Solar eclipse of November 24, 2068

A partial solar eclipse will occur at the Moon's ascending node of orbit on Saturday, November 24, 2068, with a magnitude of 0.9109. 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.
The partial solar eclipse will be visible for parts of the Russian Far East and much of North America.

Eclipse details

Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the Moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.

Event	Time
First Penumbral External Contact	2068 November 24 at 19:16:52.1 UTC
Equatorial Conjunction	2068 November 24 at 21:21:22.0 UTC
Greatest Eclipse	2068 November 24 at 21:32:29.6 UTC
Ecliptic Conjunction	2068 November 24 at 21:44:08.8 UTC
Last Penumbral External Contact	2068 November 24 at 23:48:07.0 UTC

Parameter	Value
Eclipse Magnitude	0.91091
Eclipse Obscuration	0.85473
Gamma	1.02988
Sun Right Ascension	16h05m39.1s
Sun Declination	-20°49'55.6"
Sun Semi-Diameter	16'12.0"
Sun Equatorial Horizontal Parallax	08.9"
Moon Right Ascension	16h06m01.8s
Moon Declination	-19°53'06.5"
Moon Semi-Diameter	15'08.3"
Moon Equatorial Horizontal Parallax	0°55'33.5"
ΔT	96.7 s

Eclipse season

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.