Solar eclipse of May 9, 2032

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Solar eclipse of May 9, 2032
SE2032May09A.png
Map
Type of eclipse
NatureAnnular
Gamma-0.9375
Magnitude0.9957
Maximum eclipse
Duration22 sec (0 m 22 s)
Coordinates51°18′S 7°06′W / 51.3°S 7.1°W / -51.3; -7.1
Max. width of band44 km (27 mi)
Times (UTC)
Greatest eclipse13:26:42
References
Saros148 (22 of 75)
Catalog # (SE5000)9579

An annular solar eclipse will occur on May 9, 2032. 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.

Images[edit]

SE2032May09A.gif
Animated path

Related eclipses[edit]

Solar eclipses 2029-2032[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 January 14, 2029 and July 11, 2029 occur on the previous lunar year eclipse set.

Metonic cycle[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]