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Cha 110913-773444
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Cha 110913-773444 : ウィキペディア英語版
Cha 110913-773444



Cha 110913-773444 (sometimes abbreviated ''Cha 110913'') is an astronomical object surrounded by what appears to be a protoplanetary disk. There is no consensus yet among astronomers whether to classify the object as a sub-brown dwarf (with planets) or a rogue planet (with moons).
Cha 110913-773444 was discovered in 2004 by Kevin Luhman and others at Pennsylvania State University using the Spitzer Space Telescope and the Hubble Space Telescope, as well as two Earth-bound telescopes in Chile.
== See also ==

* OTS 44
* SCR 1845-6357
* PSO J318.5-22

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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