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Chi Draconis System

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Exoplanetary Scratchpad

[SysBP Img]

Chi Draconis is also known as Gl 713. Nearby yellow-white dwarf star (A) with an orange dwarf companion (B). Star A is also known as HR 6927 and HD 170153, and is a little bit more massive and larger than the Sun. Star B varies from 0.6 to 1.4 AU from the star, to close for a habitable planet, which would orbit at Mars-like distances from Star A. The stars' are significantly non-planar to each other. Star B was first detected by William Wright in 1898. The stars are about a billion years old.

Chi Draconis System Web PagesEdit

Chi Draconis System In the NewsEdit

Sample (Year)Edit

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