Solar eclipse of January 16, 1972

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Template:Short description Script error: No such module "Solar eclipse". An annular solar eclipse occurred at the Moon's ascending node of orbit on Sunday, January 16, 1972,[1] with a magnitude of 0.9692. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 7.3 days after apogee (on January 9, 1972, at 3:30 UTC), the Moon's apparent diameter was smaller.[2]

Annularity was visible from a part of Antarctica. A partial eclipse was visible for parts of Antarctica and extreme southern South America.

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.[3]

January 16, 1972 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 1972 January 16 at 08:45:57.2 UTC
First Umbral External Contact 1972 January 16 at 10:22:15.3 UTC
First Central Line 1972 January 16 at 10:25:28.8 UTC
Greatest Duration 1972 January 16 at 10:25:28.8 UTC
First Umbral Internal Contact 1972 January 16 at 10:28:57.8 UTC
Equatorial Conjunction 1972 January 16 at 10:33:15.2 UTC
Ecliptic Conjunction 1972 January 16 at 10:53:05.1 UTC
Greatest Eclipse 1972 January 16 at 11:03:22.3 UTC
Last Umbral Internal Contact 1972 January 16 at 11:38:09.6 UTC
Last Central Line 1972 January 16 at 11:41:35.3 UTC
Last Umbral External Contact 1972 January 16 at 11:44:45.6 UTC
Last Penumbral External Contact 1972 January 16 at 13:20:54.1 UTC
January 16, 1972 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.96925
Eclipse Obscuration 0.93945
Gamma −0.93651
Sun Right Ascension 19h49m32.3s
Sun Declination -21°03'34.9"
Sun Semi-Diameter 16'15.5"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 19h50m37.0s
Moon Declination -21°55'10.9"
Moon Semi-Diameter 15'40.7"
Moon Equatorial Horizontal Parallax 0°57'32.6"
ΔT 42.3 s

Eclipse season

Script error: No such module "Labelled list hatnote". 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 January 1972
January 16
Ascending node (new moon)
January 30
Descending node (full moon)
File:SE1972Jan16A.png File:Lunar eclipse chart close-1972Jan30.png
Annular solar eclipse
Solar Saros 121
Total lunar eclipse
Lunar Saros 133

Related eclipses

Eclipses in 1972

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 121

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.[4]

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
File:SE1971Jul22P.png
Partial
1.513 121 January 16, 1972
File:SE1972Jan16A.png
Annular
−0.9365
126 July 10, 1972
File:SE1972Jul10T.png
Total
0.6872 131 January 4, 1973
File:SE1973Jan04A.png
Annular
−0.2644
136 June 30, 1973
File:SE1973Jun30T.png
Total
−0.0785 141 December 24, 1973
File:SE1973Dec24A.png
Annular
0.4171
146 June 20, 1974
File:SE1974Jun20T.png
Total
−0.8239 151 December 13, 1974
File:SE1974Dec13P.png
Partial
1.0797

Saros 121

Template:Solar Saros series 121

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.

20 eclipse events between June 10, 1964 and August 21, 2036
June 10–11 March 28–29 January 14–16 November 3 August 21–22
117 119 121 123 125
File:SE1964Jun10P.png
June 10, 1964
File:SE1968Mar28P.png
March 28, 1968
File:SE1972Jan16A.png
January 16, 1972
File:SE1975Nov03P.png
November 3, 1975
File:SE1979Aug22A.png
August 22, 1979
127 129 131 133 135
File:SE1983Jun11T.png
June 11, 1983
File:SE1987Mar29H.png
March 29, 1987
File:SE1991Jan15A.png
January 15, 1991
File:SE1994Nov03T.png
November 3, 1994
File:SE1998Aug22A.png
August 22, 1998
137 139 141 143 145
File:SE2002Jun10A.png
June 10, 2002
File:SE2006Mar29T.png
March 29, 2006
File:SE2010Jan15A.png
January 15, 2010
File:SE2013Nov03H.png
November 3, 2013
File:SE2017Aug21T.png
August 21, 2017
147 149 151 153 155
File:SE2021Jun10A.png
June 10, 2021
File:SE2025Mar29P.png
March 29, 2025
File:SE2029Jan14P.png
January 14, 2029
File:SE2032Nov03P.png
November 3, 2032
File:SE2036Aug21P.png
August 21, 2036

Tritos series

Template:Solar Tritos series 2004 October 14

Inex series

Template:Solar Inex series 2000 December 25

Notes

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References

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