-31 March 18-19
111 113 115 117 119

January 5, 1935
File:SE1942Aug12P.png
August 12, 1942
File:SE1946May30P.png
May 30, 1946
File:SE1950Mar18A.png
March 18, 1950
121 123 125 127 129
File:SE1954Jan05A.png
January 5, 1954
File:SE1957Oct23T.png
October 23, 1957
File:SE1961Aug11A.png
August 11, 1961
File:SE1965May30T.png
May 30, 1965
File:SE1969Mar18A.png
March 18, 1969
131 133 135 137 139
File:SE1973Jan04A.png
January 4, 1973
File:SE1976Oct23T.png
October 23, 1976
File:SE1980Aug10A.png
August 10, 1980
File:SE1984May30A.png
May 30, 1984
File:SE1988Mar18T.png
March 18, 1988
141 143 145 147 149
File:SE1992Jan04A.png
January 4, 1992
File:SE1995Oct24T.png
October 24, 1995
File:SE1999Aug11T.png
August 11, 1999
File:SE2003May31A.png
May 31, 2003
File:SE2007Mar19P.png
March 19, 2007
151 153 155
File:SE2011Jan04P.png
January 4, 2011
File:SE2014Oct23P.png
October 23, 2014
File:SE2018Aug11P.png
August 11, 2018

References

  1. "Partial Solar Eclipse of 1935 Jan 05". eclipse.gsfc.nasa.gov. Retrieved 15 October 2021.
  2. 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.

External links


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