Solar eclipse of December 13, 1936

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Solar eclipse of December 13, 1936
SE1936Dec13A.png
Map
Type of eclipse
NatureAnnular
Gamma-0.2493
Magnitude0.9349
Maximum eclipse
Duration445 sec (7 m 25 s)
Coordinates37°48′S 172°36′W / 37.8°S 172.6°W / -37.8; -172.6
Max. width of band251 km (156 mi)
Times (UTC)
Greatest eclipse23:28:12
References
Saros131 (46 of 70)
Catalog # (SE5000)9368

An annular solar eclipse occurred on December 13–14, 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. Annularity was visible from Australia, New Zealand on December 14th (Monday), and Oeno Island in Pitcairn Islands on December 13th (Sunday).

Related eclipses[]

Solar eclipses of 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.[1]

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[]

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. All eclipses in this series occurs at the Moon’s ascending node.

Series members 33–70 occur between 1702 and 2369
33 34 35
SE1702Jul24H.png
July 24, 1702
SE1720Aug04A.png
August 4, 1720
SE1738Aug15A.png
August 15, 1738
36 37 38
SE1756Aug25A.png
August 25, 1756
SE1774Sep06A.png
September 6, 1774
SE1792Sep16A.png
September 16, 1792
39 40 41
SE1810Sep28A.png
September 28, 1810
SE1828Oct09A.png
October 9, 1828
SE1846Oct20A.png
October 20, 1846
42 43 44
SE1864Oct30A.png
October 30, 1864
SE1882Nov10A.png
November 10, 1882
SE1900Nov22A.png
November 22, 1900
45 46 47
SE1918Dec03A.png
December 3, 1918
SE1936Dec13A.png
December 13, 1936
SE1954Dec25A.png
December 25, 1954
48 49 50
SE1973Jan04A.png
January 4, 1973
SE1991Jan15A.png
January 15, 1991
SE2009Jan26A.png
January 26, 2009
51 52 53
SE2027Feb06A.png
February 6, 2027
SE2045Feb16A.png
February 16, 2045
SE2063Feb28A.png
February 28, 2063
54 55 56
SE2081Mar10A.png
March 10, 2081
SE2099Mar21A.png
March 21, 2099
SE2117Apr02A.png
April 2, 2117
57 58 59
SE2135Apr13A.png
April 13, 2135
SE2153Apr23A.png
April 23, 2153
SE2171May05A.png
May 5, 2171
60 61 62
SE2189May15A.png
May 15, 2189
SE2207May27A.png
May 27, 2207
SE2225Jun06A.png
June 6, 2225
63 64 65
SE2243Jun18A.png
June 18, 2243
SE2261Jun28P.png
June 28, 2261
SE2279Jul09P.png
July 9, 2279
66 67 68
SE2297Jul20P.png
July 20, 2297
SE2315Aug01P.png
August 1, 2315
SE2333Aug11P.png
August 11, 2333
69 70
SE2351Aug22P.png
August 22, 2351
SE2369Sep02P.png
September 2, 2369

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.

Tritos series[]

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.

Series members between 1801 and 2100
SE1805Dec21A.gif
December 21, 1805
(Saros 119)
SE1816Nov19T.gif
November 19, 1816
(Saros 120)
SE1827Oct20H.gif
October 20, 1827
(Saros 121)
SE1838Sep18A.gif
September 18, 1838
(Saros 122)
SE1849Aug18T.gif
August 18, 1849
(Saros 123)
SE1860Jul18T.gif
July 18, 1860
(Saros 124)
SE1871Jun18A.gif
June 18, 1871
(Saros 125)
SE1882May17T.png
May 17, 1882
(Saros 126)
SE1893Apr16T.png
April 16, 1893
(Saros 127)
SE1904Mar17A.png
March 17, 1904
(Saros 128)
SE1915Feb14A.png
February 14, 1915
(Saros 129)
SE1926Jan14T.png
January 14, 1926
(Saros 130)
SE1936Dec13A.png
December 13, 1936
(Saros 131)
SE1947Nov12A.png
November 12, 1947
(Saros 132)
SE1958Oct12T.png
October 12, 1958
(Saros 133)
SE1969Sep11A.png
September 11, 1969
(Saros 134)
SE1980Aug10A.png
August 10, 1980
(Saros 135)
SE1991Jul11T.png
July 11, 1991
(Saros 136)
SE2002Jun10A.png
June 10, 2002
(Saros 137)
SE2013May10A.png
May 10, 2013
(Saros 138)
SE2024Apr08T.png
April 8, 2024
(Saros 139)
SE2035Mar09A.png
March 9, 2035
(Saros 140)
SE2046Feb05A.png
February 5, 2046
(Saros 141)
SE2057Jan05T.png
January 5, 2057
(Saros 142)
SE2067Dec06H.png
December 6, 2067
(Saros 143)
SE2078Nov04A.png
November 4, 2078
(Saros 144)
SE2089Oct04T.png
October 4, 2089
(Saros 145)
SE2100Sep04T.png
September 4, 2100
(Saros 146)

In the 22nd century:

  • Solar saros 147: annular solar eclipse of August 4, 2111
  • Solar saros 148: total solar eclipse of July 4, 2122
  • Solar saros 149: total solar eclipse of June 3, 2133
  • Solar saros 150: annular solar eclipse of May 3, 2144
  • Solar saros 151: annular solar eclipse of April 2, 2155
  • Solar saros 152: total solar eclipse of March 2, 2166
  • Solar saros 153: annular solar eclipse of January 29, 2177
  • Solar saros 154: annular solar eclipse of December 29, 2187
  • Solar saros 155: total solar eclipse of November 28, 2198

In the 23rd century:

  • Solar saros 156: annular solar eclipse of October 29, 2209
  • Solar saros 157: annular solar eclipse of September 27, 2220
  • Solar saros 158: total solar eclipse of August 28, 2231
  • Solar saros 159: partial solar eclipse of July 28, 2242
  • Solar saros 160: partial solar eclipse of June 26, 2253
  • Solar saros 161: partial solar eclipse of May 26, 2264
  • Solar saros 162: partial solar eclipse of April 26, 2275
  • Solar saros 163: partial solar eclipse of March 25, 2286
  • Solar saros 164: partial solar eclipse of February 22, 2297

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.

References[]

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