Solar eclipse of July 10, 1972

A total solar eclipse occurred at the Moon's descending node of orbit between Monday, July 10 and Tuesday, July 11, 1972,[1] with a magnitude of 1.0379. 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. Occurring about 2.8 days after perigee (on July 7, 1972, at 23:50 UTC), the Moon's apparent diameter was larger.[2]

Solar eclipse of July 10, 1972
Map
Type of eclipse
NatureTotal
Gamma0.6872
Magnitude1.0379
Maximum eclipse
Duration156 s (2 min 36 s)
Coordinates63°30′N 94°12′W / 63.5°N 94.2°W / 63.5; -94.2
Max. width of band175 km (109 mi)
Times (UTC)
Greatest eclipse19:46:38
References
Saros126 (45 of 72)
Catalog # (SE5000)9448

It was visible as a total eclipse along a path of totality that began in Sea of Okhotsk and traversed the far eastern portions of the Soviet Union (which now belongs to Russia) on July 11 local time, northern Alaska in the United States, Northern Canada, eastern Quebec and the Canadian Maritimes on July 10 local time. A partial eclipse was visible for parts of the northern Soviet Union, North America, the Caribbean, northern South America, and Northern Europe.

The eclipse was mostly seen on July 10, 1972, except for the Asian part of Soviet Union and Japanese island Hokkaido, where either a partial or a total eclipse was seen on July 11 local time, and part of the Soviet Union along the coast of Kara Sea, where a partial eclipse started on July 10, passing midnight and ended on July 11 due to the midnight sun.

Observations

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A team of the Academy of Sciences of the Soviet Union observed the total solar eclipse in Russkaya Koshka, Magadan Oblast (now separated into Chukotka Autonomous Okrug) on the coast of Gulf of Anadyr. The weather condition was clear, and the team successfully took images of the corona and made polarization observations to study its structure and physical characteristics.[3] In Nova Scotia, Canada, the eclipse was clouded out and could not be observed. Besides that, 850 passengers boarded a cruise ship from New York City and saw a total eclipse successfully in North Atlantic Ocean. Many scientists also boarded the ship and did research, and some also gave classes in meteorology, oceanography, etc., which almost all passengers attended.[4][5]

"You're So Vain"

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The eclipse is referenced in the lyrics of Carly Simon's 1972 hit song "You're So Vain."[6] The subject of the song, after witnessing his racehorse win "naturally" at the Saratoga Race Course, flies his Learjet to Nova Scotia to see the eclipse; Simon uses the two phenomena as examples of how the subject seems to be "where (he) should be all the time." Simon released the song four months after the eclipse.[7]

Eclipse details

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Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.[8]

July 10, 1972 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 1972 July 10 at 17:19:47.5 UTC
First Umbral External Contact 1972 July 10 at 18:28:23.8 UTC
First Central Line 1972 July 10 at 18:29:24.0 UTC
First Umbral Internal Contact 1972 July 10 at 18:30:24.5 UTC
Equatorial Conjunction 1972 July 10 at 19:29:05.3 UTC
Ecliptic Conjunction 1972 July 10 at 19:39:28.3 UTC
Greatest Duration 1972 July 10 at 19:43:47.8 UTC
Greatest Eclipse 1972 July 10 at 19:46:38.1 UTC
Last Umbral Internal Contact 1972 July 10 at 21:03:06.0 UTC
Last Central Line 1972 July 10 at 21:04:04.1 UTC
Last Umbral External Contact 1972 July 10 at 21:05:01.8 UTC
Last Penumbral External Contact 1972 July 10 at 22:13:41.2 UTC
July 10, 1972 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 1.03790
Eclipse Obscuration 1.07723
Gamma 0.68719
Sun Right Ascension 07h20m39.3s
Sun Declination 22°08'59.1"
Sun Semi-Diameter 15'43.9"
Sun Equatorial Horizontal Parallax 08.6"
Moon Right Ascension 07h21m20.3s
Moon Declination 22°48'27.6"
Moon Semi-Diameter 16'08.2"
Moon Equatorial Horizontal Parallax 0°59'13.3"
ΔT 42.8 s

Eclipse season

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This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.

Eclipse season of July 1972
July 10
Descending node (new moon)
July 26
Ascending node (full moon)
   
Total solar eclipse
Solar Saros 126
Partial lunar eclipse
Lunar Saros 138
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Eclipses in 1972

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Solar Saros 126

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Inex

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Triad

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Solar eclipses of 1971–1974

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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.[9]

The partial solar eclipses on February 25, 1971 and August 20, 1971 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 1971 to 1974
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
116 July 22, 1971
 
Partial
1.513 121 January 16, 1972
 
Annular
−0.9365
126 July 10, 1972
 
Total
0.6872 131 January 4, 1973
 
Annular
−0.2644
136 June 30, 1973
 
Total
−0.0785 141 December 24, 1973
 
Annular
0.4171
146 June 20, 1974
 
Total
−0.8239 151 December 13, 1974
 
Partial
1.0797

Saros 126

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This eclipse is a part of Saros series 126, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on March 10, 1179. It contains annular eclipses from June 4, 1323 through April 4, 1810; hybrid eclipses from April 14, 1828 through May 6, 1864; and total eclipses from May 17, 1882 through August 23, 2044. The series ends at member 72 as a partial eclipse on May 3, 2459. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of annularity was produced by member 11 at 6 minutes, 30 seconds on June 26, 1359, and the longest duration of totality was produced by member 45 at 2 minutes, 36 seconds on July 10, 1972. All eclipses in this series occur at the Moon’s descending node of orbit.[10]

Series members 36–57 occur between 1801 and 2200:
36 37 38
 
April 4, 1810
 
April 14, 1828
 
April 25, 1846
39 40 41
 
May 6, 1864
 
May 17, 1882
 
May 28, 1900
42 43 44
 
June 8, 1918
 
June 19, 1936
 
June 30, 1954
45 46 47
 
July 10, 1972
 
July 22, 1990
 
August 1, 2008
48 49 50
 
August 12, 2026
 
August 23, 2044
 
September 3, 2062
51 52 53
 
September 13, 2080
 
September 25, 2098
 
October 6, 2116
54 55 56
 
October 17, 2134
 
October 28, 2152
 
November 8, 2170
57
 
November 18, 2188

Metonic series

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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 descending node.

21 eclipse events between July 11, 1953 and July 11, 2029
July 10–11 April 29–30 February 15–16 December 4 September 21–23
116 118 120 122 124
 
July 11, 1953
 
April 30, 1957
 
February 15, 1961
 
December 4, 1964
 
September 22, 1968
126 128 130 132 134
 
July 10, 1972
 
April 29, 1976
 
February 16, 1980
 
December 4, 1983
 
September 23, 1987
136 138 140 142 144
 
July 11, 1991
 
April 29, 1995
 
February 16, 1999
 
December 4, 2002
 
September 22, 2006
146 148 150 152 154
 
July 11, 2010
 
April 29, 2014
 
February 15, 2018
 
December 4, 2021
 
September 21, 2025
156
 
July 11, 2029

Tritos series

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This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200
 
October 19, 1808
(Saros 111)
 
September 19, 1819
(Saros 112)
 
August 18, 1830
(Saros 113)
 
July 18, 1841
(Saros 114)
 
June 17, 1852
(Saros 115)
 
May 17, 1863
(Saros 116)
 
April 16, 1874
(Saros 117)
 
March 16, 1885
(Saros 118)
 
February 13, 1896
(Saros 119)
 
January 14, 1907
(Saros 120)
 
December 14, 1917
(Saros 121)
 
November 12, 1928
(Saros 122)
 
October 12, 1939
(Saros 123)
 
September 12, 1950
(Saros 124)
 
August 11, 1961
(Saros 125)
 
July 10, 1972
(Saros 126)
 
June 11, 1983
(Saros 127)
 
May 10, 1994
(Saros 128)
 
April 8, 2005
(Saros 129)
 
March 9, 2016
(Saros 130)
 
February 6, 2027
(Saros 131)
 
January 5, 2038
(Saros 132)
 
December 5, 2048
(Saros 133)
 
November 5, 2059
(Saros 134)
 
October 4, 2070
(Saros 135)
 
September 3, 2081
(Saros 136)
 
August 3, 2092
(Saros 137)
 
July 4, 2103
(Saros 138)
 
June 3, 2114
(Saros 139)
 
May 3, 2125
(Saros 140)
 
April 1, 2136
(Saros 141)
 
March 2, 2147
(Saros 142)
 
January 30, 2158
(Saros 143)
 
December 29, 2168
(Saros 144)
 
November 28, 2179
(Saros 145)
 
October 29, 2190
(Saros 146)

Inex series

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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.

Series members between 1801 and 2200
 
October 20, 1827
(Saros 121)
 
September 29, 1856
(Saros 122)
 
September 8, 1885
(Saros 123)
 
August 21, 1914
(Saros 124)
 
August 1, 1943
(Saros 125)
 
July 10, 1972
(Saros 126)
 
June 21, 2001
(Saros 127)
 
June 1, 2030
(Saros 128)
 
May 11, 2059
(Saros 129)
 
April 21, 2088
(Saros 130)
 
April 2, 2117
(Saros 131)
 
March 12, 2146
(Saros 132)
 
February 21, 2175
(Saros 133)

Notes

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  1. ^ "July 10, 1972 Total Solar Eclipse". timeanddate. Retrieved 8 August 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 8 August 2024.
  3. ^ "ЗАТМЕНИЕ 30 ИЮНЯ 1972 г." (in Russian). IZMIRAN. Archived from the original on 22 June 2020.
  4. ^ "Voyage to Darkness". Pedas Family. Archived from the original on 4 April 2016.
  5. ^ Philip G. Schrag (30 July 1972). "For Two Extremely Short Minutes Everyone Gaped Into the Sky". New York Times. Archived from the original on 4 April 2016.
  6. ^ "You're So Vain by Carly Simon". Songfacts. Retrieved 2024-12-01. Glenn A. Walsh, who was Astronomical Observatory Coordinator and a Planetarium Lecturer for Pittsburgh's original Buhl Planetarium, told us: ... In fact, one day in mid-June of 1972, a colleague and I were in the radio station when the record was played. When that particular lyric was heard, he turned to me and said, 'that would be nice.' I knew he meant that it would be nice to fly to Nova Scotia and see the eclipse the next month.
  7. ^ "YOU'RE SO VAIN: THE TRUTH BEHIND CARLY SIMON'S MYSTERIOUS BREAKUP SONG". This Is Dig!. Warner Music Group. 2022-11-08. Retrieved 11 April 2024.
  8. ^ "Total Solar Eclipse of 1972 Jul 10". EclipseWise.com. Retrieved 8 August 2024.
  9. ^ 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.
  10. ^ "NASA - Catalog of Solar Eclipses of Saros 126". eclipse.gsfc.nasa.gov.

References

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