December 1991 lunar eclipse

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Template:Short description Template:Infobox lunar eclipse A partial lunar eclipse occurred at the Moon’s descending node of orbit on Saturday, December 21, 1991,[1] with an umbral magnitude of 0.0876. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring only about 23 hours before perigee (on December 22, 1991, at 9:25 UTC), the Moon's apparent diameter was larger.[2]

This eclipse was the last of four lunar eclipses in 1991, with the others occurring on January 30 (penumbral), June 27 (penumbral), and July 26 (penumbral).

Visibility

The eclipse was completely visible over northeast Asia, much of North America, and much of the Pacific Ocean, seen rising over central, south, and east Asia, and Australia and setting over South America and northern Europe.[3]

File:Lunar eclipse from moon-1991Dec21.png File:Lunar eclipse chart close-1991Dec21.png

Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]

December 21, 1991 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 1.06511
Umbral Magnitude 0.08762
Gamma 0.97094
Sun Right Ascension 17h55m52.1s
Sun Declination -23°26'13.9"
Sun Semi-Diameter 16'15.5"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 05h56m15.5s
Moon Declination +24°25'15.3"
Moon Semi-Diameter 16'38.0"
Moon Equatorial Horizontal Parallax 1°01'02.6"
ΔT 58.3 s

Eclipse season

Script error: No such module "Labelled list hatnote". 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 December 1991–January 1992
December 21
Descending node (full moon)
January 4
Ascending node (new moon)
File:Lunar eclipse chart close-1991Dec21.png File:SE1992Jan04A.png
Partial lunar eclipse
Lunar Saros 115
Annular solar eclipse
Solar Saros 141

Related eclipses

Eclipses in 1991

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 115

Inex

Triad

Lunar eclipses of 1991–1994

Template:Lunar eclipse set 1991-1994

Metonic series

The Metonic cycle repeats nearly exactly every 19 years and represents a Saros cycle plus one lunar year. Because it occurs on the same calendar date, the Earth's shadow will be in nearly the same location relative to the background stars.

Ascending node Descending node
  1. 1991 Jun 27 - penumbral (110)
  2. 2010 Jun 26 - partial (120)
  3. 2029 Jun 26 - total (130)
  4. 2048 Jun 26 - partial (140)
  5. 2067 Jun 27 - penumbral (150)
  1. 1991 Dec 21 - partial (115)
  2. 2010 Dec 21 - total (125)
  3. 2029 Dec 20 - total (135)
  4. 2048 Dec 20 - partial (145)
File:Metonic lunar eclipse 1991-2067A.png File:Metonic lunar eclipse 1991-2048D.png

Saros 115

Template:Lunar Saros series 115

Tritos series

Template:Lunar Tritos series November 2002

Inex series

Template:Lunar Inex series November 2020

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[5] This lunar eclipse is related to two partial solar eclipses of Solar Saros 122.

December 15, 1982 December 25, 2000
File:SE1982Dec15P.png File:SE2000Dec25P.png

See also

References

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  4. Script error: No such module "citation/CS1".
  5. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

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External links

Template:Lunar eclipses