Solar eclipse of February 25, 1971

Last updated
Solar eclipse of February 25, 1971
SE1971Feb25P.png
Map
Type of eclipse
NaturePartial
Gamma 1.1188
Magnitude 0.7872
Maximum eclipse
Coordinates 61°24′N33°30′W / 61.4°N 33.5°W / 61.4; -33.5
Times (UTC)
Greatest eclipse9:38:07
References
Saros 149 (18 of 71)
Catalog # (SE5000) 9444

A partial solar eclipse occurred on February 25, 1971 with a magnitude of 0.7872. 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. In this partial solar eclipse, the Moon covered 78.7% of the Sun.

Contents

Solar eclipses of 1968–1971

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 1968–1971
Ascending node Descending node
SarosMapGammaSarosMapGamma
119 SE1968Mar28P.png
1968 March 28
Partial
−1.03704124 SE1968Sep22T.png
1968 September 22
Total
0.94507
129 SE1969Mar18A.png
1969 March 18
Annular
−0.27037134 SE1969Sep11A.png
1969 September 11
Annular
0.22014
139 SE1970Mar07T.png
1970 March 7
Total
0.44728144 SE1970Aug31A.png
1970 August 31
Annular
−0.53640
149 SE1971Feb25P.png
1971 February 25
Partial
1.11876154 SE1971Aug20P.png
1971 August 20
Partial
−1.26591
A partial solar eclipse of July 22, 1971 occurs in the next lunar year set.

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).

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References

  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.