Solar eclipse of July 20, 1982

Last updated
Solar eclipse of July 20, 1982
SE1982Jul20P.png
Map
Type of eclipse
NaturePartial
Gamma 1.2886
Magnitude 0.4643
Maximum eclipse
Coordinates 68°36′N64°12′E / 68.6°N 64.2°E / 68.6; 64.2
Times (UTC)
Greatest eclipse18:44:44
References
Saros 155 (4 of 71)
Catalog # (SE5000) 9469

A partial solar eclipse occurred at the Moon's ascending node of orbit on Tuesday, July 20, 1982, [1] with a magnitude of 0.4643. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

Contents

This was the third of four partial solar eclipses in 1982, with the others occurring on January 25, June 21, and December 15.

A partial eclipse was visible for parts of the northern Soviet Union, northern Alaska, northern Canada, Greenland, and Northern Europe.

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. [2]

July 20, 1982 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact1982 July 20 at 17:19:36.7 UTC
Equatorial Conjunction1982 July 20 at 18:30:56.4 UTC
Greatest Eclipse1982 July 20 at 18:44:43.8 UTC
Ecliptic Conjunction1982 July 20 at 18:57:30.7 UTC
Last Penumbral External Contact1982 July 20 at 20:09:59.1 UTC
July 20, 1982 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.46434
Eclipse Obscuration0.35755
Gamma1.28859
Sun Right Ascension07h59m09.9s
Sun Declination+20°37'14.1"
Sun Semi-Diameter15'44.4"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension07h59m44.7s
Moon Declination+21°55'14.5"
Moon Semi-Diameter16'37.4"
Moon Equatorial Horizontal Parallax1°01'00.4"
ΔT52.6 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. The first and last eclipse in this sequence is separated by one synodic month.

Eclipse season of June–July 1982
June 21
Ascending node (new moon)
July 6
Descending node (full moon)
July 20
Ascending node (new moon)
SE1982Jun21P.png Lunar eclipse chart close-1982Jul06.png SE1982Jul20P.png
Partial solar eclipse
Solar Saros 117
Total lunar eclipse
Lunar Saros 129
Partial solar eclipse
Solar Saros 155

Eclipses in 1982

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 155

Inex

Triad

Solar eclipses of 1979–1982

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. [3]

The partial solar eclipses on June 21, 1982 and December 15, 1982 occur in the next lunar year eclipse set.

Solar eclipse series sets from 1979 to 1982
Descending node Ascending node
SarosMapGammaSarosMapGamma
120
1979 Solar eclipse, Brandon Manitoba Canada (35907221663).jpg
Totality in Brandon, MB,
Canada
February 26, 1979
SE1979Feb26T.png
Total
0.8981125 August 22, 1979
SE1979Aug22A.png
Annular
−0.9632
130 February 16, 1980
SE1980Feb16T.png
Total
0.2224135 August 10, 1980
SE1980Aug10A.png
Annular
−0.1915
140 February 4, 1981
SE1981Feb04A.png
Annular
−0.4838145 July 31, 1981
SE1981Jul31T.png
Total
0.5792
150 January 25, 1982
SE1982Jan25P.png
Partial
−1.2311155 July 20, 1982
SE1982Jul20P.png
Partial
1.2886

Saros 155

This eclipse is a part of Saros series 155, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on June 17, 1928. It contains total eclipses from September 12, 2072 through August 30, 2649; hybrid eclipses from September 10, 2667 through October 2, 2703; and annular eclipses from October 13, 2721 through May 8, 3064. The series ends at member 71 as a partial eclipse on July 24, 3190. 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 totality will be produced by member 14 at 4 minutes, 5 seconds on November 6, 2162, and the longest duration of annularity will be produced by member 63 at 5 minutes, 31 seconds on April 28, 3046. All eclipses in this series occur at the Moon’s ascending node of orbit. [4]

Series members 1–16 occur between 1928 and 2200:
123
SE1928Jun17P.png
June 17, 1928
SE1946Jun29P.png
June 29, 1946
SE1964Jul09P.png
July 9, 1964
456
SE1982Jul20P.png
July 20, 1982
SE2000Jul31P.png
July 31, 2000
SE2018Aug11P.png
August 11, 2018
789
SE2036Aug21P.png
August 21, 2036
SE2054Sep02P.png
September 2, 2054
SE2072Sep12T.png
September 12, 2072
101112
SE2090Sep23T.png
September 23, 2090
Saros155 11van71 SE2108Oct05T.jpg
October 5, 2108
Saros155 12van71 SE2126Oct16T.jpg
October 16, 2126
131415
Saros155 13van71 SE2144Oct26T.jpg
October 26, 2144
Saros155 14van71 SE2162Nov07T.jpg
November 7, 2162
Saros155 15van71 SE2180Nov17T.jpg
November 17, 2180
16
Saros155 16van71 SE2198Nov28T.jpg
November 28, 2198

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 ascending node.

22 eclipse events between December 13, 1898 and July 20, 1982
December 13–14October 1–2July 20–21May 9February 24–25
111113115117119
SE1898Dec13P.gif
December 13, 1898
SE1906Jul21P.png
July 21, 1906
SE1910May09T.png
May 9, 1910
SE1914Feb25A.png
February 25, 1914
121123125127129
SE1917Dec14A.png
December 14, 1917
SE1921Oct01T.png
October 1, 1921
SE1925Jul20A.png
July 20, 1925
SE1929May09T.png
May 9, 1929
SE1933Feb24A.png
February 24, 1933
131133135137139
SE1936Dec13A.png
December 13, 1936
SE1940Oct01T.png
October 1, 1940
SE1944Jul20A.png
July 20, 1944
SE1948May09A.png
May 9, 1948
SE1952Feb25T.png
February 25, 1952
141143145147149
SE1955Dec14A.png
December 14, 1955
SE1959Oct02T.png
October 2, 1959
SE1963Jul20T.png
July 20, 1963
SE1967May09P.png
May 9, 1967
SE1971Feb25P.png
February 25, 1971
151153155
SE1974Dec13P.png
December 13, 1974
SE1978Oct02P.png
October 2, 1978
SE1982Jul20P.png
July 20, 1982

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 1982
SE1807Nov29H.gif
November 29, 1807
(Saros 139)
SE1818Oct29T.gif
October 29, 1818
(Saros 140)
SE1829Sep28A.gif
September 28, 1829
(Saros 141)
SE1840Aug27T.gif
August 27, 1840
(Saros 142)
SE1851Jul28T.png
July 28, 1851
(Saros 143)
SE1862Jun27P.gif
June 27, 1862
(Saros 144)
SE1873May26P.gif
May 26, 1873
(Saros 145)
SE1884Apr25P.gif
April 25, 1884
(Saros 146)
SE1895Mar26P.gif
March 26, 1895
(Saros 147)
SE1906Feb23P.png
February 23, 1906
(Saros 148)
SE1917Jan23P.png
January 23, 1917
(Saros 149)
SE1927Dec24P.png
December 24, 1927
(Saros 150)
SE1938Nov21P.png
November 21, 1938
(Saros 151)
SE1949Oct21P.png
October 21, 1949
(Saros 152)
SE1960Sep20P.png
September 20, 1960
(Saros 153)
SE1971Aug20P.png
August 20, 1971
(Saros 154)
SE1982Jul20P.png
July 20, 1982
(Saros 155)

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 2069
SE1808Nov18P.gif
November 18, 1808
(Saros 149)
SE1837Oct29P.gif
October 29, 1837
(Saros 150)
SE1866Oct08P.gif
October 8, 1866
(Saros 151)
SE1895Sep18P.gif
September 18, 1895
(Saros 152)
SE1924Aug30P.png
August 30, 1924
(Saros 153)
SE1953Aug09P.png
August 9, 1953
(Saros 154)
SE1982Jul20P.png
July 20, 1982
(Saros 155)
SE2011Jul01P.png
July 1, 2011
(Saros 156)
SE2069May20P.png
May 20, 2069
(Saros 158)

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References

  1. "July 20, 1982 Partial Solar Eclipse". timeanddate. Retrieved 9 August 2024.
  2. "Partial Solar Eclipse of 1982 Jul 20". EclipseWise.com. Retrieved 9 August 2024.
  3. 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.
  4. "NASA - Catalog of Solar Eclipses of Saros 155". eclipse.gsfc.nasa.gov.