December 2009 lunar eclipse

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Template:Short description Template:Use dmy dates Template:Infobox lunar eclipse A partial lunar eclipse occurred at the Moon’s descending node of orbit on Thursday, December 31, 2009,[1] with an umbral magnitude of 0.0779. 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 20 hours before perigee (on January 1, 2010, at 15:30 UTC), the Moon's apparent diameter was larger.[2]

This eclipse was the last of four lunar eclipses in 2009, with the others occurring on February 9 (penumbral), July 7 (penumbral), and August 6 (penumbral).

This lunar eclipse was also notable, because it occurred during a blue moon (a second full moon in December) and was near perigee (making it a supermoon). The next eclipse on New Year's Eve and blue moon will occur on December 31, 2028.

Only a small portion of the Moon entered the Earth's umbral shadow, but there was a distinct darkening visible over the Moon's southern surface at greatest eclipse.

Visibility

The eclipse was completely visible over Europe, Asia, and much of Africa, seen rising over eastern North America and setting over Australia and the Pacific Ocean.[3]

File:Lunar eclipse from moon-2009Dec31.png File:Lunar eclipse chart close-2009Dec31.png
Hourly motion shown right to left
File:Lunar eclipse chart-2009Dec31.png
The Moon's hourly motion across the Earth's shadow in the constellation of Gemini.
File:Visibility Lunar Eclipse 2009-12-31.png
Visibility map

Images

File:2009-12-31 Lunar Eclipse Sketch.png
NASA chart of the eclipse

Gallery

File:-20091231sequence.jpg
Progression from Degania A, Israel

Eclipse details

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

December 31, 2009 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 1.05719
Umbral Magnitude 0.07793
Gamma 0.97660
Sun Right Ascension 18h44m37.2s
Sun Declination -23°02'33.1"
Sun Semi-Diameter 16'15.9"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 06h45m22.4s
Moon Declination +24°01'10.3"
Moon Semi-Diameter 16'36.6"
Moon Equatorial Horizontal Parallax 1°00'57.6"
ΔT 66.1 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 2009–January 2010
December 31
Descending node (full moon)
January 15
Ascending node (new moon)
File:Lunar eclipse chart close-2009Dec31.png File:SE2010Jan15A.png
Partial lunar eclipse
Lunar Saros 115
Annular solar eclipse
Solar Saros 141

Related eclipses

Eclipses in 2009

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 115

Inex

Triad

Lunar eclipses of 2009–2013

Template:Lunar eclipse set 2009-2013

Saros 115

Template:Lunar Saros series 115

Tritos series

Template:Lunar Tritos series December 2009

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).[5] This lunar eclipse is related to two partial solar eclipses of Solar Saros 122.

December 25, 2000 January 6, 2019
File:SE2000Dec25P.png File:SE2019Jan06P.png

See also

References

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  5. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

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External links

Template:Lunar eclipses

Template:Sister project