Solar eclipse of November 13, 1993

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Solar eclipse of November 13, 1993
SE1993Nov13P.png
Map
Type of eclipse
NaturePartial
Gamma-1.0411
Magnitude0.928
Maximum eclipse
Coordinates69°36′S 58°18′E / 69.6°S 58.3°E / -69.6; 58.3
Times (UTC)
Greatest eclipse21:45:51
References
Saros123 (52 of 70)
Catalog # (SE5000)9494

A partial solar eclipse occurred on November 13–14, 1993. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth. It was visible at sunrise over parts of Australia on November 14th (Sunday), and ended at sunset over the southern tip of South America on November 13th (Saturday).

Images[]

SE1993Nov13P.gif

Related eclipses[]

Eclipses of 1993[]

  • A partial solar eclipse (north) on May 21.
  • A total lunar eclipse (central, passing north of the axis) on June 4.
  • A partial solar eclipse (south) on November 13.
  • A total lunar eclipse (south) on November 29.

Solar eclipses 1993–1996[]

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 1993–1996
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
118 1993 May 21
SE1993May21P.png
Partial
1.13720 123 1993 November 13
SE1993Nov13P.png
Partial
-1.04114
128
Solar Eclipse 1994 (7160293094).jpg
Partial from Bismarck, ND
1994 May 10
SE1994May10A.png
Annular
0.40771 133
Diamond Ring, Total Solar Eclipse, Bolivia, 1994 (3183977692).jpg
Totality at Bolivia
1994 November 3
SE1994Nov03T.png
Total
-0.35216
138 1995 April 29
SE1995Apr29A.png
Annular
-0.33821 143
Hao WLCC 941103.jpg
Totality at Dundlod, India
1995 October 24
SE1995Oct24T.png
Total
0.35176
148 1996 April 17
SE1996Apr17P.png
Partial
-1.05796 153 1996 October 12
SE1996Oct12P.png
Partial
1.12265

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.

21 eclipse events between June 21, 1982, and June 21, 2058
June 21 April 8–9 January 26 November 13–14 September 1–2
107 109 111 113 115
June 21, 1963 April 9, 1967 January 26, 1971 November 14, 1974 September 2, 1978
117 119 121 123 125
SE1982Jun21P.png
June 21, 1982
SE1986Apr09P.png
April 9, 1986
SE1990Jan26A.png
January 26, 1990
SE1993Nov13P.png
November 13, 1993
SE1997Sep02P.png
September 2, 1997
127 129 131 133 135
SE2001Jun21T.png
June 21, 2001
SE2005Apr08H.png
April 8, 2005
SE2009Jan26A.png
January 26, 2009
SE2012Nov13T.png
November 13, 2012
SE2016Sep01A.png
September 1, 2016
137 139 141 143 145
SE2020Jun21A.png
June 21, 2020
SE2024Apr08T.png
April 8, 2024
SE2028Jan26A.png
January 26, 2028
SE2031Nov14H.png
November 14, 2031
SE2035Sep02T.png
September 2, 2035
147 149 151 153 155
SE2039Jun21A.png
June 21, 2039
SE2043Apr09T.png
April 9, 2043
SE2047Jan26P.png
January 26, 2047
SE2050Nov14P.png
November 14, 2050
SE2054Sep02P.png
September 2, 2054
157
SE2058Jun21P.png
June 21, 2058

References[]

  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.

External links[]

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