Solar eclipse of November 24, 2068

A partial solar eclipse will occur on November 24, 2068. 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 November 24, 2068
Map
Type of eclipse
NaturePartial
Gamma1.0299
Magnitude0.9109
Maximum eclipse
Coordinates68.5°N 131.1°W / 68.5; -131.1
Times (UTC)
Greatest eclipse21:32:30
References
Saros153 (12 of 70)
Catalog # (SE5000)9661

Solar eclipses 2065–2069

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]

118July 3, 2065

Partial		 123December 27, 2065

Partial
128June 22, 2066

Annular		 133December 17, 2066

Total
138June 11, 2067

Annular		 143December 6, 2067

Hybrid
148May 31, 2068

Total		 153November 24, 2068

Partial
158May 20, 2069

Partial

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

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). All eclipses in this table occur at the Moon's ascending node.

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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.
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