February 2009 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 descending node of orbit on Monday, February 9, 2009,[1] with an umbral magnitude of −0.0863. 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 1.9 days after perigee (on February 7, 2009, at 15:10 UTC), the Moon's apparent diameter was larger.[2]

This eclipse was the first of four lunar eclipses in 2009, with the others occurring on July 7 (penumbral), August 6 (penumbral), and December 31 (partial).

It also happened on the Lantern Festival, the first since February 20, 1989.

Visibility

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

File:Lunar eclipse from moon-2009Feb09.png File:Lunar eclipse chart close-09feb09.png
Hourly motion shown right to left
File:Lunar eclipse chart-2009feb09.png
The Moon's hourly motion across the Earth's shadow in the constellation of Leo.
File:Visibility Lunar Eclipse 2009-02-09.png
Visibility map

Images

File:Lunar eclipse from moon-09feb09.png
This simulated view shows the Earth and Sun as viewed from the center of the Moon near contact points P1 and P4. The eclipse will be visible from Earth from the locations of the world as seen on the Earth above.

Gallery

Eclipse details

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

February 9, 2009 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.90132
Umbral Magnitude −0.08632
Gamma −1.06401
Sun Right Ascension 21h33m30.0s
Sun Declination -14°30'07.1"
Sun Semi-Diameter 16'12.6"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 09h31m42.1s
Moon Declination +13°31'37.5"
Moon Semi-Diameter 16'24.8"
Moon Equatorial Horizontal Parallax 1°00'14.2"
ΔT 65.8 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 2009
January 26
Ascending node (new moon)
February 9
Descending node (full moon)
File:SE2009Jan26A.png File:Lunar eclipse chart close-09feb09.png
Annular solar eclipse
Solar Saros 131
Penumbral lunar eclipse
Lunar Saros 143

Related eclipses

Eclipses in 2009

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 143

Inex

Triad

Lunar eclipses of 2006–2009

Template:Lunar eclipse set 2006-2009

Saros 143

Template:Lunar Saros series 143

Tritos series

Template:Lunar Tritos series February 2009

Inex series

Template:Lunar Inex series February 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 150.

February 5, 2000 February 15, 2018
File:SE2000Feb05P.png File:SE2018Feb15P.png

See also

Notes

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

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External links

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