Solar eclipse of November 22, 1984

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Solar eclipse of November 22, 1984
Solar eclipse of 22 November 1984.JPG
Partial from Gisborne, New Zealand
SE1984Nov22T.png
Map
Type of eclipse
NatureTotal
Gamma-0.3132
Magnitude1.0237
Maximum eclipse
Duration120 sec (2 m 0 s)
Coordinates37°48′S 173°36′W / 37.8°S 173.6°W / -37.8; -173.6
Max. width of band85 km (53 mi)
Times (UTC)
Greatest eclipse22:54:17
References
Saros142 (21 of 72)
Catalog # (SE5000)9475

A total solar eclipse occurred on November 22, 1984. 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. Totality was visible in Indonesia, Papua New Guinea and southern Pacific Ocean. West of the International Date Line the eclipse took place on November 23, including all land in the path of totality. Occurring only 2.1 days after perigee (Perigee on November 20, 1984), the Moon's apparent diameter was fairly larger.

Related eclipses[]

Eclipses of 1984[]

Solar eclipses of 1982–1985[]

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.[1]

Note: Partial solar eclipses on January 25, 1982 and July 20, 1982 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 1982–1985
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
117 SE1982Jun21P.png
1982 June 21
Partial
-1.21017 122 SE1982Dec15P.png
1982 December 15
Partial
1.12928
127 SE1983Jun11T.png
1983 June 11
Total
-0.49475 132 SE1983Dec04A.png
1983 December 4
Annular
0.40150
137 SE1984May30A.png
1984 May 30
Annular
0.27552 142
Solar eclipse of 22 November 1984.JPG
Partial from Gisborne, NZ
SE1984Nov22T.png
1984 November 22
Total
-0.31318
147 SE1985May19P.png
1985 May 19
Partial
1.07197 152 SE1985Nov12T.png
1985 November 12
Total
-0.97948

Saros 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.[2]

Series members 17–41 occur between 1901 and 2359
17 18 19
SE1912Oct10T.png
October 10, 1912
SE1930Oct21T.png
October 21, 1930
SE1948Nov01T.png
November 1, 1948
20 21 22
SE1966Nov12T.png
November 12, 1966
SE1984Nov22T.png
November 22, 1984
SE2002Dec04T.png
December 4, 2002
23 24 25
SE2020Dec14T.png
December 14, 2020
SE2038Dec26T.png
December 26, 2038
SE2057Jan05T.png
January 5, 2057
26 27 28
SE2075Jan16T.png
January 16, 2075
SE2093Jan27T.png
January 27, 2093
SE2111Feb08T.png
February 8, 2111
29 30 31
SE2129Feb18T.png
February 18, 2129
SE2147Mar02T.png
March 2, 2147
SE2165Mar12T.png
March 12, 2165
32 33 34
SE2183Mar23T.png
March 23, 2183
SE2201Apr04T.png
April 4, 2201
SE2219Apr15T.png
April 15, 2219
35 36 37
SE2237Apr25T.png
April 25, 2237
SE2255May07T.png
May 7, 2255
SE2273May17T.png
May 17, 2273
38 39 40
SE2291May28T.png
May 28, 2291
SE2309Jun09T.png
June 9, 2309
SE2327Jun20T.png
June 20, 2327
41
SE2345Jun30T.png
June 30, 2345

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.

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.

22 eclipse events between September 12, 1931 and July 1, 2011.
September 11-12 June 30-July 1 April 17-19 February 4-5 November 22-23
114 116 118 120 122
SE1931Sep12P.png
September 12, 1931
SE1935Jun30P.png
June 30, 1935
SE1939Apr19A.png
April 19, 1939
SE1943Feb04T.png
February 4, 1943
SE1946Nov23P.png
November 23, 1946
124 126 128 130 132
SE1950Sep12T.png
September 12, 1950
SE1954Jun30T.png
June 30, 1954
SE1958Apr19A.png
April 19, 1958
SE1962Feb05T.png
February 5, 1962
SE1965Nov23A.png
November 23, 1965
134 136 138 140 142
SE1969Sep11A.png
September 11, 1969
SE1973Jun30T.png
June 30, 1973
SE1977Apr18A.png
April 18, 1977
SE1981Feb04A.png
February 4, 1981
SE1984Nov22T.png
November 22, 1984
144 146 148 150 152
SE1988Sep11A.png
September 11, 1988
SE1992Jun30T.png
June 30, 1992
SE1996Apr17P.png
April 17, 1996
SE2000Feb05P.png
February 5, 2000
SE2003Nov23T.png
November 23, 2003
154 156 158 160 162
SE2007Sep11P.png
September 11, 2007
SE2011Jul01P.png
July 1, 2011
April 18, 2015 February 4, 2019 November 23, 2022

Notes[]

  1. ^ 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.
  2. ^ http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros142.html

References[]

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