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Z Chamaeleontis : ウィキペディア英語版
Z Chamaeleontis


Z Chamaeleontis (abbreviated Z Cha) is an dwarf nova variable star system approximately 316 light-years away from the Sun, where two stars orbit each other every 1.78 hours. The system comprises an eclipsing white dwarf and red dwarf and possibly a yet unconfirmed third low-mass substellar companion.
== Substellar companion ==

Dai et al. (2009) invoke the presence of a third object to explain orbital period variations with an apparent periodicity of roughly 28 years. The third body could yield a minimum mass 20 times greater than Jupiter and be located 9.9 Astronomical Units away from the dwarf nova, being likely a low-mass brown dwarf.


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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