Solar eclipse of February 18, 2091

A partial solar eclipse will occur at the Moon's descending node of orbit on Sunday, February 18, 2091, with a magnitude of 0.6558. 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 Europe, North Africa, and Central Asia.

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	2091 February 18 at 07:53:39.7 UTC
Ecliptic Conjunction	2091 February 18 at 09:41:09.3 UTC
Greatest Eclipse	2091 February 18 at 09:54:39.8 UTC
Equatorial Conjunction	2091 February 18 at 10:31:28.4 UTC
Last Penumbral External Contact	2091 February 18 at 11:55:26.8 UTC

Parameter	Value
Eclipse Magnitude	0.65581
Eclipse Obscuration	0.55496
Gamma	1.17790
Sun Right Ascension	22h08m17.5s
Sun Declination	-11°28'13.5"
Sun Semi-Diameter	16'11.1"
Sun Equatorial Horizontal Parallax	08.9"
Moon Right Ascension	22h07m09.8s
Moon Declination	-10°25'58.4"
Moon Semi-Diameter	14'56.6"
Moon Equatorial Horizontal Parallax	0°54'50.7"
ΔT	115.1 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.