Solar eclipse of October 23, 1957

Solar eclipse of October 23, 1957
Map
Type of eclipse
Nature Total
Gamma 1.0022
Magnitude 1.0013
Maximum eclipse
Duration -
Coordinates 71°12′S 23°06′W / 71.2°S 23.1°W / -71.2; -23.1
Max. width of band - km
Times (UTC)
Greatest eclipse 4:54:02
References
Saros 123 (50 of 70)
Catalog # (SE5000) 9415

A total solar eclipse occurred on October 23, 1957. 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.

Solar eclipses of 1957-1960

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 1957–1960
Descending node   Ascending node
SarosMap SarosMap
118
April 30, 1957
Annular
123
October 23, 1957
Total
128
April 19, 1958
Annular
133
October 12, 1958
Total
138
April 8, 1959
Annular
143
October 2, 1959
Total
148
March 27, 1960
Partial
153
September 20, 1960
Partial

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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