Solar eclipse of December 24, 1927

Summary

A partial solar eclipse occurred on December 24, 1927. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

Solar eclipse of December 24, 1927
Map
Type of eclipse
NaturePartial
Gamma−1.2416
Magnitude0.549
Maximum eclipse
Coordinates66°06′S 47°42′W / 66.1°S 47.7°W / -66.1; -47.7
Times (UTC)
Greatest eclipse3:59:41
References
Saros150 (12 of 71)
Catalog # (SE5000)9345

Related eclipses edit

Solar eclipses 1924–1928 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 1924 to 1928
Ascending node   Descending node
115 July 31, 1924
 
Partial
120 January 24, 1925
 
Total
125 July 20, 1925
 
Annular
130 January 14, 1926
 
Total
135 July 9, 1926
 
Annular
140 January 3, 1927
 
Annular
145 June 29, 1927
 
Total
150 December 24, 1927
 
Partial
155 June 17, 1928
 
Partial

Saros 150 edit

It is a part of Saros cycle 150, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on August 24, 1729. It contains annular eclipses from April 22, 2126, through June 22, 2829. There are no total eclipses in this series. The series ends at member 71 as a partial eclipse on September 29, 2991. The longest duration of annularity will be 9 minutes, 58 seconds on December 19, 2522.

References 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.

External links edit

  • Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
    • Besselian elements