Binary star system in the constellation Aries
For other stars with this Bayer designation , see ρ Arietis .
Rho Arietis
Observation dataEpoch J2000.0 Equinox J2000.0 (ICRS )
Constellation
Aries
Right ascension
02 56 26.1549
Declination
+18° 01′ 23.2277″
Apparent magnitude (V)
5.63
Characteristics
Spectral type
F6 V
U−B color index
−0.02
B−V color index
+0.44
V−R color index
0.3
R−I color index
0.2
Astrometry Radial velocity (Rv )+10.5 km/s Proper motion (μ) RA: +281.75 mas /yr Dec.: −218.90 mas /yr Parallax (π)28.29 ± 0.43 mas Distance 115 ± 2 ly (35.3 ± 0.5 pc ) Absolute magnitude (MV )2.89
Details Surface gravity (log g )4.19 cgs Temperature 6,380 K Metallicity 0.23 dex Rotational velocity (v sin i )15 km/s Age 2.4 Gyr
Other designations ρ Ari, Rho Arietis, Rho Ari, 46 Arietis , 46 Ari, BD +17 458, FK5 2204, GC 3532, HD 18256, HIP 13702, HR 869, LTT 10961, NLTT 9363, PPM 118684, SAO 93195.
Database references SIMBAD data
Rho Arietis (Rho Ari , ρ Arietis , ρ Ari ) is the Bayer designation for a star in the northern constellation of Aries . It is faintly visible to the naked eye with an apparent visual magnitude of 5.63. Based upon an annual parallax shift of 28.29 mas , this star is located at a distance of approximately 115 light-years (35 parsecs ) from Earth.
This is an astrometric binary system. The visible component is an F-type main sequence star with a stellar classification of F6 V. It is around 2.4 billion years old and has a high abundance of elements other than hydrogen and helium when compared to the Sun.
Name
This star, along with δ Ari , ε Ari , ζ Ari , and π Ari , were Al Bīrūnī's Al Buṭain (ألبطين ), the dual of Al Baṭn , the Belly. According to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars , Al Buṭain were the title for five stars : δ Ari as Botein , π Ari as Al Buṭain I , ρ Ari as Al Buṭain II , ε Ari as Al Buṭain III dan ζ Ari as Al Buṭain IV
References
^ van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics , 474 (2): 653–664, arXiv :0708.1752 , Bibcode :2007A&A...474..653V , doi :10.1051/0004-6361:20078357 , S2CID 18759600 .
^ "rho Ari" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2012-08-09.{{cite web }}
: CS1 maint: postscript (link )
^ Abt, Helmut A. (January 2009), "MK Classifications of Spectroscopic Binaries", The Astrophysical Journal Supplement , 180 (1): 117–118, Bibcode :2009ApJS..180..117A , doi :10.1088/0067-0049/180/1/117 , S2CID 122811461 .
^ 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
^ Balachandran, Suchitra (May 1, 1990), "Lithium depletion and rotation in main-sequence stars", Astrophysical Journal, Part 1 , 354 : 310–332, Bibcode :1990ApJ...354..310B , doi :10.1086/168691 .
Bernacca, P. L.; Perinotto, M. (1970), "A catalogue of stellar rotational velocities", Contributi Osservatorio Astronomico di Padova in Asiago , 239 (1): 1, Bibcode :1970CoAsi.239....1B .
Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society , 389 (2): 869–879, arXiv :0806.2878 , Bibcode :2008MNRAS.389..869E , doi :10.1111/j.1365-2966.2008.13596.x , S2CID 14878976 .
Allen, R. H. (1963), Star Names: Their Lore and Meaning (Reprint ed.), New York, NY: Dover Publications Inc, p. 83 , ISBN 0-486-21079-0 , retrieved 2010-12-12.
Jack W. Rhoads - Technical Memorandum 33-507-A Reduced Star Catalog Containing 537 Named Stars , Jet Propulsion Laboratory, California Institute of Technology; November 15, 1971
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