An annular solar eclipse will occur at the Moon's ascending node of orbit on Friday, February 27, 2082, with a magnitude of 0.9298. 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 2.7 days before apogee (on March 2, 2082, at 8:00 UTC), the Moon's apparent diameter will be smaller.

The path of annularity will be visible from parts of Peru, Brazil, southeastern Suriname, French Guiana, Portugal, Spain, France, Switzerland, Italy, southern Germany, Liechtenstein, Austria, Slovenia, northern Croatia, and western Hungary. A partial solar eclipse will also be visible for parts of South America, Central America, the Caribbean, Mexico, the southeastern United States, eastern Canada, West Africa, North Africa, Greenland, and Europe.

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.

+February 27, 2082 Solar Eclipse Times Event Time (UTC) First Penumbral External Contact 2082 February 27 at 11:45:40.8 UTC First Umbral External Contact 2082 February 27 at 12:52:36.1 UTC First Central Line 2082 February 27 at 12:55:43.3 UTC First Umbral Internal Contact 2082 February 27 at 12:58:51.2 UTC First Penumbral Internal Contact 2082 February 27 at 14:15:39.6 UTC Greatest Duration 2082 February 27 at 14:34:08.6 UTC Greatest Eclipse 2082 February 27 at 14:46:59.8 UTC Ecliptic Conjunction 2082 February 27 at 14:51:00.7 UTC Equatorial Conjunction 2082 February 27 at 15:07:59.3 UTC Last Penumbral Internal Contact 2082 February 27 at 15:17:48.9 UTC Last Umbral Internal Contact 2082 February 27 at 16:34:54.0 UTC Last Central Line 2082 February 27 at 16:38:03.7 UTC Last Umbral External Contact 2082 February 27 at 16:41:12.7 UTC Last Penumbral External Contact 2082 February 27 at 17:48:13.9 UTC

+February 27, 2082 Solar Eclipse Parameters Parameter Value Eclipse Magnitude 0.92978 Eclipse Obscuration 0.86449 Gamma 0.33612 Sun Right Ascension 22h44m00.6s Sun Declination -08°01'49.1" Sun Semi-Diameter 16'09.0" Sun Equatorial Horizontal Parallax 08.9" Moon Right Ascension 22h43m26.2s Moon Declination -07°45'43.0" Moon Semi-Diameter 14'48.3" Moon Equatorial Horizontal Parallax 0°54'19.9" ΔT 107.2 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 February 2082 February 13Descending node (full moon) February 27Ascending node (new moon) Partial lunar eclipseLunar Saros 115 Annular solar eclipseSolar Saros 141

Related eclipses Eclipses in 2082 A partial lunar eclipse on February 13. An annular solar eclipse on February 27. A penumbral lunar eclipse on August 8. A total solar eclipse on August 24.

Metonic Preceded by: Solar eclipse of May 11, 2078 Followed by: Solar eclipse of December 16, 2085

Tzolkinex Preceded by: Solar eclipse of January 16, 2075 Followed by: Solar eclipse of April 10, 2089

Half-Saros Preceded by: Lunar eclipse of February 22, 2073 Followed by: Lunar eclipse of March 5, 2091

Tritos Preceded by: Solar eclipse of March 31, 2071 Followed by: Solar eclipse of January 27, 2093

Solar Saros 141 Preceded by: Solar eclipse of February 17, 2064 Followed by: Solar eclipse of March 10, 2100

Inex Preceded by: Solar eclipse of March 20, 2053 Followed by: Solar eclipse of February 8, 2111

Triad Preceded by: Solar eclipse of April 29, 1995 Followed by: Solar eclipse of December 29, 2168

Solar eclipses of 2080–2083

Saros 141

Metonic series

Tritos series

Inex series

Notes

References