Pi Mensae

4.7 L ☉

Mensae π (Pi Mensae, π Men), also known as HD 39091, a 60 light-years distant supergiant of spectral type G3 with an apparent magnitude of 5.7 is like.

The star is surrounded by a sub-stellar object with the systematic name Pi Mensae b, in which it could be a exoplanets ( Butler et al., 2001).

Mensa (constellation) Declination Color index Astrometry Radial velocity Intrinsic brightness Proper motion Solar mass Bright Star Catalogue Smithsonian Astrophysical Observatory Star Catalog Subgiant R. Paul Butler
652106
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