Solar eclipse of December 13, 1936

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Solar eclipse of December 13, 1936
SE1936Dec13A.png
Map
Type of eclipse
Nature Annular
Gamma -0.2493
Magnitude 0.9349
Maximum eclipse
Duration 445 sec (7 m 25 s)
Coordinates 37°48′S 172°36′W / 37.8°S 172.6°W / -37.8; -172.6
Max. width of band 251 km (156 mi)
Times (UTC)
Greatest eclipse 23:28:12
References
Saros 131 (46 of 70)
Catalog # (SE5000) 9368

An annular solar eclipse occurred on December 13, 1936. 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 of 1935-1938[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 1935-1938
Ascending node   Descending node
111 January 5, 1935
SE1935Jan05P.png
Partial
116 June 30, 1935
SE1935Jun30P.png
Partial
121 December 25, 1935
SE1935Dec25A.png
Annular
126 June 19, 1936
SE1936Jun19T.png
Total
131 December 13, 1936
SE1936Dec13A.png
Annular
136 June 8, 1937
SE1937Jun08T.png
Total
141 December 2, 1937
SE1937Dec02A.png
Annular
146 May 29, 1938
SE1938May29T.png
Total
151 November 21, 1938
SE1938Nov21P.png
Partial

Saros 131[edit]

It is a part of Saros cycle 131, repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on August 1, 1125. It contains total eclipses from March 27, 1522 through May 30, 1612 and hybrid eclipses from June 10, 1630 through July 24, 1702, and annular eclipses from August 4, 1720 through June 18, 2243. The series ends at member 70 as a partial eclipse on September 2, 2369. The longest duration of totality was only 58 seconds on May 30, 1612.[1]

Tritos series[edit]

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Notes[edit]

References[edit]