Solar eclipse of February 5, 1962

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Solar eclipse of February 5, 1962
SE1962Feb05T.png
Map
Type of eclipse
Nature Total
Gamma 0.2107
Magnitude 1.043
Maximum eclipse
Duration 248 sec (4 m 8 s)
Coordinates Lua error in package.lua at line 80: module 'strict' not found.
Max. width of band 147 km (91 mi)
Times (UTC)
Greatest eclipse 0:12:38
References
Saros 130 (49 of 73)
Catalog # (SE5000) 9424

A total solar eclipse occurred on February 5, 1962. 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.

Related eclipses

Solar eclipses of 1961-1964

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 1961-1964
Ascending node   Descending node
Saros Map Saros Map
120 SE1961Feb15T.png
February 15, 1961
Total
125 SE1961Aug11A.png
August 11, 1961
Annular
130 SE1962Feb05T.png
February 5, 1962
Total
135 SE1962Jul31A.png
July 31, 1962
Annular
140 SE1963Jan25A.png
January 25, 1963
Annular
145 SE1963Jul20T.png
July 20, 1963
Total
150 SE1964Jan14P.png
January 14, 1964
Partial
155 SE1964Jul09P.png
July 9, 1964
Partial
Partial solar eclipses of June 10, 1964 and December 4, 1964 belong in the next lunar year set.

Saros 130

It is a part of Saros cycle 130, repeating every 18 years, 11 days, containing 73 events. The series started with partial solar eclipse on August 20, 1096. It contains total eclipses from April 5, 1475 through July 18, 2232. The series ends at member 73 as a partial eclipse on October 25, 2394. The longest duration of totality was 6 minutes, 41 seconds on July 11, 1619.[1]

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Series members between 1901 and 2100

Series members 46-56 occur between 1901 and 2100:

46 47 48
SE1908Jan03T.png
January 3, 1908
SE1926Jan14T.png
January 14, 1926
SE1944Jan25T.png
January 25, 1944
49 50 51
SE1962Feb05T.png
February 5, 1962
SE1980Feb16T.png
February 16, 1980
SE1998Feb26T.png
February 26, 1998
52 53 54
SE2016Mar09T.png
March 9, 2016
SE2034Mar20T.png
March 20, 2034
SE2052Mar30T.png
March 30, 2052
55 56
SE2070Apr11T.png
April 11, 2070
SE2088Apr21T.png
April 21, 2088


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).

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
150px
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

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References

  1. http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros130.html