Solar eclipse of May 19, 1928

A total solar eclipse occurred on May 19, 1928. 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 May 19, 1928
Map
Type of eclipse
NatureTotal
Gamma1.0048
Magnitude1.014
Maximum eclipse
Duration-
Coordinates63.3°S 22.5°E / -63.3; 22.5
Max. width of band- km
Times (UTC)
Greatest eclipse13:24:20
References
Saros117 (64 of 71)
Catalog # (SE5000)9347

While it was a total solar eclipse, it was a non-central total eclipse.

This was the last of 56 umbral solar eclipses of Solar Saros 117. The 1st was in 936 AD and the 56th was in 1928. The total duration is 992 years.

Solar eclipses 1928–1931

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]

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). All eclipses in this table occur at the Moon's ascending node.

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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