Solar eclipse of October 3, 1986

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Solar eclipse of October 3, 1986
SE1986Oct03H.png
Map
Type of eclipse
Nature Hybrid
Gamma 0.9931
Magnitude 1
Maximum eclipse
Duration 0m 0s
Coordinates 59.9N 37.1W
Max. width of band 1 km
Times (UTC)
Greatest eclipse 19:06:15
References
Saros 124 (53 of 73)
Catalog # (SE5000) 9479

A total solar eclipse occurred on October 3, 1986. It was a hybrid event (normally, an eclipse which is annular for most of its duration, but with totality either at the beginning, end or at sometime during the eclipse) that did not officially satisfy the definition of totality. Totality occurred for a very short time (calculated at 0.2 seconds) in an area in the Atlantic Ocean, just east of the southern tip of Greenland. The path, on the surface of the Earth, was a narrow, tapered, horse-shoe, and visible only from a thin strip between Iceland and Greenland. At maximum eclipse the solar elevation was about 6°.

This eclipse was the last central eclipse of saros 124 and the only hybrid eclipse of that saros.

Related eclipses[edit]

Solar eclipses of 1986-1989[edit]

Each member 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.

Solar eclipse series sets from 1986-1989
Ascending node   Descending node
Saros Map Saros Map
119 SE1986Apr09P.png
April 9, 1986
Partial
124 SE1986Oct03H.png
October 3, 1986
Hybrid
129 SE1987Mar29H.png
March 29, 1987
Hybrid
134 SE1987Sep23A.png
September 23, 1987
Annular
139 SE1988Mar18T.png
March 18, 1988
Total
144 SE1988Sep11A.png
September 11, 1988
Annular
149 SE1989Mar07P.png
March 7, 1989
Partial
154 SE1989Aug31P.png
August 31, 1989
Partial

Metonic cycle[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).

References[edit]

External links[edit]