Solar eclipse of January 4, 1973
Map
Type of eclipse
NatureAnnular
Gamma−0.2644
Magnitude0.9303
Maximum eclipse
Duration469 sec (7 m 49 s)
Coordinates37°54′S 51°12′W / 37.9°S 51.2°W / -37.9; -51.2
Max. width of band271 km (168 mi)
Times (UTC)
Greatest eclipse15:46:21
References
Saros131 (48 of 70)
Catalog # (SE5000)9449

An annular solar eclipse occurred on January 4, 1973, with an eclipse magnitude of 0.9303. 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. Annularity was visible from Chile and Argentina.

Eclipses in 1973

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.[1]

Note: Partial solar eclipses on February 25, 1971 and August 20, 1971 occur in the next lunar year set.

Solar eclipse series sets from 1971–1974
Descending node   Ascending node
SarosMapGamma SarosMapGamma
116
1971 July 22
Partial
1.51298 121
1972 January 16
Annular
−0.93651
126
1972 July 10
Total
0.68719 131
1973 January 4
Annular
−0.26441
136
1973 June 30
Total
−0.07853 141
1973 December 24
Annular
0.41710
146
1974 June 20
Total
−0.82388 151
1974 December 13
Partial
1.07974

Saros 131

It is a part of Saros cycle 131, repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on August 1, 1125. It contains total eclipses from March 27, 1522 through May 30, 1612 and hybrid eclipses from June 10, 1630 through July 24, 1702, and annular eclipses from August 4, 1720 through June 18, 2243. The series ends at member 70 as a partial eclipse on September 2, 2369. The longest duration of totality was only 58 seconds on May 30, 1612. All eclipses in this series occurs at the Moon’s ascending node.

Series members 33–70 occur between 1702 and 2369
33 34 35

July 24, 1702

August 4, 1720

August 15, 1738
36 37 38

August 25, 1756

September 6, 1774

September 16, 1792
39 40 41

September 28, 1810

October 9, 1828

October 20, 1846
42 43 44

October 30, 1864

November 10, 1882

November 22, 1900
45 46 47

December 3, 1918

December 13, 1936

December 25, 1954
48 49 50

January 4, 1973

January 15, 1991

January 26, 2009
51 52 53

February 6, 2027

February 16, 2045

February 28, 2063
54 55 56

March 10, 2081

March 21, 2099

April 2, 2117
57 58 59

April 13, 2135

April 23, 2153

May 5, 2171
60 61 62

May 15, 2189

May 27, 2207

June 6, 2225
63 64 65

June 18, 2243

June 28, 2261

July 9, 2279
66 67 68

July 20, 2297

August 1, 2315

August 11, 2333
69 70

August 22, 2351

September 2, 2369

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 January 5, 1935 and August 11, 2018
January 4-5 October 23-24 August 10-12 May 30-31 March 18-19
111 113 115 117 119

January 5, 1935

August 12, 1942

May 30, 1946

March 18, 1950
121 123 125 127 129

January 5, 1954

October 23, 1957

August 11, 1961

May 30, 1965

March 18, 1969
131 133 135 137 139

January 4, 1973

October 23, 1976

August 10, 1980

May 30, 1984

March 18, 1988
141 143 145 147 149

January 4, 1992

October 24, 1995

August 11, 1999

May 31, 2003

March 19, 2007
151 153 155

January 4, 2011

October 23, 2014

August 11, 2018

Notess

  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.

References


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