Difference between revisions of "Himalia"
Jump to navigation
Jump to search
(HImalia.) Tag: Removed redirect |
(Added category.) |
||
(3 intermediate revisions by the same user not shown) | |||
Line 69: | Line 69: | ||
Animation of Himalia orbit around Jupiter.gif|<center>Animation of Himalia's orbit over time due to perturbations,<br>from Wikimedia Commons</center> | Animation of Himalia orbit around Jupiter.gif|<center>Animation of Himalia's orbit over time due to perturbations,<br>from Wikimedia Commons</center> | ||
</gallery> | </gallery> | ||
+ | |||
+ | [[Category:Articles]] | ||
+ | [[Category:Celestial bodies]] | ||
+ | [[Category:Solar System]] | ||
+ | [[Category:Natural satellites]] | ||
+ | [[Category:Satellites of Jupiter]] | ||
{{JupiterSat}} | {{JupiterSat}} | ||
{{SolarSystem}} | {{SolarSystem}} |
Latest revision as of 03:41, 12 September 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 stellite 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]
|