Exoplanetary Scratchpad

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Struve 1321 is also known as Gl 338, Sigma 1321, and HD 79210. Nearby double system of late orange dwarf flare stars. First observed as a binary star by Struve in 1817. They are separated on average by 108 AUs. Star A is also known as HD 79210, while B is also known as HD 79211. In the 1970s and 1980s, each star was thought to have an unseen companion per radial velocity measurements, which have since been disproved.

Struve 1321 System Web PagesEdit

Struve 1321 System In the NewsEdit

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