MarketSeptember 2006 lunar eclipse
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September 2006 lunar eclipse

A partial lunar eclipse occurred at the Moon's ascending node of orbit on Thursday, September 7, 2006, with an umbral magnitude of 0.1837. 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 4 hours before perigee, the Moon's apparent diameter was larger.

Visibility
The eclipse was completely visible over Asia, east Africa, eastern Europe and western Australia, seen rising over west Africa and western Europe and setting over eastern Australia and the western Pacific Ocean. == Images ==
Gallery
Degania A, Israel File:Astrowoosie - 20.32.29 (by).jpg|North Wales, UK File:Partial-lunar-eclipse-7sept2006-sofia-bulgaria.JPG|Sofia, Bulgaria File:Lunar Eclipse 12.43 (3446066150).jpg|Jaipur, India File:Strollers - lunar eclipse (by-sa).jpg|Shizuoka City, Japan == Eclipse details ==
Eclipse details
Shown below is a table displaying details about this particular lunar eclipse. It describes various parameters pertaining to this eclipse. == Eclipse season ==
Eclipse season
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. == Related eclipses ==
Related eclipses
Eclipses in 2006 A penumbral lunar eclipse on March 14. • A total solar eclipse on March 29. • A partial lunar eclipse on September 7.An annular solar eclipse on September 22. Metonic • Preceded by: Lunar eclipse of November 20, 2002 • Followed by: Lunar eclipse of June 26, 2010 Tzolkinex • Preceded by: Lunar eclipse of July 28, 1999 • Followed by: Lunar eclipse of October 18, 2013 Half-Saros • Preceded by: Solar eclipse of September 2, 1997 • Followed by: Solar eclipse of September 13, 2015 Tritos • Preceded by: Lunar eclipse of October 8, 1995 • Followed by: Lunar eclipse of August 7, 2017 Lunar Saros 118 • Preceded by: Lunar eclipse of August 27, 1988 • Followed by: Lunar eclipse of September 18, 2024 Inex • Preceded by: Lunar eclipse of September 27, 1977 • Followed by: Lunar eclipse of August 19, 2035 Triad • Preceded by: Lunar eclipse of November 7, 1919 • Followed by: Lunar eclipse of July 8, 2093 Lunar eclipses of 2006–2009 Metonic series Saros 118 Tritos series Inex series Half-Saros cycle A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). This lunar eclipse is related to two partial solar eclipses of Solar Saros 125. == See also ==
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