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An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit. [ 1 ] The penumbral lunar eclipses on February 9, 2009 and August 6, 2009 occur in the previous lunar year eclipse set, and the lunar eclipses on April 25, 2013 (partial) and October 18, 2013 ...
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An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit. [1] The lunar eclipses on July 7, 2009 (penumbral) and December 31, 2009 (partial) occur in the next lunar year eclipse set.
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 ...
English: Diagram of lunar phases. The lunar phase depends on the Moon's position in orbit around the Earth and the Earth's position in orbit around the sun. Graphics of the Earth and Moon were obtained from the NASA public domain images File:The Earth seen from Apollo 17.jpg and File:Moon_PIA00302.jpg
A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Thursday, August 6, 2009, [1] with an umbral magnitude of −0.6642. 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 ...