Solar eclipse of August 31, 1932

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Solar eclipse of August 31, 1932
SE1932Aug31T.png
Map
Type of eclipse
NatureTotal
Gamma0.8307
Magnitude1.0257
Maximum eclipse
Duration105 sec (1 m 45 s)
Coordinates54°30′N 79°30′W / 54.5°N 79.5°W / 54.5; -79.5
Max. width of band155 km (96 mi)
Times (UTC)
Greatest eclipse20:03:41
References
Saros124 (50 of 73)
Catalog # (SE5000)9357
August 31, 1932 Total Solar Eclipse MEC.jpg

A total solar eclipse occurred on August 31, 1932. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Totality was visible from Northwest Territories (today's Northwest Territories and Nunavut) and Quebec in Canada, and northeastern Vermont, New Hampshire, southwestern Maine, northeastern tip of Massachusetts and northeastern Cape Cod in United States.

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 1931–1935
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 124[]

Solar saros 124, repeating every about 18 years and 11 days, contains 73 events. The series started with partial solar eclipse on March 6, 1049. It contains total eclipses from June 12, 1211, to September 22, 1968, and a hybrid solar eclipse on October 3, 1986. The series ends at member 73 as a partial eclipse on May 11, 2347. The longest total eclipse occurred on May 3, 1734, at 5 minutes and 46 seconds.[2]

Series members 43–59 occur between 1801 and 2100:
43 44 45
SE1806Jun16T.png
June 16, 1806
SE1824Jun26T.png
June 26, 1824
SE1842Jul08T.png
July 8, 1842
46 47 48
SE1860Jul18T.png
July 18, 1860
SE1878Jul29T.png
July 29, 1878
SE1896Aug09T.png
August 9, 1896
49 50 51
SE1914Aug21T.png
August 21, 1914
SE1932Aug31T.png
August 31, 1932
SE1950Sep12T.png
September 12, 1950
52 53 54
SE1968Sep22T.png
September 22, 1968
SE1986Oct03H.png
October 3, 1986
SE2004Oct14P.png
October 14, 2004
55 56 57
SE2022Oct25P.png
October 25, 2022
SE2040Nov04P.png
November 4, 2040
SE2058Nov16P.png
November 16, 2058
58 59
SE2076Nov26P.png
November 26, 2076
SE2094Dec07P.png
December 7, 2094

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 120: Total Solar Eclipse of 1816 Nov 19
  • Solar Saros 121: Hybrid Solar Eclipse of 1845 Oct 30
  • Solar Saros 122: Annular Solar Eclipse of 1874 Oct 10

In the 22nd century:

  • Solar Saros 130: Total Solar Eclipse of 2106 May 03
  • Solar Saros 131: Annular Solar Eclipse of 2135 Apr 13
  • Solar Saros 132: Hybrid Solar Eclipse of 2164 Mar 23
  • Solar Saros 133: Total Solar Eclipse of 2193 Mar 03

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).

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.
  2. ^ Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site.

References[]

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