Solar eclipse of December 25, 1935

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Solar eclipse of December 25, 1935
SE1935Dec25A.png
Map
Type of eclipse
NatureAnnular
Gamma-0.9228
Magnitude0.9752
Maximum eclipse
Duration90 sec (1 m 30 s)
Coordinates83°30′S 9°24′E / 83.5°S 9.4°E / -83.5; 9.4
Max. width of band234 km (145 mi)
Times (UTC)
Greatest eclipse17:59:52
References
Saros121 (56 of 71)
Catalog # (SE5000)9366

An annular solar eclipse occurred on December 25, 1935. 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. This was the 5th solar eclipse in 1935, the maximum possible. The next time this will occur is 2206.

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.[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 121[]

Solar saros 121, repeating every about 18 years, 11 days, and 8 hours, contains 71 events. The series started with a partial solar eclipse on April 25, 944. It contains total eclipses from July 10, 1070, to October 9, 1809. It contains hybrid eclipses on October 20, 1827, and October 30, 1845. It contains annular eclipses from November 11, 1863, to February 28, 2044. The series ends at member 71 as a partial eclipse on June 7, 2206. The longest total eclipse occurred on June 21, 1629, with greatest duration of totality at 6 minutes and 20 seconds. The longest annular eclipse will occur on February 28, 2044, with greatest duration of annularity at 2 minutes and 27 seconds.[2]

Series members 49–65 occur between 1801 and 2100:
49 50 51
SE1809Oct09T.gif
October 9, 1809
SE1827Oct20H.gif
October 20, 1827
SE1845Oct30H.gif
October 30, 1845
52 53 54
SE1863Nov11A.gif
November 11, 1863
SE1881Nov21A.gif
November 21, 1881
SE1899Dec03A.gif
December 3, 1899
55 56 57
SE1917Dec14A.png
December 14, 1917
SE1935Dec25A.png
December 25, 1935
SE1954Jan05A.png
January 5, 1954
58 59 60
SE1972Jan16A.png
January 16, 1972
SE1990Jan26A.png
January 26, 1990
SE2008Feb07A.png
February 7, 2008
61 62 63
SE2026Feb17A.png
February 17, 2026
SE2044Feb28A.png
February 28, 2044
SE2062Mar11P.png
March 11, 2062
64 65
SE2080Mar21P.png
March 21, 2080
SE2098Apr01P.png
April 1, 2098

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.

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 December 24, 1916 and July 31, 2000
December 24–25 October 12–13 July 31-Aug 1 May 18–20 March 7–8
91 93 95 97 99
December 23, 1878 October 12, 1882 July 31, 1886 May 18, 1890 March 7, 1894
101 103 105 107 109
December 23, 1897 October 12, 1901 August 1, 1905 May 19, 1909 March 8, 1913
111 113 115 117 119
SE1916Dec24P.png
December 24, 1916
October 12, 1920 SE1924Jul31P.png
July 31, 1924
SE1928May19T.png
May 19, 1928
SE1932Mar07A.png
March 7, 1932
121 123 125 127 129
SE1935Dec25A.png
December 25, 1935
SE1939Oct12T.png
October 12, 1939
SE1943Aug01A.png
August 1, 1943
SE1947May20T.png
May 20, 1947
SE1951Mar07A.png
March 7, 1951
131 133 135 137 139
SE1954Dec25A.png
December 25, 1954
SE1958Oct12T.png
October 12, 1958
SE1962Jul31A.png
July 31, 1962
SE1966May20A.png
May 20, 1966
SE1970Mar07T.png
March 7, 1970
141 143 145 147 149
SE1973Dec24A.png
December 24, 1973
SE1977Oct12T.png
October 12, 1977
SE1981Jul31T.png
July 31, 1981
SE1985May19P.png
May 19, 1985
SE1989Mar07P.png
March 7, 1989
151 153 155 157 159
SE1992Dec24P.png
December 24, 1992
SE1996Oct12P.png
October 12, 1996
SE2000Jul31P.png
July 31, 2000
May 19, 2004 March 7, 2008
161 163 165 167 169
December 24, 2011 October 13, 2015 August 1, 2019 May 19, 2023 March 8, 2027

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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