January 1999 lunar eclipse

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Template:Short description Template:Infobox lunar eclipse A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Sunday, January 31, 1999,[1] with an umbral magnitude of −0.0258. 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 4.8 days after perigee (on January 26, 1999, at 21:25 UTC), the Moon's apparent diameter was larger.[3]

Visibility

The eclipse was completely visible over Asia and Australia, seen rising over much of Africa, Europe, and the Middle East and setting over western North America and the central Pacific Ocean.[4]

File:Lunar eclipse from moon-1999Jan31.png File:Lunar eclipse chart close-1999Jan31.png

Gallery

File:Penumbral lunar eclipse 1999 jan 31.png
This simulated view compares this penumbral eclipse (left) to the full moon (right) as it appeared an hour before the eclipse.

Eclipse details

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

January 31, 1999 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 1.00272
Umbral Magnitude −0.02583
Gamma −1.01898
Sun Right Ascension 20h55m10.7s
Sun Declination -17°22'34.0"
Sun Semi-Diameter 16'14.0"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 08h54m26.3s
Moon Declination +16°24'30.3"
Moon Semi-Diameter 15'47.0"
Moon Equatorial Horizontal Parallax 0°57'55.6"
ΔT 63.5 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 1999
January 31
Ascending node (full moon)
February 16
Descending node (new moon)
File:Lunar eclipse chart close-1999Jan31.png File:SE1999Feb16A.png
Penumbral lunar eclipse
Lunar Saros 114
Annular solar eclipse
Solar Saros 140

Related eclipses

Eclipses in 1999

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 114

Inex

Triad

Lunar eclipses of 1998–2002

Template:Lunar eclipse set 1998-2002

Saros 114

Template:Lunar Saros series 114

Tritos series

Template:Lunar Tritos series December 2009

Inex series

Template:Lunar Inex series January 2028

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 26, 1990 February 7, 2008
File:SE1990Jan26A.png File:SE2008Feb07A.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

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External links

Template:Lunar eclipses Script error: No such module "Side box".