Pollux b

Pollux b, also designated β Geminorum b (Latinized to beta Geminorum b, abbreviated, β Gem b) and HD 62509 b, formally named Thestias /ˈθɛstiəs/, is an extrasolar planet approximately 34 light-years away in the constellation of Gemini (the Twins). This planet was discovered orbiting the star Pollux in 2006 by astronomer Artie P. Hatzes, confirming his hypothesis originally published in 1993. The planet has at least twice the mass of Jupiter. It moves around Pollux in 1.61 years at a distance of 1.64 AU in a nearly circular orbit.

Pollux b

Discovery
Discovered by	Hatzes et al.
Discovery site	United States
Discovery date	16 June 2006
Detection method	Radial velocity
Orbital characteristics
Semi-major axis	1.64 ± 0.27 AU (245,000,000 ± 40,000,000 km)
Eccentricity	0.02±0.03
Orbital period	589.64±0.81 d 1.61432±0.00222 y
Time of periastron	2,447,739.02±4.5
Semi-amplitude	41.0±1.6
Star	Pollux

In July 2014 the International Astronomical Union launched a process for giving proper names to certain exoplanets and their host stars.[1] The process involved public nomination and voting for the new names.[2] In December 2015, the IAU announced the winning name was Thestias for this planet.[3] The winning name was based on that originally submitted by theSkyNet of Australia; namely Leda, Pollux's mother in Greek and Roman mythology. At the request of the IAU, 'Thestias' (the patronym of Leda, a daughter of Thestius) was substituted. This was because 'Leda' was already attributed to an asteroid and to one of Jupiter's satellites.[4][5]