Difference between revisions of "Himalia"
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+ | |[https://www.orbiter-forum.com/resources/celestial-bodies-motion-part-2-4-v2-0-0.295/ Celestial Bodies Motion - Part 2/4 - v2.0.0]||O-F Resources||v2.0.0||cristiapi||Scenery||2 July 2015||*module only|| | ||
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|[https://library.avsim.net/esearch.php?DLID=&Name=&FileName=outer_planets-060929-base.zip&Author=&CatID=root The Outer Planets 060929 Base]||AVSIM||||Rolf Keibel<br>Carl Romanik<br>Tony Dunn||Scenery||30 September 2006||Orbiter 2006-P1|| | |[https://library.avsim.net/esearch.php?DLID=&Name=&FileName=outer_planets-060929-base.zip&Author=&CatID=root The Outer Planets 060929 Base]||AVSIM||||Rolf Keibel<br>Carl Romanik<br>Tony Dunn||Scenery||30 September 2006||Orbiter 2006-P1|| |
Latest revision as of 13:16, 10 November 2024
This natural satellite related article is a stub. You can help Orbiterwiki by expanding it.
Himalia (Jupiter VI) is the is the largest irregular satellite and the sixth largest satellite of Jupiter. It was discovered by Charles Dillon Perrine at the Lick Observatory on 3 December 1904. Himalia was named after a nymph in Greek mythology who bore three sons by Zeus. Himalia in Orbiter[edit]Himalia was introduced to Orbiter with the release of jupiter-iii.zip in October 2002.
See also[edit]Gallery[edit]
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