Solar eclipse of November 12, 1966

Last updated
Solar eclipse of November 12, 1966
SE1966Nov12T.png
Map
Type of eclipse
NatureTotal
Gamma −0.33
Magnitude 1.0234
Maximum eclipse
Duration117 s (1 min 57 s)
Coordinates 35°36′S48°12′W / 35.6°S 48.2°W / -35.6; -48.2
Max. width of band84 km (52 mi)
Times (UTC)
Greatest eclipse14:23:28
References
Saros 142 (20 of 72)
Catalog # (SE5000) 9435
The eclipse as viewed from Gemini XII Gemini XII Mission Image - Solar Eclipse.jpg
The eclipse as viewed from Gemini XII

A total solar eclipse occurred on Saturday, [1] November 12, 1966. 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. The path of totality cut a swath across South America from north of Lima, Peru, passing the northeastern tip of Chile, Bolivia, Northwest of Argentina, southwestern tip of Ñeembucú Department in Paraguay, nearly to the southernmost tip of Brazil.

Contents

Observations

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 the crew thought for a moment that they were slightly off track, their aim had actually been accurate. [2]

The 28 October 1966 launch of the U.S. Air Force's Orbiting Vehicle 3-2 (OV3-2) was timed such that it could observe ambient charged particle variations before, during, and after the eclipse. [3]

Solar eclipses of 1964–1967

This eclipse is a member of a 1964–1967 series at alternating nodes every 6 synodic months.

Note: Partial solar eclipses on January 14, 1964 and July 9, 1964 belong to the previous lunar year set.

Solar eclipse series sets from 1964 to 1967
Ascending node Descending node
SarosMapGammaSarosMapGamma
117 SE1964Jun10P.png
1964 June 10
Partial
−1.13926122 SE1964Dec04P.png
1964 December 4
Partial
1.11929
127 SE1965May30T.png
1965 May 30
Total
−0.42251132 SE1965Nov23A.png
1965 November 23
Annular
0.39061
137 SE1966May20A.png
1966 May 20
Annular
0.34672142 SE1966Nov12T.png
1966 November 12
Total
−0.33001
147 SE1967May09P.png
1967 May 9
Partial
1.14218152 SE1967Nov02T.png
1967 November 2
Total (non-central)
−1.00067

Saros series 142

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. All eclipses in this series occurs at the Moon’s descending node. [4]

Series members 17–41 occur between 1901 and 2359
171819
SE1912Oct10T.png
October 10, 1912
SE1930Oct21T.png
October 21, 1930
SE1948Nov01T.png
November 1, 1948
202122
SE1966Nov12T.png
November 12, 1966
SE1984Nov22T.png
November 22, 1984
SE2002Dec04T.png
December 4, 2002
232425
SE2020Dec14T.png
December 14, 2020
SE2038Dec26T.png
December 26, 2038
SE2057Jan05T.png
January 5, 2057
262728
SE2075Jan16T.png
January 16, 2075
SE2093Jan27T.png
January 27, 2093
SE2111Feb08T.png
February 8, 2111
293031
SE2129Feb18T.png
February 18, 2129
SE2147Mar02T.png
March 2, 2147
SE2165Mar12T.png
March 12, 2165
323334
SE2183Mar23T.png
March 23, 2183
SE2201Apr04T.png
April 4, 2201
SE2219Apr15T.png
April 15, 2219
353637
SE2237Apr25T.png
April 25, 2237
SE2255May07T.png
May 7, 2255
SE2273May17T.png
May 17, 2273
383940
SE2291May28T.png
May 28, 2291
SE2309Jun09T.png
June 9, 2309
SE2327Jun20T.png
June 20, 2327
41
SE2345Jun30T.png
June 30, 2345

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).

Notes

  1. https://www.calendar-365.com/1966-calendar.html
  2. "Gemini 12". Archived from the original on 2012-09-22.
  3. "OV3-2". NASA. Retrieved 27 September 2021.
  4. http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros142.html

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References