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Solar eclipse of October 23, 1976

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Solar eclipse of October 23, 1976
Map
Type of eclipse
NatureTotal
Gamma−0.327
Magnitude1.0572
Maximum eclipse
Duration286 s (4 min 46 s)
Coordinates30°00′S 92°18′E / 30°S 92.3°E / -30; 92.3
Max. width of band199 km (124 mi)
Times (UTC)
Greatest eclipse5:13:45
References
Saros133 (43 of 72)
Catalog # (SE5000)9457

A total solar eclipse occurred at the Moon's ascending node of the orbit on Saturday, October 23, 1976. 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. This total solar eclipse began at sunrise in Tanzania near the border with Burundi, with the path of totality passing just north of the large Tanzanian city of Dar es Salaam. It then crossed the Indian Ocean, passing St. Pierre Island, Providence Atoll and Farquhar Atoll of Seychelles before making landfall in southeastern Australia. The largest city that saw totality was Melbourne. After leaving the Australian mainland, the path of totality left the Earth's surface just north of the north island of New Zealand.

Eclipses in 1976

Solar eclipses of 1975–1978

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]

Solar eclipse series sets from 1975 to 1978
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
118 May 11, 1975

Partial
1.0647 123 November 3, 1975

Partial
−1.0248
128 April 29, 1976

Annular
0.3378 133 October 23, 1976

Total
−0.327
138 April 18, 1977

Annular
−0.399 143 October 12, 1977

Total
0.3836
148 April 7, 1978

Partial
−1.1081 153 October 2, 1978

Partial
1.1616

Saros 133

This eclipse is a part of Saros series 133, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on July 13, 1219. It contains annular eclipses from November 20, 1435 through January 13, 1526; a hybrid eclipse on January 24, 1544; and total eclipses from February 3, 1562 through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. 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 25 at 1 minutes, 14 seconds on November 30, 1453, and the longest duration of totality was produced by member 61 at 6 minutes, 50 seconds on August 7, 1850. All eclipses in this series occur at the Moon’s ascending node of orbit.[2]

Series members 34–55 occur between 1801 and 2200:
34 35 36

July 17, 1814

July 27, 1832

August 7, 1850
37 38 39

August 18, 1868

August 29, 1886

September 9, 1904
40 41 42

September 21, 1922

October 1, 1940

October 12, 1958
43 44 45

October 23, 1976

November 3, 1994

November 13, 2012
46 47 48

November 25, 2030

December 5, 2048

December 17, 2066
49 50 51

December 27, 2084

January 8, 2103

January 19, 2121
52 53 54

January 30, 2139

February 9, 2157

February 21, 2175
55

March 3, 2193

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

References

  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. ^ "NASA - Catalog of Solar Eclipses of Saros 133". eclipse.gsfc.nasa.gov.