StarCitizen:Baker I: Difference between revisions
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| galactapedia = https://robertsspaceindustries.com/galactapedia/article/Vy2dg37KDa-baker-i | | galactapedia = https://robertsspaceindustries.com/galactapedia/article/Vy2dg37KDa-baker-i | ||
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'''Baker I''' is a small planet with a dense iron core that is in a dangerously close orbit around [[StarCitizen:Baker system|Baker]]'s two suns. This proximity leads to an unstable orbital trajectory, and scientists posit that its orbit will steadily decay until it is subsumed by the larger star within the next one hundred and fifty million years.<ref>{{Cite RSI|url=comm-link/spectrum-dispatch/14230-Baker-System|text=Galactic Guide: Baker System}}</ref> | '''Baker I''' is a small planet with a dense iron core that is in a dangerously close orbit around [[StarCitizen:Baker system|Baker]]'s two suns. This proximity leads to an unstable orbital trajectory, and scientists posit that its orbit will steadily decay until it is subsumed by the larger star within the next one hundred and fifty million years.<ref>{{SC/Cite RSI|url=comm-link/spectrum-dispatch/14230-Baker-System|text=Galactic Guide: Baker System}}</ref> | ||
==References== | ==References== | ||
<references /> | <references /> | ||
{{System navplate|Baker}} | {{SC/System navplate|Baker}} | ||
Revision as of 21:26, 9 April 2026
Template:Astronomical object Baker I is a small planet with a dense iron core that is in a dangerously close orbit around Baker's two suns. This proximity leads to an unstable orbital trajectory, and scientists posit that its orbit will steadily decay until it is subsumed by the larger star within the next one hundred and fifty million years.<ref>Script error: No such module "Cite RSI".</ref>
References
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