Solar eclipse of November 23, 1965

Solar eclipse of November 23, 1965
Map
Type of eclipse
Nature Annular
Gamma 0.3906
Magnitude 0.9656
Maximum eclipse
Duration 242 sec (4 m 2 s)
Coordinates 1°42′N 119°48′E / 1.7°N 119.8°E / 1.7; 119.8
Max. width of band 134 km (83 mi)
Times (UTC)
Greatest eclipse 4:14:51
References
Saros 132 (43 of 71)
Catalog # (SE5000) 9433

An annular solar eclipse occurred on November 23, 1965. 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

Solar eclipses of 1964-1967

Template:Lunar year eclipse Template:Saros map 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
SarosMap SarosMap
117
June 10, 1964
Partial
122
December 4, 1964
Partial
127
May 30, 1965
Total
132
November 23, 1965
Annular
137
May 20, 1966
Annular
142
November 12, 1966
Total
147
May 9, 1967
Partial
152
November 2, 1967
Total

Saros 132

It is a part of Saros cycle 132, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on August 13, 1208. It contains annular eclipses from March 17, 1569 through March 12, 2146, hybrid on March 23, 2164 and April 3, 2183 and total eclipses from April 14, 2200 through June 19, 2308. The series ends at member 71 as a partial eclipse on September 25, 2470. The longest duration of annular was 6 minutes, 56 seconds on May 9, 1641, and totality will be 2 minutes, 14 seconds on June 8, 2290.[1]

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).

Notes

References

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