Solar eclipse of December 16, 2085

An annular solar eclipse will occur on December 16, 2085. 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. If a moon with same apparent diameter in this eclipse near the Aphelion, it will be Total Solar Eclipse, but in this time of the year, just 2 weeks and 4 days (18 days) before perihelion, it is an Annular Solar Eclipse.

Solar eclipse of December 16, 2085
Map
Type of eclipse
NatureAnnular
Gamma0.2786
Magnitude0.9971
Maximum eclipse
Duration19 sec (0 m 19 s)
Coordinates7.3°S 160.8°W / -7.3; -160.8
Max. width of band10 km (6.2 mi)
Times (UTC)
Greatest eclipse22:37:48
References
Saros143 (27 of 72)
Catalog # (SE5000)9700

Solar eclipses 2083–2087

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 15, 2083

Partial		 123January 7, 2084

Partial
128July 3, 2084

Annular		 133December 27, 2084

Total
138June 22, 2085

Annular		 143December 16, 2085

Annular
148June 11, 2086

Total		 153December 6, 2086

Partial
158June 1, 2087

Partial

Saros 143

It is a part of Saros cycle 143, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on March 7, 1617 and total event from June 24, 1797 through October 24, 1995. It has hybrid eclipses from November 3, 2013 through December 6, 2067, and annular eclipses from December 16, 2085 through September 16, 2536. The series ends at member 72 as a partial eclipse on April 23, 2873. The longest duration of totality was 3 minutes, 50 seconds on August 19, 1887. All eclipses in this series occurs at the Moon’s ascending node.

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.
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gollark: It's just palaiaologos being wrong, as is typical.
gollark: Fortunately, Sofia may or may not be my alt.
gollark: This is very muonic.
gollark: Wrong.

References
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