StarCitizen:Oretani VI: Difference between revisions
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'''Oretani VI''' is a dwarf planet on a lonely orbit around the edge of the system.<ref>Starmap: Oretani VI</ref> Located on the very outskirts of the system, the planet has an orbit that takes thousands of days to complete.<ref name="GAORVI">{{ | '''Oretani VI''' is a dwarf planet on a lonely orbit around the edge of the system.<ref>Starmap: Oretani VI</ref> Located on the very outskirts of the system, the planet has an orbit that takes thousands of days to complete.<ref name="GAORVI">{{Cite RSI|text=Galactapedia: Oretani VI|url=https://robertsspaceindustries.com/galactapedia/article/0GxAvne3wa-oretani-vi|accessdate=2023-02-01}}</ref> | ||
Oretani VI is largely dark red in color, caused by the presence of a hydrocarbon sludge on its surface formed from simple organic compounds long exposed to ultraviolet radiation. Methane ice is visible in the areas around impact craters<ref name="GAORVI" />. | Oretani VI is largely dark red in color, caused by the presence of a hydrocarbon sludge on its surface formed from simple organic compounds long exposed to ultraviolet radiation. Methane ice is visible in the areas around impact craters<ref name="GAORVI" />. | ||
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{{ | {{System map|Oretani}} | ||
{{System navplate|Oretani}} | |||
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Revision as of 11:31, 15 August 2026
Template:Infobox Astronomical Object
Oretani VI is a dwarf planet on a lonely orbit around the edge of the system.<ref>Starmap: Oretani VI</ref> Located on the very outskirts of the system, the planet has an orbit that takes thousands of days to complete.<ref name="GAORVI">Template:Cite RSI</ref>
Oretani VI is largely dark red in color, caused by the presence of a hydrocarbon sludge on its surface formed from simple organic compounds long exposed to ultraviolet radiation. Methane ice is visible in the areas around impact craters<ref name="GAORVI" />.
References
<references />