Solar eclipse of February 16, 1980

Solar eclipse of February 16, 1980
	Map
Type of eclipse
Nature	Total
Gamma	0.2224
Magnitude	1.0434
Maximum eclipse
Duration	248 sec (4 m 8 s)
Coordinates	0°06′S 47°06′E / 0.1°S 47.1°E
Max. width of band	149 km (93 mi)
Times (UTC)
Greatest eclipse	8:54:01
References
Saros	130 (50 of 73)
Catalog # (SE5000)	9464

A total solar eclipse occurred on February 16, 1980. 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. The path of totality crossed central Africa, southern India, and into China at sunset. The southern part of Mount Kilimanjaro, the highest mountain in Africa, also lies in the path of totality.

Related eclipses

Solar eclipses of 1979-1982

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 1979 to 1982
Descending node		Ascending node
Saros	Map	Saros	Map
120	February 26, 1979 Total	125	August 22, 1979 Annular
130	February 16, 1980 Total	135	August 10, 1980 Annular
140	February 4, 1981 Annular	145	July 31, 1981 Total
150	January 25, 1982 Partial	155	July 20, 1982 Partial
Partial solar eclipses on June 21, 1982 and December 15, 1982 occur in the next lunar year eclipse set.

Saros 130

It is a part of Saros cycle 130, repeating every 18 years, 11 days, containing 73 events. The series started with partial solar eclipse on August 20, 1096. It contains total eclipses from April 5, 1475 through July 18, 2232. The series ends at member 73 as a partial eclipse on October 25, 2394. The longest duration of totality was 6 minutes, 41 seconds on July 11, 1619.^[2]

Series members 43–56 between 1853 and 2100
43	44	45
November 30, 1853	December 12, 1871	December 22, 1889
46	47	48
January 3, 1908	January 14, 1926	January 25, 1944
49	50	51
February 5, 1962	February 16, 1980	February 26, 1998
52	53	54
March 9, 2016	March 20, 2034	March 30, 2052
55	56
April 11, 2070	April 21, 2088

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).

21 eclipse events, progressing from north to south between July 11, 1953 and July 11, 2029
July 10-11	April 29-30	February 15-16	December 4	September 21-23
116	118	120	122	124
July 11, 1953	April 30, 1957	February 15, 1961	December 4, 1964	September 22, 1968
126	128	130	132	134
July 10, 1972	April 29, 1976	February 16, 1980	December 4, 1983	September 23, 1987
136	138	140	142	144
July 11, 1991	April 29, 1995	February 16, 1999	December 4, 2002	September 22, 2006
146	148	150	152	154
July 11, 2010	April 29, 2014	February 15, 2018	December 4, 2021	September 21, 2025
156
July 11, 2029

Notes

↑ 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.
↑ "Saros Series catalog of solar eclipses". NASA.

References

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[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] "Saros Series catalog of solar eclipses". NASA.