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The following other wikis use this file: Usage on ca.wikipedia.org Nodes de la Lluna; Eclipsi de Lluna; Astrologia occidental; Usage on cbk-zam.wikipedia.org
This eclipse is a member of a semester series. 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 June 17, 2038 and December 11, 2038 occur in the next lunar year eclipse set.
English: A diagram illustrating the difference between a full moon and a lunar eclipse, and the difference between a new moon and a solar eclipse. This is caused by the 5° incline of the moon's orbital plane around earth, meaning that an eclipse can only happen when the moon is nearly in line with the nodal line.
This file was derived from: Tom Ruen - Lunar eclipse shadow paths (pd).gif. Transferred from to Commons by Common Good using CommonsHelper. Author: MatthewZimmerman at English Wikipedia: Other versions
More than 100 pages use this file. The following list shows the first 100 pages that use this file only. A full list is available.. April 1977 lunar eclipse; April 1986 lunar eclipse
<noinclude>[[Category:Lunar eclipse templates]]</noinclude> to the end of the template code, making sure it starts on the same line as the code's last character. Pages in category "Lunar eclipse templates"
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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