Solar eclipse of April 18, 1977

An annular solar eclipse took place at the Moon's descending node of the orbit on Monday, April 18, 1977. 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 in South West Africa (today's Namibia), Angola, Zambia, southeastern Zaire (today's Democratic Republic of Congo), northern Malawi, Tanzania, Seychelles and the whole British Indian Ocean Territory.

Solar eclipse of April 18, 1977
Map
Type of eclipse
NatureAnnular
Gamma−0.399
Magnitude0.9449
Maximum eclipse
Duration424 s (7 min 4 s)
Coordinates11°54′S 28°18′E / 11.9°S 28.3°E / -11.9; 28.3
Max. width of band220 km (140 mi)
Times (UTC)
Greatest eclipse10:31:30
References
Saros138 (29 of 70)
Catalog # (SE5000)9458

Related eclipses edit

Eclipses in 1977 edit

Solar eclipses of 1975–1978 edit

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

Solar eclipse series sets from 1975 to 1978
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
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 138 edit

It is a part of Saros cycle 138, repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on June 6, 1472. It contains annular eclipses from August 31, 1598, through February 18, 2482 with a hybrid eclipse on March 1, 2500. It has total eclipses from March 12, 2518, through April 3, 2554. The series ends at member 70 as a partial eclipse on July 11, 2716. The longest duration of totality will be only 56 seconds on April 3, 2554.

Inex series edit

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Metonic series edit

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 descending node.

22 eclipse events between September 12, 1931 and July 1, 2011.
September 11-12 June 30-July 1 April 17-19 February 4-5 November 22-23
114 116 118 120 122
 
September 12, 1931
 
June 30, 1935
 
April 19, 1939
 
February 4, 1943
 
November 23, 1946
124 126 128 130 132
 
September 12, 1950
 
June 30, 1954
 
April 19, 1958
 
February 5, 1962
 
November 23, 1965
134 136 138 140 142
 
September 11, 1969
 
June 30, 1973
 
April 18, 1977
 
February 4, 1981
 
November 22, 1984
144 146 148 150 152
 
September 11, 1988
 
June 30, 1992
 
April 17, 1996
 
February 5, 2000
 
November 23, 2003
154 156
 
September 11, 2007
 
July 1, 2011


Notes edit

References edit