Solar eclipse of January 26, 1990

Solar eclipse of January 26, 1990
Map
Type of eclipse
Nature Annular
Gamma -0.9457
Magnitude 0.967
Maximum eclipse
Duration 123 sec (2 m 3 s)
Coordinates 71°00′S 22°12′W / 71°S 22.2°W / -71; -22.2
Max. width of band 373 km (232 mi)
Times (UTC)
Greatest eclipse 19:31:24
References
Saros 121 (59 of 71)
Catalog # (SE5000) 9486

An annular solar eclipse occurred on January 26, 1990. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

Solar eclipses of 1990-1992

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).

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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