Solar eclipse of October 1, 1921

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 eclipse of October 1, 1921
Map
Type of eclipse
NatureTotal
Gamma−0.9383
Magnitude1.0293
Maximum eclipse
Duration112 s (1 min 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

Related eclipses edit

Solar eclipses 1921–1924 edit

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 to 1924
Descending node   Ascending node
118 April 8, 1921
 
Annular
123 October 1, 1921
 
Total
128 March 28, 1922
 
Annular
133 September 21, 1922
 
Total
138 March 17, 1923
 
Annular
143 September 10, 1923
 
Total
148 March 5, 1924
 
Partial
153 August 30, 1924
 
Partial

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

  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 edit