Eta Arietis
Star in the constellation Aries
Eta Arietis , Latinized from η Arietis, is the Bayer designation for a star in the northern constellation of Aries . It is dimly visible to the naked eye with an apparent visual magnitude of 5.231.[ 2] With an annual parallax shift of 33.34 mas ,[ 1] the distance to this star is approximately 97.8 light-years (30.0 parsecs ). It is drifting further away with a radial velocity of +4.5 km/s.[ 2]
This is an F-type main sequence star with a stellar classification of F5 V.[ 3] It is younger than the Sun at an age of about 2.6 billion years.[ 2] The effective temperature of the outer atmosphere is 6,380 K,[ 3] giving it the yellow-white-hued glow of an F-type star . Eta Arietis was examined using the HARPS instrument for radial velocity variations that may be caused by an orbiting companion, but no signal was detected.[ 8] Nor has an infrared excess been detected using the Spitzer Space Telescope , which might otherwise indicate the presence of circumstellar gas or dust.[ 9]
References
^ a b c d e f Brown, A. G. A. ; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties" . Astronomy & Astrophysics . 616 . A1. arXiv :1804.09365 . Bibcode :2018A&A...616A...1G . doi :10.1051/0004-6361/201833051 . Gaia DR2 record for this source at VizieR .
^ a b c d e f g Holmberg, J.; Nordström, B.; Andersen, J. (July 2009), "The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics", Astronomy and Astrophysics , 501 (3): 941–947, arXiv :0811.3982 , Bibcode :2009A&A...501..941H , doi :10.1051/0004-6361/200811191 , S2CID 118577511 .
^ a b c d e Cenarro, A. J.; et al. (January 2007), "Medium-resolution Isaac Newton Telescope library of empirical spectra - II. The stellar atmospheric parameters", Monthly Notices of the Royal Astronomical Society , 374 (2): 664–690, arXiv :astro-ph/0611618 , Bibcode :2007MNRAS.374..664C , doi :10.1111/j.1365-2966.2006.11196.x , S2CID 119428437 .
^ a b c "eta Ari" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2012-08-04 .
^ a b Luck, R. Earle (January 2017), "Abundances in the Local Region II: F, G, and K Dwarfs and Subgiants", The Astronomical Journal , 153 (1): 19, arXiv :1611.02897 , Bibcode :2017AJ....153...21L , doi :10.3847/1538-3881/153/1/21 , S2CID 119511744 , 21.
^ a b c Schofield, Mathew; Chaplin, William J.; Huber, Daniel; Campante, Tiago L.; Davies, Guy R.; Miglio, Andrea; Ball, Warrick H.; Appourchaux, Thierry; Basu, Sarbani; Bedding, Timothy R.; Christensen-Dalsgaard, Jørgen; Creevey, Orlagh; García, Rafael A.; Handberg, Rasmus; Kawaler, Steven D. (2019-03-01), "The Asteroseismic Target List for Solar-like Oscillators Observed in 2 minute Cadence with the Transiting Exoplanet Survey Satellite", The Astrophysical Journal Supplement Series , 241 (1): 12, arXiv :1901.10148 , Bibcode :2019ApJS..241...12S , doi :10.3847/1538-4365/ab04f5 , ISSN 0067-0049 eta Arietis' database entry at VizieR .
^ Takeda, Yoichi; et al. (February 2005), "High-Dispersion Spectra Collection of Nearby F--K Stars at Okayama Astrophysical Observatory: A Basis for Spectroscopic Abundance Standards", Publications of the Astronomical Society of Japan , 57 (1): 13–25, Bibcode :2005PASJ...57...13T , doi :10.1093/pasj/57.1.13 .
^ Lagrange, A.-M.; et al. (February 2009), "Extrasolar planets and brown dwarfs around A-F type stars. VI. High precision RV survey of early type dwarfs with HARPS", Astronomy and Astrophysics , 495 (1): 335–352, arXiv :0809.4636 , Bibcode :2009A&A...495..335L , doi :10.1051/0004-6361:200810105 , S2CID 62894956 .
^ Trilling, D. E.; et al. (February 2008), "Debris Disks around Sun-like Stars", The Astrophysical Journal , 674 (2): 1086–1105, arXiv :0710.5498 , Bibcode :2008ApJ...674.1086T , doi :10.1086/525514 , S2CID 54940779 .
External links