Solar eclipse of November 23, 1965

From Wikipedia, the free encyclopedia
Jump to: navigation, search
Solar eclipse of November 23, 1965
SE1965Nov23A.png
Map
Type of eclipse
Nature Annular
Gamma 0.3906
Magnitude 0.9656
Maximum eclipse
Duration 4m 2s
Coordinates 1.7N 119.8E
Max. width of band 134 km
Times (UTC)
Greatest eclipse 4:14:51
References
Saros 132 (43 of 71)
Catalog # (SE5000) 9433

An annual solar eclipse occurred on November 23, 1965. 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 1964-1967[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.

Note: Partial solar eclipses on January 14, 1964 and July 9, 1964 belong to the previous lunar year set.

Solar eclipse series sets from 1964-1967
Ascending node   Descending node
Saros Map Saros Map
117 SE1964Jun10P.png
June 10, 1964
Partial
122 SE1964Dec04P.png
December 4, 1964
Partial
127 SE1965May30T.png
May 30, 1965
Total
132 SE1965Nov23A.png
November 23, 1965
Annular
137 SE1966May20A.png
May 20, 1966
Annular
142 SE1966Nov12T.png
November 12, 1966
Total
147 SE1967May09P.png
May 9, 1967
Partial
152 SE1967Nov02T.png
November 2, 1967
Total

Saros 132[edit]

It is a part of Saros cycle 132, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on August 13, 1208. It contains annular eclipses from March 17, 1569 through March 12, 2146, hybrid on March 23, 2164 and April 3, 2183 and total eclipses from April 14, 2200 through June 19, 2308. The series ends at member 71 as a partial eclipse on September 25, 2470. The longest duration of annular was 4 minutes, 2 seconds on 1965 Nov 23, and totality will be 2 minutes, 14 seconds on May 27, 2272.[1]

Series members 40-50 occur between 1901 and 2100:

40 41 42
SE1911Oct22A.png
October 22, 1911
SE1929Nov01A.png
November 1, 1929
SE1947Nov12A.png
November 12, 1947
43 44 45
SE1965Nov23A.png
November 23, 1965
SE1983Dec04A.png
December 4, 1983
SE2001Dec14A.png
December 14, 2001
46 47 48
SE2019Dec26A.png
December 26, 2019
SE2038Jan05A.png
January 5, 2038
SE2056Jan16A.png
January 16, 2056
49 50
SE2074Jan27A.png
January 27, 2074
SE2092Feb07A.png
February 7, 2092

Metonic series[edit]

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).

This series has 22 eclipse events between September 12, 1931 and July 1, 2011.

September 11-12 June 30-July 1 April 18-19 February 4-5 November 22-23
114 116 118 120 122
SE1931Sep12P.png
September 12, 1931
SE1935Jun30P.png
June 30, 1935
SE1939Apr19A.png
April 19, 1939
SE1943Feb04T.png
February 4, 1943
SE1946Nov23P.png
November 23, 1946
124 126 128 130 132
SE1950Sep12T.png
September 12, 1950
SE1954Jun30T.png
June 30, 1954
SE1958Apr19A.png
April 19, 1958
SE1962Feb05T.png
February 5, 1962
SE1965Nov23A.png
November 23, 1965
134 136 138 140 142
SE1969Sep11A.png
September 11, 1969
SE1973Jun30T.png
June 30, 1973
SE1977Apr18A.png
April 18, 1977
SE1981Feb04A.png
February 4, 1981
SE1984Nov22T.png
November 22, 1984
144 146 148 150 152
SE1988Sep11A.png
September 11, 1988
SE1992Jun30T.png
June 30, 1992
SE1996Apr17P.png
April 17, 1996
SE2000Feb05P.png
February 5, 2000
SE2003Nov23T.png
November 23, 2003
154 156
SE2007Sep11P.png
September 11, 2007
SE2011Jul01P.png
July 1, 2011

Notes[edit]

References[edit]