Solar eclipse of December 13, 1974

A partial solar eclipse occurred on December 13, 1974. 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 13, 1974
Map
Type of eclipse
NaturePartial
Gamma1.0797
Magnitude0.8266
Maximum eclipse
Coordinates66°48′N 69°24′W / 66.8°N 69.4°W / 66.8; -69.4
Times (UTC)
Greatest eclipse16:13:13
References
Saros151 (12 of 72)
Catalog # (SE5000)9453

Related eclipses edit

Eclipses in 1974 edit

Solar eclipses of 1971–1974 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]

Note: Partial solar eclipses on February 25, 1971 and August 20, 1971 occur in the next lunar year set.

Solar eclipse series sets from 1971 to 1974
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
116  
1971 July 22
Partial
1.51298 121  
1972 January 16
Annular
−0.93651
126  
1972 July 10
Total
0.68719 131  
1973 January 4
Annular
−0.26441
136  
1973 June 30
Total
−0.07853 141  
1973 December 24
Annular
0.41710
146  
1974 June 20
Total
−0.82388 151  
1974 December 13
Partial
1.07974

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).

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