Mu Arae b explained

Mu Arae b / Quijote
Discoverer:Butler, Marcy
Discovery Site:California, US
Discovered:December 12, 2000
Discovery Method:Doppler Spectroscopy
Apsis:astron
Aphelion:1.689AU
Perihelion:1.304AU
Semimajor:1.497AU[1]
Eccentricity:0.128
Period:643.25 ± 0.90 d
1.7611 y
Time Periastron:2452365.6 ± 12.6
Arg Peri:22.0 ± 7.0
Semi-Amplitude:37.78 ± 0.40
Star:Mu Arae

Mu Arae b, often designated HD 160691 b, formally named Quijote, is an exoplanet orbiting the star Mu Arae of the constellation Ara.

The planet is at least one and a half times the mass of Jupiter, and its orbital period is 643.25 days. The discovery of this planet was announced on December 12, 2002, and was originally thought to be on a highly eccentric orbit.[2] The latest models of Mu Arae planetary system, which has four known planets, give a lower eccentricity orbit. Although the planet itself is likely to be a gas giant with no solid surface, the orbital distance of 1.497 astronomical units from its star puts it within the habitable zone of its planetary system. As a result, large satellites of the planet, if they exist, could potentially support life. However, it may not receive enough ultraviolet light for abiogenesis to proceed.[3] Furthermore, it is not clear that Earth-size moons can actually be formed in the environment around a gas giant planet.[4]

Name

In July 2014 the International Astronomical Union launched NameExoWorlds, a process for giving proper names to certain exoplanets and their host stars.[5] The process involved public nomination and voting for the new names.[6] In December 2015, the IAU announced the winning name was Quijote for this planet.[7] The winning name was submitted by the Planetario de Pamplona, Spain. Quijote was the lead character of the novel Don Quixote.[8] Although the character's name is more commonly spelled Quixote in English, Quijote is the current Spanish spelling.

Notes and References

  1. 2007A&A...462..769P. The HARPS search for southern extra-solar planets. VIII. μ Arae, a system with four planets. Pepe, F. . 4 . Correia, A. C. M. . Mayor, M. . Tamuz, O. . Couetdic, J. . Benz, W. . Bertaux, J.-L. . Bouchy, F. . Laskar, J. . Lovis, C. . Naef, D. . Queloz, D. . Santos, N. C. . Sivan, J.-P. . Sosnowska, D. . Udry, S.. Astronomy and Astrophysics. 462. 2. 2007. 769–776. 10.1051/0004-6361:20066194. astro-ph/0608396 . 119071803.
  2. 2001ApJ...555..410B . Butler, R. Paul . 4 . Tinney, C. G. . Marcy, Geoffrey W. . Jones, Hugh R. A. . Penny, Alan J. . Apps, Kevin . Two New Planets from the Anglo-Australian Planet Search . . 555 . 1 . 2001 . 410–417 . 10.1086/321467 . 2299/137 . 122572834 . free .
  3. 2006Icar..183..491B. Buccino, Andrea P. . Lemarchand, Guillermo A. . Mauas, Pablo J. D.. Ultraviolet Radiation Constraints around the Circumstellar Habitable Zones. Icarus. 183. 2. 491 - 503. 2006. 10.1016/j.icarus.2006.03.007. astro-ph/0512291 . 2241081 .
  4. Canup, R. . Robin Canup . Ward, W.. A common mass scaling for satellite systems of gaseous planets. Nature. 441. 2006. 834 - 839. 10.1038/nature04860. 16778883. 7095. 2006Natur.441..834C . 4327454.
  5. http://www.iau.org/news/pressreleases/detail/iau1404/ NameExoWorlds: An IAU Worldwide Contest to Name Exoplanets and their Host Stars
  6. Web site: NameExoWorlds The Process . 2015-09-05 . 2015-08-15 . https://web.archive.org/web/20150815025117/http://nameexoworlds.iau.org/process . dead .
  7. http://www.iau.org/news/pressreleases/detail/iau1514/ Final Results of NameExoWorlds Public Vote Released
  8. Web site: NameExoWorlds The Approved Names . 2016-01-03 . 2018-02-01 . https://web.archive.org/web/20180201043609/http://nameexoworlds.iau.org/names . dead .