Solar eclipse of July 20, 1963

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Solar eclipse of July 20, 1963
Map
Type of eclipse
NatureTotal
Gamma0.6571
Magnitude1.0224
Maximum eclipse
Duration100 s (1 min 40 s)
Coordinates61°42′N 119°36′W / 61.7°N 119.6°W / 61.7; -119.6
Max. width of band101 km (63 mi)
Times (UTC)
Greatest eclipse20:36:13
References
Saros145 (19 of 77)
Catalog # (SE5000)9427

A total solar eclipse occurred on July 20, 1963. 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 at least the same size as the Sun's or larger, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with a partial solar eclipse visible over the surrounding region thousands of kilometres wide. Totality was visible from Hokkaido in Japan and Kuril Islands in Soviet Union (now belonging to Russia) on July 21, and Alaska, and Maine in the United States and also Canada on July 20. Astronomer Charles H. Smiley observed the eclipse from a U.S. Air Force F-104D Starfighter supersonic aircraft that was "racing the Moon's shadow" at 1,300 mph (2,100 km/h) extending the duration of totality to 4 minutes 3 seconds.[1] The Moon was 375,819 km (233,523 mi) from the Earth.

The Moon's apparent diameter was 4.8 arcseconds smaller than the January 25, 1963 annular solar eclipse. This was a total solar eclipse because it occurred in July when the Earth is near aphelion (furthest from the Sun). The Moon's apparent diameter was just over 2.2% larger than the Sun's.

Occurring about 4.1 days after perigee (Perigee on July 16, 1963), the Moon's apparent diameter was larger.

In popular culture[edit]

The eclipse was featured in the comic strip Peanuts (July 15–20, 1963), with Linus demonstrating a safe way of observing the eclipse as opposed to looking directly at the eclipse. On the day the eclipse passed over his area, Linus was left helplessly standing in the rain with cloud cover entirely too thick to witness the eclipse.[2]

This particular eclipse event plays an important part in two of Stephen King's novels, Gerald's Game (1992) and Dolores Claiborne (1992).[citation needed]

The eclipse is mentioned in passing in John Updike' s novel Couples (1968) in relation to Piet and Foxy.

The eclipse was featured in the season 3 episode of Mad Men entitled "Seven Twenty Three" (2009, S03E07).[3]

Related eclipses[edit]

Tzolkinex[edit]

Sar (Half-Saros), Lunar Saros 138[edit]

Tritos[edit]

Solar Saros 145[edit]

Inex[edit]

Solar eclipses of 1961–1964[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.[4]

Solar eclipse series sets from 1961 to 1964
Descending node   Ascending node
Saros Map Saros Map
120
1961 February 15
Total
125
1961 August 11
Annular
130
1962 February 5
Total
135
1962 July 31
Annular
140
1963 January 25
Annular
145
1963 July 20
Total
150
1964 January 14
Partial
155
1964 July 9
Partial
Partial solar eclipses of June 10, 1964 and December 4, 1964 belong in the next lunar year set.

Saros 145[edit]

This solar eclipse is a part of Saros cycle 145, repeating every 18 years, 11 days, 8 hours, containing 77 events. The series started with a partial solar eclipse on January 4, 1639, and reached a first annular eclipse on June 6, 1891. It was a hybrid event on June 17, 1909, and total eclipses from June 29, 1927, through September 9, 2648. The series ends at member 77 as a partial eclipse on April 17, 3009. The longest eclipse will occur on June 25, 2522, with a maximum duration of totality of 7 minutes, 12 seconds. All eclipses in this series occurs at the Moon's ascending node.

Series members 10–32 occur between 1801 and 2359
10 11 12

April 13, 1801

April 24, 1819

May 4, 1837
13 14 15

May 16, 1855

May 26, 1873

June 6, 1891
16 17 18

June 17, 1909

June 29, 1927

July 9, 1945
19 20 21

July 20, 1963

July 31, 1981

August 11, 1999
22 23 24

August 21, 2017

September 2, 2035

September 12, 2053
25 26 27

September 23, 2071

October 4, 2089

October 16, 2107
28 29 30

October 26, 2125

November 7, 2143

November 17, 2161
31 32 33

November 28, 2179

December 9, 2197

December 21, 2215
34 35 36

December 31, 2233

January 12, 2252

January 22, 2270
37 38 39

February 2, 2288

February 14, 2306

February 25, 2324
40

March 8, 2342

Inex series[edit]

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings. In the 19th century:

  • Solar saros 140: total solar eclipse of October 29, 1818
  • Solar saros 141: annular solar eclipse of October 9, 1847
  • Solar saros 142: total solar eclipse of September 17, 1876

In the 22nd century:

  • Solar saros 150: partial solar eclipse of April 11, 2108
  • Solar saros 151: annular solar eclipse of March 21, 2137
  • Solar saros 152: total solar eclipse of March 2, 2166
  • Solar saros 153: annular solar eclipse of February 10, 2195

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).

Notes[edit]

  1. ^ Smiley, Charles H. (February 1964). "Racing the Moon's Shadow on July 20, 1963". Journal of the Royal Astronomical Society of Canada. 58 (1): 10–12. Bibcode:1964JRASC..58...10S. The United States Air Force provided an F-104D, a Starfighter made by Lockheed, and Major William A. Cato piloted the plane from Kirkland Air Force Base in New Mexico to Uplands Airport, Ottawa. Since the duration of totality depends on the difference between the speed of the plane and the speed of the moon's shadow, we elected to fly north-west to meet the shadow, then turn and increase speed so that we would reach our maximum speed at 42,000 feet as the shadow overtook us and we continued to climb, attaining 48,000 feet as the shadow left us.
  2. ^ Schulz, Charles (July 20, 1963). "Peanuts by Charles Schulz for July 20, 1963 | GoComics.com". GoComics. Retrieved November 21, 2021.
  3. ^ AMC (2011). Episode 7: Seven Twenty Three (Details tab). Originally retrieved from http://www.amctv.com/shows/mad-men/episodes/season-3/seven-twenty-three. Archived on 2011-04-11 at https://web.archive.org/web/20110411231230/http://www.amctv.com/shows/mad-men/episodes/season-3/seven-twenty-three.
  4. ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved October 6, 2018.

References[edit]