| Solar eclipse of November 12, 1966 | |
|---|---|
|
Map
|
|
| Type of eclipse | |
| Nature | Total |
| Gamma | -0.33 |
| Magnitude | 1.0234 |
| Maximum eclipse | |
| Duration | 1m 57s |
| Coordinates | 35.6S 48.2W |
| Max. width of band | 84 km |
| Times (UTC) | |
| Greatest eclipse | 14:23:28 |
| References | |
| Saros | 142 (20 of 72) |
| Catalog # (SE5000) | 9435 |
A total solar eclipse occurred on November 12, 1966. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partially 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, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across the surface of the Earth, while a partial solar eclipse will be visible over a region thousands of kilometres wide.
The path of totality cut a swath across South America from north of Lima, Peru, nearly to the southernmost tip of Brazil.
Contents |
The NASA Gemini XII mission observed this total eclipse from space:
The Canary Island controller greeted the crew in the morning with the news that there would be a second maneuver - 5 meters forward - to line the vehicles up properly. The prospects panned out richly, and the crew reported seeing the eclipse "right on the money at 16:01:44 g.e.t." Although they thought for a moment, they were slightly off track, their aim had been accurate.[1]
This set of solar eclipses repeat approximately every 177 days and 4 hours 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.
| Ascending node | Descending node | |||
|---|---|---|---|---|
| Saros | Map | Saros | Map | |
| 117 | June 10, 1964 Partial |
122 | December 4, 1964 Partial |
|
| 127 | May 30, 1965 Total |
132 | November 23, 1965 Annular |
|
| 137 | May 20, 1966 Annular |
142 | November 12, 1966 Total |
|
| 147 | May 9, 1967 Partial |
152 | November 2, 1967 Total |
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It is a part of Saros cycle 142, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on April 17, 1624. It contains one hybrid eclipse on July 14, 1768, and total eclipses from July 25, 1786 through October 29, 2543. The series ends at member 72 as a partial eclipse on June 5, 2904. The longest duration of totality will be 6 minutes, 34 seconds on May 28, 2291.[2]
Series members 17-27 occur between 1901 and 2100:
| 17 | 18 | 19 |
|---|---|---|
October 10, 1912 |
October 21, 1930 |
November 1, 1948 |
| 20 | 21 | 22 |
November 12, 1966 |
November 22, 1984 |
December 4, 2002 |
| 23 | 24 | 25 |
December 14, 2020 |
December 26, 2038 |
January 5, 2057 |
| 26 | 27 | |
January 16, 2075 |
January 27, 2093 |
