Exoplanetary Scratchpad

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Lacaille 9352 is also called Gl 887 and HD 217987 and informally Proxima Piscis Austrini. Nearby red dwarf star with about half the sun's mass and radius. It is the second bright red dwarf in the sky, but is too dim to see unaided. Its high proper motion was discovered by Gould.

Lacaille 9352 System Web PagesEdit

Lacaille 9352 System In the NewsEdit

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