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 (ring). 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 (on November 23, 2095, at 6:10 UTC), 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.
+November 27, 2095 Solar Eclipse Times Event Time (UTC) First Penumbral External Contact 2095 November 26 at 22:08:18.5 UTC First Umbral External Contact 2095 November 26 at 23:17:51.3 UTC First Central Line 2095 November 26 at 23:21:03.1 UTC First Umbral Internal Contact 2095 November 26 at 23:24:16.3 UTC Equatorial Conjunction 2095 November 27 at 00:46:21.1 UTC Ecliptic Conjunction 2095 November 27 at 00:57:09.8 UTC Greatest Eclipse 2095 November 27 at 01:02:57.4 UTC Greatest Duration 2095 November 27 at 01:13:24.5 UTC Last Umbral Internal Contact 2095 November 27 at 02:41:51.2 UTC Last Central Line 2095 November 27 at 02:45:02.1 UTC Last Umbral External Contact 2095 November 27 at 02:48:11.5 UTC Last Penumbral External Contact 2095 November 27 at 03:57:38.7 UTC
+November 27, 2095 Solar Eclipse Parameters Parameter Value Eclipse Magnitude 0.93303 Eclipse Obscuration 0.87054 Gamma 0.49030 Sun Right Ascension 16h12m24.6s Sun Declination -21°07'41.4" Sun Semi-Diameter 16'12.2" Sun Equatorial Horizontal Parallax 08.9" Moon Right Ascension 16h12m56.4s Moon Declination -20°41'58.0" Moon Semi-Diameter 14'55.2" Moon Equatorial Horizontal Parallax 0°54'45.3" ΔT 119.6 s
Eclipse season
This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) 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.
+ Eclipse season of November–December 2095 November 27Descending node (new moon) December 11Ascending node (full moon) Annular solar eclipseSolar Saros 134 Partial lunar eclipseLunar Saros 146
Related eclipses Eclipses in 2095 A total solar eclipse on June 2. A partial lunar eclipse on June 17. An annular solar eclipse on November 27. A partial lunar eclipse on December 11.
Metonic Preceded by: Solar eclipse of February 7, 2092 Followed by: Solar eclipse of September 14, 2099
Tzolkinex Preceded by: Solar eclipse of October 14, 2088 Followed by: Solar eclipse of January 8, 2103
Half-Saros Preceded by: Lunar eclipse of November 20, 2086 Followed by: Lunar eclipse of December 2, 2104
Tritos Preceded by: Solar eclipse of December 27, 2084 Followed by: Solar eclipse of October 26, 2106
Solar Saros 134 Preceded by: Solar eclipse of November 15, 2077 Followed by: Solar eclipse of December 8, 2113
Inex Preceded by: Solar eclipse of December 17, 2066 Followed by: Solar eclipse of November 6, 2124
Triad Preceded by: Solar eclipse of January 26, 2009 Followed by: Solar eclipse of September 27, 2182
Solar eclipses of 2094–2098
Saros 134
Metonic series
Tritos series
Inex series
Notes
References