Solar eclipse of July 10, 1972

Last updated
Solar eclipse of July 10, 1972
SE1972Jul10T.png
Map
Type of eclipse
NatureTotal
Gamma 0.6872
Magnitude 1.0379
Maximum eclipse
Duration156 s (2 min 36 s)
Coordinates 63°30′N94°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
Saros 126 (45 of 72)
Catalog # (SE5000) 9448

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]

Contents

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

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"

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

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
EventTime (UTC)
First Penumbral External Contact1972 July 10 at 17:19:47.5 UTC
First Umbral External Contact1972 July 10 at 18:28:23.8 UTC
First Central Line1972 July 10 at 18:29:24.0 UTC
First Umbral Internal Contact1972 July 10 at 18:30:24.5 UTC
Equatorial Conjunction1972 July 10 at 19:29:05.3 UTC
Ecliptic Conjunction1972 July 10 at 19:39:28.3 UTC
Greatest Duration1972 July 10 at 19:43:47.8 UTC
Greatest Eclipse1972 July 10 at 19:46:38.1 UTC
Last Umbral Internal Contact1972 July 10 at 21:03:06.0 UTC
Last Central Line1972 July 10 at 21:04:04.1 UTC
Last Umbral External Contact1972 July 10 at 21:05:01.8 UTC
Last Penumbral External Contact1972 July 10 at 22:13:41.2 UTC
July 10, 1972 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude1.03790
Eclipse Obscuration1.07723
Gamma0.68719
Sun Right Ascension07h20m39.3s
Sun Declination+22°08'59.1"
Sun Semi-Diameter15'43.9"
Sun Equatorial Horizontal Parallax08.6"
Moon Right Ascension07h21m20.3s
Moon Declination+22°48'27.6"
Moon Semi-Diameter16'08.2"
Moon Equatorial Horizontal Parallax0°59'13.3"
ΔT42.8 s

Eclipse season

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)
SE1972Jul10T.png Lunar eclipse chart close-1972Jul26.png
Total solar eclipse
Solar Saros 126
Partial lunar eclipse
Lunar Saros 138

Eclipses in 1972

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 126

Inex

Triad

Solar eclipses of 1971–1974

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
SarosMapGammaSarosMapGamma
116 July 22, 1971
SE1971Jul22P.png
Partial
1.513121 January 16, 1972
SE1972Jan16A.png
Annular
−0.9365
126 July 10, 1972
SE1972Jul10T.png
Total
0.6872131 January 4, 1973
SE1973Jan04A.png
Annular
−0.2644
136 June 30, 1973
SE1973Jun30T.png
Total
−0.0785141 December 24, 1973
SE1973Dec24A.png
Annular
0.4171
146 June 20, 1974
SE1974Jun20T.png
Total
−0.8239151 December 13, 1974
SE1974Dec13P.png
Partial
1.0797

Saros 126

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:
363738
SE1810Apr04A.gif
April 4, 1810
Saros126 37van72 SE1828Apr14H.jpg
April 14, 1828
SE1846Apr25H.gif
April 25, 1846
394041
SE1864May06H.gif
May 6, 1864
SE1882May17T.png
May 17, 1882
SE1900May28T.png
May 28, 1900
424344
SE1918Jun08T.png
June 8, 1918
SE1936Jun19T.png
June 19, 1936
SE1954Jun30T.png
June 30, 1954
454647
SE1972Jul10T.png
July 10, 1972
SE1990Jul22T.png
July 22, 1990
SE2008Aug01T.png
August 1, 2008
484950
SE2026Aug12T.png
August 12, 2026
SE2044Aug23T.png
August 23, 2044
SE2062Sep03P.png
September 3, 2062
515253
SE2080Sep13P.png
September 13, 2080
SE2098Sep25P.png
September 25, 2098
Saros126 53van72 SE2116Oct06P.jpg
October 6, 2116
545556
Saros126 54van72 SE2134Oct17P.jpg
October 17, 2134
Saros126 55van72 SE2152Oct28P.jpg
October 28, 2152
Saros126 56van72 SE2170Nov08P.jpg
November 8, 2170
57
Saros126 57van72 SE2188Nov18P.jpg
November 18, 2188

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). All eclipses in this table occur at the Moon's descending node.

21 eclipse events between July 11, 1953 and July 11, 2029
July 10–11April 29–30February 15–16December 4September 21–23
116118120122124
SE1953Jul11P.png
July 11, 1953
SE1957Apr30A.png
April 30, 1957
SE1961Feb15T.png
February 15, 1961
SE1964Dec04P.png
December 4, 1964
SE1968Sep22T.png
September 22, 1968
126128130132134
SE1972Jul10T.png
July 10, 1972
SE1976Apr29A.png
April 29, 1976
SE1980Feb16T.png
February 16, 1980
SE1983Dec04A.png
December 4, 1983
SE1987Sep23A.png
September 23, 1987
136138140142144
SE1991Jul11T.png
July 11, 1991
SE1995Apr29A.png
April 29, 1995
SE1999Feb16A.png
February 16, 1999
SE2002Dec04T.png
December 4, 2002
SE2006Sep22A.png
September 22, 2006
146148150152154
SE2010Jul11T.png
July 11, 2010
SE2014Apr29A.png
April 29, 2014
SE2018Feb15P.png
February 15, 2018
SE2021Dec04T.png
December 4, 2021
SE2025Sep21P.png
September 21, 2025
156
SE2029Jul11P.png
July 11, 2029

Tritos series

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
SE1808Oct19P.gif
October 19, 1808
(Saros 111)
SE1819Sep19Pe.gif
September 19, 1819
(Saros 112)
SE1830Aug18P.gif
August 18, 1830
(Saros 113)
SE1841Jul18P.gif
July 18, 1841
(Saros 114)
SE1852Jun17P.gif
June 17, 1852
(Saros 115)
SE1863May17P.gif
May 17, 1863
(Saros 116)
SE1874Apr16T.png
April 16, 1874
(Saros 117)
SE1885Mar16A.gif
March 16, 1885
(Saros 118)
SE1896Feb13A.png
February 13, 1896
(Saros 119)
SE1907Jan14T.png
January 14, 1907
(Saros 120)
SE1917Dec14A.png
December 14, 1917
(Saros 121)
SE1928Nov12P.png
November 12, 1928
(Saros 122)
SE1939Oct12T.png
October 12, 1939
(Saros 123)
SE1950Sep12T.png
September 12, 1950
(Saros 124)
SE1961Aug11A.png
August 11, 1961
(Saros 125)
SE1972Jul10T.png
July 10, 1972
(Saros 126)
SE1983Jun11T.png
June 11, 1983
(Saros 127)
SE1994May10A.png
May 10, 1994
(Saros 128)
SE2005Apr08H.png
April 8, 2005
(Saros 129)
SE2016Mar09T.png
March 9, 2016
(Saros 130)
SE2027Feb06A.png
February 6, 2027
(Saros 131)
SE2038Jan05A.png
January 5, 2038
(Saros 132)
SE2048Dec05T.png
December 5, 2048
(Saros 133)
SE2059Nov05A.png
November 5, 2059
(Saros 134)
SE2070Oct04A.png
October 4, 2070
(Saros 135)
SE2081Sep03T.png
September 3, 2081
(Saros 136)
SE2092Aug03A.png
August 3, 2092
(Saros 137)
SE2103Jul04A.png
July 4, 2103
(Saros 138)
SE2114Jun03T.png
June 3, 2114
(Saros 139)
SE2125May03A.png
May 3, 2125
(Saros 140)
SE2136Apr01A.png
April 1, 2136
(Saros 141)
SE2147Mar02T.png
March 2, 2147
(Saros 142)
SE2158Jan30A.png
January 30, 2158
(Saros 143)
SE2168Dec29A.png
December 29, 2168
(Saros 144)
SE2179Nov28T.png
November 28, 2179
(Saros 145)
SE2190Oct29H.png
October 29, 2190
(Saros 146)

Inex series

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
SE1827Oct20H.gif
October 20, 1827
(Saros 121)
SE1856Sep29A.gif
September 29, 1856
(Saros 122)
SE1885Sep08T.png
September 8, 1885
(Saros 123)
SE1914Aug21T.png
August 21, 1914
(Saros 124)
SE1943Aug01A.png
August 1, 1943
(Saros 125)
SE1972Jul10T.png
July 10, 1972
(Saros 126)
SE2001Jun21T.png
June 21, 2001
(Saros 127)
SE2030Jun01A.png
June 1, 2030
(Saros 128)
SE2059May11T.png
May 11, 2059
(Saros 129)
SE2088Apr21T.png
April 21, 2088
(Saros 130)
SE2117Apr02A.png
April 2, 2117
(Saros 131)
SE2146Mar12A.png
March 12, 2146
(Saros 132)
SE2175Feb21T.png
February 21, 2175
(Saros 133)

Notes

  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.

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A total solar eclipse occurred at the Moon's descending node of orbit on Wednesday, November 30, 1853, with a magnitude of 1.0485. 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 8.5 hours before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of June 26, 1824</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit between Saturday, June 26 and Sunday, June 27, 1824, with a magnitude of 1.0578. 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 1.9 days before perigee, the Moon's apparent diameter was larger.

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