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Gliese 15 Ab

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Planet orbiting Gliese 15 A
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Gliese 15 Ab
Discovery
Discovered byAndrew W. Howard
Discovery siteKeck Observatory
Discovery dateAugust, 2014
Radial velocity
Orbital characteristics
0.074±0.001AU
Eccentricity0.093+0.152
−0.010
11.441+0.004
−0.002
d
StarGroombridge 34A
Physical characteristics
Mass> 3.03M🜨[1]

Gliese 15 Ab (GJ 15 Ab), also calledGroombridge 34 Ab,[note 1] rarely called GX Andromedae b is anextrasolar planet approximately 11light-years away in theconstellation ofAndromeda. It is found in the night sky orbiting the starGliese 15 A, which is atright ascension 00h 18m 22.89s anddeclination +44° 01′ 22.6″.[2]

Discovery

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It was discovered in August 2014,[3] deduced from analysis of theradial velocities of the parent star by the Eta-Earth Survey using HIRES atKeck Observatory. It has around 5.35 ± 0.75Earth masses,[3] and is thought to be aSuper-Earth with a diameter greater than that of the Earth. However, researches using theCARMENES spectrograph failed to detect the planet in 2017.[4] The detection of planet was recovered in 2018, with revised minimum mass of 3.03M🜨.[1]

Orbit

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Gliese 15 Ab has a close inner orbit around Gliese 15 A with a semi-major axis of only 0.0717 ± 0.0034AU, making anorbital period that is just a little longer than 11.4days, the orbit appears to be relatively circular, with anorbital eccentricity of about 0.12. It orbits too close toGliese 15 A to be located in thehabitable zone and is unlikely to harbour life.

Notes

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  1. ^In the discovery paper, discoverers call this object "Gl 15 Ab", and never "Groombridge 34 Ab".

References

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  1. ^abPinamonti, M.; Damasso, M.; Marzari, F.; Sozzetti, A.; Desidera, S.; Maldonado, J.; Scandariato, G.; Affer, L.; Lanza, A. F.; Bignamini, A.; Bonomo, A. S.; Borsa, F.; Claudi, R.; Cosentino, R.; Giacobbe, P.; González-Álvarez, E.; González Hernández, J. I.; Gratton, R.; Leto, G.; Malavolta, L.; Martinez Fiorenzano, A.; Micela, G.; Molinari, E.; Pagano, I.; Pedani, M.; Perger, M.; Piotto, G.; Rebolo, R.; Ribas, I.; et al. (2018). "The HADES RV Programme with HARPS-N at TNG. VIII. GJ15A: A multiple wide planetary system sculpted by binary interaction".Astronomy and Astrophysics.617: A104.arXiv:1804.03476.Bibcode:2018A&A...617A.104P.doi:10.1051/0004-6361/201732535.S2CID 54990041.
  2. ^F. van Leeuwen (2007)Validation of the new Hipparcos reductionArchived 2019-12-07 at theWayback Machine. Astronomy and Astrophysics 474 (2): 653–664.
  3. ^abHoward, Andrew W.; et al. (October 2014), "The NASA-UC-UH ETA-Earth Program. IV. A Low-mass Planet Orbiting an M Dwarf 3.6 PC from Earth",The Astrophysical Journal,794 (1): 9,arXiv:1408.5645,Bibcode:2014ApJ...794...51H,doi:10.1088/0004-637X/794/1/51,S2CID 17361592, 51.
  4. ^Trifonov, Trifon; Kürster, Martin; Zechmeister, Mathias; Tal-Or, Lev; Caballero, José A.; Quirrenbach, Andreas; Amado, Pedro J.; Ribas, Ignasi; Reiners, Ansgar; et al. (2018). "The CARMENES search for exoplanets around M dwarfs. First visual-channel radial-velocity measurements and orbital parameter updates of seven M-dwarf planetary systems".Astronomy and Astrophysics.609. A117.arXiv:1710.01595.Bibcode:2018A&A...609A.117T.doi:10.1051/0004-6361/201731442.S2CID 119340839.

External links

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