Solar eclipse of November 27, 2095


An annular solar eclipse will occur at the Moon's descending node of orbit between Saturday, November 26 and Sunday, November 27, 2095, with a magnitude of 0.933. 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. An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 3.8 days after apogee, the Moon's apparent diameter will be smaller.
The path of annularity will be visible from parts of northeastern China, North Korea, South Korea, Japan, the Marshall Islands, and Kiribati. A partial solar eclipse will also be visible for parts of East Asia, Southeast Asia, Oceania, Hawaii, and southwestern Alaska.

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.
EventTime
First Penumbral External Contact2095 November 26 at 22:08:18.5 UTC
First Umbral External Contact2095 November 26 at 23:17:51.3 UTC
First Central Line2095 November 26 at 23:21:03.1 UTC
First Umbral Internal Contact2095 November 26 at 23:24:16.3 UTC
Equatorial Conjunction2095 November 27 at 00:46:21.1 UTC
Ecliptic Conjunction2095 November 27 at 00:57:09.8 UTC
Greatest Eclipse2095 November 27 at 01:02:57.4 UTC
Greatest Duration2095 November 27 at 01:13:24.5 UTC
Last Umbral Internal Contact2095 November 27 at 02:41:51.2 UTC
Last Central Line2095 November 27 at 02:45:02.1 UTC
Last Umbral External Contact2095 November 27 at 02:48:11.5 UTC
Last Penumbral External Contact2095 November 27 at 03:57:38.7 UTC

ParameterValue
Eclipse Magnitude0.93303
Eclipse Obscuration0.87054
Gamma0.49030
Sun Right Ascension16h12m24.6s
Sun Declination-21°07'41.4"
Sun Semi-Diameter16'12.2"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension16h12m56.4s
Moon Declination-20°41'58.0"
Moon Semi-Diameter14'55.2"
Moon Equatorial Horizontal Parallax0°54'45.3"
ΔT119.6 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.
November 27
Descending node
December 11
Ascending node
Annular solar eclipse
Solar Saros 134		Partial lunar eclipse
Lunar Saros 146

Related eclipses

Eclipses in 2095

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 134

Inex

Triad