Solar eclipse of August 21, 1933

From Wikipedia, the free encyclopedia
Jump to: navigation, search
Solar eclipse of August 21, 1933
SE1933Aug21A.png
Map
Type of eclipse
Nature Annular
Gamma 0.0869
Magnitude 0.9801
Maximum eclipse
Duration 2m 4s
Coordinates 16.9N 95.9E
Max. width of band 71 km
Times (UTC)
Greatest eclipse 5:49:11
References
Saros 134 (39 of 71)
Catalog # (SE5000) 9359

An annular solar eclipse occurred on August 21, 1933. 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[edit]

Solar eclipses 1931-1935[edit]

Each member 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.

Solar eclipse series sets from 1931-1935
Descending node   Ascending node
114 September 12, 1931
SE1931Sep12P.png
Partial
119 March 7, 1932
SE1932Mar07A.png
Annular
124 August 31, 1932
SE1932Aug31T.png
Total
129 February 24, 1933
SE1933Feb24A.png
Annular
134 August 21, 1933
SE1933Aug21A.png
Annular
139 February 14, 1934
SE1934Feb14T.png
Total
144 August 10, 1934
SE1934Aug10A.png
Annular
149 February 3, 1935
SE1935Feb03P.png
Partial
154 July 30, 1935
SE1935Jul30P.png
Partial

Saros 134[edit]

It is a part of Saros cycle 134, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on June 22, 1248. It contains total eclipses from October 9, 1428 through December 24, 1554 and hybrid eclipses from January 3, 1573 through June 27, 1843, and annular eclipses from July 8, 1861 through May 21, 2384. The series ends at member 71 as a partial eclipse on August 6, 2510. The longest duration of totality was 1 minutes, 30 seconds on October 9, 1428.[1]

Series members 38-48 occur between 1901 and 2100:

38 39 40
SE1915Aug10A.png
August 10, 1915
SE1933Aug21A.png
August 21, 1933
SE1951Sep01A.png
September 1, 1951
41 42 43
SE1969Sep11A.png
September 11, 1969
SE1987Sep23A.png
September 23, 1987
SE2005Oct03A.png
October 3, 2005
44 45 46
SE2023Oct14A.png
October 14, 2023
SE2041Oct25A.png
October 25, 2041
SE2059Nov05A.png
November 5, 2059
47 48
SE2077Nov15A.png
November 15, 2077
SE2095Nov27A.png
November 27, 2095

Inex series[edit]

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 synchonization 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.

Inex series members between 1901 and 2100:

SE1904Sep09T.png
September 9, 1904
(Saros 133)
SE1933Aug21A.png
August 21, 1933
(Saros 134)
SE1962Jul31A.png
July 31, 1962
(Saros 135)
SE1991Jul11T.png
July 11, 1991
(Saros 136)
SE2020Jun21A.png
June 21, 2020
(Saros 137)
SE2049May31A.png
May 31, 2049
(Saros 138)
SE2078May11T.png
May 11, 2078
(Saros 139)

Notes[edit]

References[edit]