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Solar eclipse of October 12, 1958

A total solar eclipse occurred at the Moon's ascending node of orbit on Sunday, October 12, 1958, with a magnitude of 1.0608. 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. Totality was visible in Tokelau, Cook Islands, French Polynesia, Chile and Argentina. This solar eclipse occurred over 3 months after the final game of 1958 FIFA World Cup.

Solar eclipse of October 12, 1958
Map
Type of eclipse
NatureTotal
Gamma−0.2951
Magnitude1.0608
Maximum eclipse
Duration311 s (5 min 11 s)
Coordinates24°00′S 142°24′W / 24°S 142.4°W / -24; -142.4
Max. width of band209 km (130 mi)
Times (UTC)
Greatest eclipse20:55:28
References
Saros133 (42 of 72)
Catalog # (SE5000)9417
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Eclipses in 1958

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Solar Saros 133

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Inex

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Triad

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Solar eclipses of 1957–1960

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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 1957 to 1960
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
118 April 30, 1957
 
Annular (non-central)
0.9992 123 October 23, 1957
 
Total (non-central)
1.0022
128 April 19, 1958
 
Annular
0.275 133 October 12, 1958
 
Total
−0.2951
138 April 8, 1959
 
Annular
−0.4546 143 October 2, 1959
 
Total
0.4207
148 March 27, 1960
 
Partial
−1.1537 153 September 20, 1960
 
Partial
1.2057

Saros 133

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This eclipse is a part of Saros series 133, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on July 13, 1219. It contains annular eclipses from November 20, 1435 through January 13, 1526; a hybrid eclipse on January 24, 1544; and total eclipses from February 3, 1562 through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of annularity was produced by member 25 at 1 minutes, 14 seconds on November 30, 1453, and the longest duration of totality was produced by member 61 at 6 minutes, 50 seconds on August 7, 1850. All eclipses in this series occur at the Moon’s ascending node of orbit.[2]

Series members 34–55 occur between 1801 and 2200:
34 35 36
 
July 17, 1814
 
July 27, 1832
 
August 7, 1850
37 38 39
 
August 18, 1868
 
August 29, 1886
 
September 9, 1904
40 41 42
 
September 21, 1922
 
October 1, 1940
 
October 12, 1958
43 44 45
 
October 23, 1976
 
November 3, 1994
 
November 13, 2012
46 47 48
 
November 25, 2030
 
December 5, 2048
 
December 17, 2066
49 50 51
 
December 27, 2084
 
January 8, 2103
 
January 19, 2121
52 53 54
 
January 30, 2139
 
February 9, 2157
 
February 21, 2175
55
 
March 3, 2193

Tritos series

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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
 
December 21, 1805
(Saros 119)
 
November 19, 1816
(Saros 120)
 
October 20, 1827
(Saros 121)
 
September 18, 1838
(Saros 122)
 
August 18, 1849
(Saros 123)
 
July 18, 1860
(Saros 124)
 
June 18, 1871
(Saros 125)
 
May 17, 1882
(Saros 126)
 
April 16, 1893
(Saros 127)
 
March 17, 1904
(Saros 128)
 
February 14, 1915
(Saros 129)
 
January 14, 1926
(Saros 130)
 
December 13, 1936
(Saros 131)
 
November 12, 1947
(Saros 132)
 
October 12, 1958
(Saros 133)
 
September 11, 1969
(Saros 134)
 
August 10, 1980
(Saros 135)
 
July 11, 1991
(Saros 136)
 
June 10, 2002
(Saros 137)
 
May 10, 2013
(Saros 138)
 
April 8, 2024
(Saros 139)
 
March 9, 2035
(Saros 140)
 
February 5, 2046
(Saros 141)
 
January 5, 2057
(Saros 142)
 
December 6, 2067
(Saros 143)
 
November 4, 2078
(Saros 144)
 
October 4, 2089
(Saros 145)
 
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

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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
 
December 24, 1916
October 12, 1920  
July 31, 1924
 
May 19, 1928
 
March 7, 1932
121 123 125 127 129
 
December 25, 1935
 
October 12, 1939
 
August 1, 1943
 
May 20, 1947
 
March 7, 1951
131 133 135 137 139
 
December 25, 1954
 
October 12, 1958
 
July 31, 1962
 
May 20, 1966
 
March 7, 1970
141 143 145 147 149
 
December 24, 1973
 
October 12, 1977
 
July 31, 1981
 
May 19, 1985
 
March 7, 1989
151 153 155 157 159
 
December 24, 1992
 
October 12, 1996
 
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

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  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. ^ "NASA - Catalog of Solar Eclipses of Saros 133". eclipse.gsfc.nasa.gov.

References

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