January 2000 lunar eclipse

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Template:Short description Template:Use dmy dates Template:Infobox lunar eclipse A total lunar eclipse occurred at the Moon’s ascending node of orbit on Friday, January 21, 2000,[1] with an umbral magnitude of 1.3246. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. 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. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring about 1.5 days after perigee (on January 19, 2000, at 17:50 UTC), the Moon's apparent diameter was larger.[2]

Visibility

The eclipse was completely visible over most of North America, South America, and western Europe, seen rising over the Pacific Ocean and setting over Africa, Europe, and west Asia.[3]

File:Lunar eclipse from moon-2000Jan21.png File:Lunar eclipse chart close-2000Jan21.png
Hourly motion shown right to left

Eclipse details

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

January 21, 2000 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 2.30601
Umbral Magnitude 1.32459
Gamma −0.29571
Sun Right Ascension 20h10m32.9s
Sun Declination -20°03'20.2"
Sun Semi-Diameter 16'15.2"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 08h10m24.0s
Moon Declination +19°45'29.3"
Moon Semi-Diameter 16'33.7"
Moon Equatorial Horizontal Parallax 1°00'46.8"
ΔT 63.8 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 2000
January 21
Ascending node (full moon)
February 5
Descending node (new moon)
File:Lunar eclipse chart close-2000Jan21.png File:SE2000Feb05P.png
Total lunar eclipse
Lunar Saros 124
Partial solar eclipse
Solar Saros 150

Related eclipses

Eclipses in 2000

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 124

Inex

Triad

Lunar eclipses of 1998–2002

Template:Lunar eclipse set 1998-2002

Saros 124

Template:Lunar Saros series 124

Tritos series

Template:Lunar Tritos series January 2000

Inex series

Template:Lunar Inex series January 2000

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 annular solar eclipses of Solar Saros 131.

January 15, 1991 January 26, 2009
File:SE1991Jan15A.png File:SE2009Jan26A.png

See also

References

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

External links

Template:Lunar eclipses

Template:Sister project