January 1981 lunar eclipse

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Template:Short description Script error: No such module "Unsubst". Template:Infobox lunar eclipse A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Tuesday, January 20, 1981,[1] with an umbral magnitude of −0.0192. It was a relatively rare total penumbral lunar eclipse, with the Moon passing entirely within the penumbral shadow without entering the darker umbral shadow.[2] A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into 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 about 5.2 days after perigee (on January 15, 1981, at 3:35 UTC), the Moon's apparent diameter was larger.[3]

Visibility

The eclipse was completely visible over northeast Asia, North America, and western South America, seen rising over east Asia and eastern Australia and setting over eastern South America, west Africa and much of Europe.[4]

File:Lunar eclipse from moon-1981Jan20.png File:Lunar eclipse chart close-1981Jan20.png

Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[5]

January 20, 1981 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 1.01360
Umbral Magnitude −0.01916
Gamma −1.01421
Sun Right Ascension 20h09m28.4s
Sun Declination -20°06'46.4"
Sun Semi-Diameter 16'15.2"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 08h08m59.5s
Moon Declination +19°08'35.7"
Moon Semi-Diameter 15'44.3"
Moon Equatorial Horizontal Parallax 0°57'45.5"
ΔT 51.4 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 January–February 1981
January 20
Ascending node (full moon)
February 4
Descending node (new moon)
File:Lunar eclipse chart close-1981Jan20.png File:SE1981Feb04A.png
Penumbral lunar eclipse
Lunar Saros 114
Annular solar eclipse
Solar Saros 140

Related eclipses

Eclipses in 1981

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 114

Inex

Triad

Lunar eclipses of 1980–1984

Template:Lunar eclipse set 1980-1984

Saros 114

Template:Lunar Saros series 114

Tritos series

Template:Lunar Tritos series November 2002

Inex series

Template:Lunar Inex series December 2009

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[6] This lunar eclipse is related to two annular solar eclipses of Solar Saros 121.

January 16, 1972 January 26, 1990
File:SE1972Jan16A.png File:SE1990Jan26A.png

See also

Notes

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  1. Script error: No such module "citation/CS1".
  2. Total Penumbral Lunar Eclipses, Jean Meeus, June 1980
  3. Script error: No such module "citation/CS1".
  4. Script error: No such module "citation/CS1".
  5. Script error: No such module "citation/CS1".
  6. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

Script error: No such module "Check for unknown parameters".

External links

Template:Lunar eclipses