Solar eclipse of October 1, 1921
Map
Type of eclipse
NatureTotal
Gamma−0.9383
Magnitude1.0293
Maximum eclipse
Duration112 sec (1 m 52 s)
Coordinates66°06′S 56°06′W / 66.1°S 56.1°W / -66.1; -56.1
Max. width of band291 km (181 mi)
Times (UTC)
Greatest eclipse12:35:58
References
Saros123 (48 of 70)
Catalog # (SE5000)9331

A total solar eclipse occurred on October 1, 1921. 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 1921–1924

This eclipse is a member of a semester series. An eclipse 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.[1]

Solar eclipse series sets from 1921–1924
Descending node   Ascending node
118April 8, 1921

Annular
123October 1, 1921

Total
128March 28, 1922

Annular
133September 21, 1922

Total
138March 17, 1923

Annular
143September 10, 1923

Total
148March 5, 1924

Partial
153August 30, 1924

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

  1. van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.

References

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