Odius: Difference between revisions

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Odius is the secondary star of the [[Yakei-Odius|Yakei-Odius binary system]]. It is a brown dwarf which orbits [[Yakei]] at a distance of 143.89 AU. It has five planets orbiting it. It has a very long orbital period of approximately 1,800 Y, with its absolute motion over a lifetime slight but noticeable. Its surface temperature is warm enough that it emits a small amount of visible light, although its visibility within the [[Yakeic System]] is dominated by the light it reflects from Yakei.
Odius is the secondary star of the [[Yakei-Odius|Yakei-Odius binary system]]. It is a brown dwarf which orbits [[Yakei]] at a distance of 143.89 AU. It has five planets orbiting it. It has a very long orbital period of approximately 1,800 Y, with its absolute motion over a lifetime slight but noticeable. Its surface temperature is warm enough that it emits a great deal of red light, but very little higher energy light, giving it the appearance of an extremely red, bright point of light from within the [[Yakeic System]].

Latest revision as of 08:54, 18 January 2022

Odius is the secondary star of the Yakei-Odius binary system. It is a brown dwarf which orbits Yakei at a distance of 143.89 AU. It has five planets orbiting it. It has a very long orbital period of approximately 1,800 Y, with its absolute motion over a lifetime slight but noticeable. Its surface temperature is warm enough that it emits a great deal of red light, but very little higher energy light, giving it the appearance of an extremely red, bright point of light from within the Yakeic System.