Solar eclipse of October 4, 2051

Summary

A partial solar eclipse will occur on Wednesday, October 4, 2051. 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 October 4, 2051
Map
Type of eclipse
NaturePartial
Gamma−1.2094
Magnitude0.6024
Maximum eclipse
Coordinates72°00′S 117°42′E / 72°S 117.7°E / -72; 117.7
Times (UTC)
Greatest eclipse21:02:14
References
Saros125 (56 of 73)
Catalog # (SE5000)9622

Related eclipses edit

Solar eclipses 2051–2054 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 2051 to 2054
Descending node   Ascending node
Saros Map Saros Map
120 April 11, 2051
 
Partial
125 October 4, 2051
 
Partial
130 March 30, 2052
 
Total
135 September 22, 2052
 
Annular
140 March 20, 2053
 
Annular
145 September 12, 2053
 
Total
150 March 9, 2054
 
Partial
155 September 2, 2054
 
Partial

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

  • http://eclipse.gsfc.nasa.gov/SEplot/SEplot2051/SE2051Oct04P.GIF