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February 2009 lunar eclipse

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February 2009 lunar eclipse
Penumbral eclipse
Just before maximum eclipse (14:29 UTC) from Chennai, India
Date9 February 2009
Gamma−1.06401
Magnitude0.89946
Saros cycle143 (18 of 73)
Penumbral238 minutes, 54 seconds
Contacts (UTC)
P112:38:46
Greatest14:38:15
P416:37:40

A penumbral lunar eclipse took place on February 9, 2009, the first of four lunar eclipses in 2009, and being the deepest of three penumbral eclipses.[1] It also happened on the Lantern Festival, the first since February 20, 1989. The tables below contain detailed predictions and additional information on the Penumbral Lunar Eclipse of 9 February 2009.

This is the second eclipse this season.

First eclipse this season: 26 January 2009 Annular Solar Eclipse

Eclipse Characteristics

Penumbral Magnitude: 0.89946

Umbral Magnitude: -0.08818

Gamma: -1.06401

Opposition Times

Greatest Eclipse: 09 Feb 2009 14:38:15.4 UTC (14:39:21.2 TD)

Ecliptic Opposition: 09 Feb 2009 14:49:10.0 UTC (14:50:15.8 TD)

Equatorial Opposition: 09 Feb 2009 15:28:37.6 UTC (15:29:43.5 TD)

Geocentric Coordinates of Sun and Moon

Sun right ascension: 21 hours, 33 minutes, 30.0 seconds

Moon right ascension: 9 hours, 31 minutes, 42.1 seconds

Earth's shadow right ascension: 9 hours, 33 minutes, 30.0 seconds

Sun declination: 14 degrees, 30 minutes, 7.1 seconds south of Celestial Equator

Moon declination: 13 degrees, 31 minutes, 37.5 seconds north of Celestial Equator

Earth's shadow declination: 14 degrees, 30 minutes, 7.1 seconds north of Celestial Equator

Sun diameter: 1945.2 arcseconds

Moon diameter: 1969.6 arcseconds

Earth's penumbral shadow diameter: 2 degrees, 2063.52 arcseconds

Earth's umbral shadow diameter: 1 degree, 1773.36 arcseconds

Saros series: 143rd (17/72)

Delta T: 1 minute, 5.8 seconds

Penumbral Begins: 09 Feb 2009 12:38:46.4 UTC (12:39:52.2 TD)

Greatest Eclipse: 09 Feb 2009 14:38:15.4 UTC (14:39:21.2 TD)

Penumbral Ends: 09 Feb 2009 16:37:39.9 UTC (16:38:45.7 TD)

Total duration: 3 hours, 58 minutes, 53.5 seconds

Visibility

The eclipse was not visible in the East coast of the United States, South America and southernmost Mexico, Western Africa and western Europe. Best visibility was expected over most of Asia, the Western US, Mexico and throughout the Pacific region.[2]


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.

Map

Relation to other eclipses

Eclipses of 2009

Lunar eclipse series sets from 2006–2009
Descending node   Ascending node
Saros #
and photo
Date
Viewing
Type
Chart
Gamma Saros #
and photo
Date
Viewing
Type
Chart
Gamma
113
2006 Mar 14
penumbral
1.0211 118
2006 Sep 7
partial
−0.9262
123
2007 Mar 03
total
0.3175 128
2007 Aug 28
total
−0.2146
133
2008 Feb 21
total
−0.3992 138
2008 Aug 16
partial
0.5646
143
2009 Feb 09
penumbral
−1.0640 148
2009 Aug 06
penumbral
1.3572
Last set 2005 Apr 24 Last set 2005 Oct 17
Next set 2009 Dec 31 Next set 2009 Jul 07


Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[3] This lunar eclipse is related to two partial solar eclipses of Solar Saros 150.

February 5, 2000 February 15, 2018

See also

Notes

  1. ^ eclipse.gsfc.nasa.gov: Penumbral Lunar Eclipse of February 09
  2. ^ Penumbral Lunar Eclipse of 2009 Feb 09
  3. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros