Solar eclipse of May 20, 1966

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Solar eclipse of May 20, 1966
SE1966May20A.png
Map
Type of eclipse
Nature Annular
Gamma 0.3467
Magnitude 0.9991
Maximum eclipse
Duration 5 sec (0 m 5 s)
Coordinates 39°12′N 26°24′E / 39.2°N 26.4°E / 39.2; 26.4
Max. width of band 3 km (1.9 mi)
Times (UTC)
Greatest eclipse 9:39:02
References
Saros 137 (33 of 70)
Catalog # (SE5000) 9434

An annular solar eclipse occurred on May 20, 1966. 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.

Related eclipses[edit]

Solar eclipses of 1964-1967[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.

Note: Partial solar eclipses on January 14, 1964 and July 9, 1964 belong to the previous lunar year set.

Solar eclipse series sets from 1964-1967
Ascending node   Descending node
Saros Map Saros Map
117 SE1964Jun10P.png
June 10, 1964
Partial
122 SE1964Dec04P.png
December 4, 1964
Partial
127 SE1965May30T.png
May 30, 1965
Total
132 SE1965Nov23A.png
November 23, 1965
Annular
137 SE1966May20A.png
May 20, 1966
Annular
142 SE1966Nov12T.png
November 12, 1966
Total
147 SE1967May09P.png
May 9, 1967
Partial
152 SE1967Nov02T.png
November 2, 1967
Total

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).

Notes[edit]

References[edit]