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 14 (Sunday), and ended at sunset over the southern tip of South America on November 13 (Saturday).
| Solar eclipse of November 13, 1993 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Partial |
| Gamma | −1.0411 |
| Magnitude | 0.928 |
| Maximum eclipse | |
| Coordinates | 69°36′S 58°18′E / 69.6°S 58.3°E |
| Times (UTC) | |
| Greatest eclipse | 21:45:51 |
| References | |
| Saros | 123 (52 of 70) |
| Catalog # (SE5000) | 9494 |
Images edit
Related eclipses edit
Eclipses of 1993 edit
- 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 edit
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 to 1996 | ||||||
|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 118 | 1993 May 21 Partial |
1.13720 | 123 | 1993 November 13 Partial |
−1.04114 | |
128.jpg) Partial from Bismarck, ND |
1994 May 10 Annular |
0.40771 | 133.jpg) Totality at Bolivia |
1994 November 3 Total |
−0.35216 | |
| 138 | 1995 April 29 Annular |
−0.33821 | 143 Totality at Dundlod, India |
1995 October 24 Total |
0.35176 | |
| 148 | 1996 April 17 Partial |
−1.05796 | 153 | 1996 October 12 Partial |
1.12265 | |
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). 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 |
 June 21, 1982 |
 April 9, 1986 |
 January 26, 1990 |
November 13, 1993 |
 September 2, 1997 |
| 127 | 129 | 131 | 133 | 135 |
 June 21, 2001 |
 April 8, 2005 |
 January 26, 2009 |
 November 13, 2012 |
 September 1, 2016 |
| 137 | 139 | 141 | 143 | 145 |
 June 21, 2020 |
 April 8, 2024 |
 January 26, 2028 |
 November 14, 2031 |
 September 2, 2035 |
| 147 | 149 | 151 | 153 | 155 |
 June 21, 2039 |
 April 9, 2043 |
 January 26, 2047 |
 November 14, 2050 |
 September 2, 2054 |
| 157 | ||||
 June 21, 2058 | ||||
References edit
- ^ 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 edit
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