astro.wikisort.org - Meteorite

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

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 ± 40 million km)
Eccentricity	0.02 ± 0.03
Orbital period (sidereal)	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 NameExoWorlds, 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]

See also

• Gemini in Chinese astronomy
• Cancer Minor (constellation) – Obsolete constellation inside modern Gemini
• Sudarsky's gas giant classification

References

• A. P. Hatzes; et al. (1993). "Long-period radial velocity variations in three K giants". The Astrophysical Journal. 413: 339–348. Bibcode:1993ApJ...413..339H. doi:10.1086/173002.
• A. P. Hatzes; et al. (2006). "Confirmation of the planet hypothesis for the long-period radial velocity variations of β Geminorum". Astronomy and Astrophysics. 457 (1): 335–341. arXiv:astro-ph/0606517. Bibcode:2006A&A...457..335H. doi:10.1051/0004-6361:20065445. S2CID 14319327.
• S. Reffert; et al. (2006). "Precise Radial Velocities of Giant Stars. II. Pollux and Its Planetary Companion". The Astrophysical Journal. 652 (1): 661–665. arXiv:astro-ph/0607136. Bibcode:2006ApJ...652..661R. doi:10.1086/507516. S2CID 18252884.

External links

• Hatzes; et al. (2006-06-16). "Confirmation of the Planet Hypothesis of the Long-period Radial velocity Variations of β Geminorum" (PDF). European Southern Observatory. Archived from the original (PDF) on 2007-09-26. Retrieved 2008-06-24.
• "Pollux". SolStation. Retrieved 2005-11-21.
• Sabine Reffert; et al. (2006-07-07). "Precise Radial Velocities of Giant Stars II. Pollux and its Planetary Companion". Astrophysical Journal. 652: 661–665. arXiv:astro-ph/0607136. Bibcode:2006ApJ...652..661R. doi:10.1086/507516. S2CID 18252884.

На других языках

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[de] Pollux b

Pollux b (Thestias) ist ein Exoplanet, der den rund 34 Lichtjahre von der Sonne entfernten Unterriesen Pollux umkreist, den hellsten Stern im Sternbild Zwillinge. Pollux (auch Beta Geminorum) ist damit der von der Erde aus gesehen hellste Stern (1,16 mag), von dem ein Planet bekannt ist.

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- [en] Pollux b

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