Solar eclipse of October 23, 1976

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.

Solar eclipse of October 23, 1976
Map
Type of eclipse
NatureTotal
Gamma−0.327
Magnitude1.0572
Maximum eclipse
Duration286 sec (4 m 46 s)
Coordinates30°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

Eclipses in 1976

Solar eclipses of 1975–1978

There were 8 solar eclipses (at 6 month intervals) between May 11, 1975 and October 2, 1978.

Solar eclipse series sets from 1975–1978
Descending node   Ascending node
SarosMapGamma SarosMapGamma
118
1975 May 11
Partial
1.06472 123
1975 November 3
Partial
−1.02475
128
1976 April 29
Annular
0.33783 133
1976 October 23
Total
−0.32699
138
1977 April 18
Annular
−0.39903 143
1977 October 12
Total
0.38363
148
1978 April 7
Partial
−1.10812 153
1978 October 2
Partial
1.16164

Saros 133

Solar Saros 133, repeating every 18 years, 11 days, contains 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, with a hybrid eclipse on January 24, 1544. It has total eclipses from February 3, 1562, through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. The longest duration of totality was 6 minutes, 49.97 seconds on August 7, 1850.[1] The total eclipses of this saros series are getting shorter and farther south with each iteration. All eclipses in this series occurs at the Moon’s ascending node.

Series members 30–56 occur between 1742 and 2211
30 31 32
June 3, 1742 June 13, 1760
June 24, 1778
33 34 35
July 4, 1796 July 17, 1814 July 27, 1832
36 37 38
August 7, 1850
August 18, 1868

August 29, 1886
39 40 41

September 9, 1904

September 21, 1922

October 1, 1940
42 43 44

October 12, 1958

October 23, 1976

November 3, 1994
45 46 47

November 13, 2012

November 25, 2030

December 5, 2048
48 49 50

December 17, 2066

December 27, 2084

January 8, 2103
51 52 53

January 19, 2121

January 30, 2139

February 9, 2157
54 55 56

February 21, 2175

March 3, 2193

March 15, 2211

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

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