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Rho1 Arietis

From Wikipedia, the free encyclopedia
Star in the constellation Aries
For other stars with this Bayer designation, seeρ Arietis.
Rho1 Arietis
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationAries[1]
Right ascension02h 54m 55.205s[2]
Declination+17° 44′ 05.08″[2]
Apparent magnitude (V)7.01[3]
Characteristics
Spectral typeA5 V[4]
U−Bcolor index+0.03[5]
B−Vcolor index+0.28[5]
Astrometry
Radial velocity (Rv)+3.2±3.6[3] km/s
Proper motion (μ)RA: +28.985mas/yr[6]
Dec.: −15.890mas/yr[6]
Parallax (π)12.5263±0.1441 mas[6]
Distance260 ± 3 ly
(79.8 ± 0.9 pc)
Absolute magnitude (MV)+2.43[1]
Details
Mass1.65±0.28[7] M
Radius1.76±0.06[7] R
Luminosity7.86±0.29[7] L
Surface gravity (log g)4.17±0.08[7] cgs
Temperature7,289±126[7] K
Other designations
Rho1 Ari,44 Arietis,BD+17°454,GC 3492,HD 18091,HIP 13579,SAO 93178,PPM 118656,TIC 257918546[8]
Database references
SIMBADdata

Rho1 Arietis is astar in the northernconstellation ofAries, the ram. Its name is aBayer designation that isLatinized from ρ1 Arietis, and abbreviated Rho1 Ari or ρ1 Ari. This star has anapparent visual magnitude of 7.01,[3] making it a challenge to see with thenaked eye even underideal dark-sky conditions. Based upon an annualparallax shift measurement of12.53 mas,[6] it is approximately 260light-years (80parsecs) distant from the Earth.

This is a white-huedA-type main-sequence star with astellar classification of A5 V.[4] It has 1.7 times the mass of the Sun and 1.8 times the Sun's radius. The star is radiating nearly 8 times the luminosity of the Sun from itsphotosphere at aneffective temperature of 7,289 K.[7]

References

[edit]
  1. ^abAnderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation",Astronomy Letters,38 (5): 331,arXiv:1108.4971,Bibcode:2012AstL...38..331A,doi:10.1134/S1063773712050015. XHIP record for this object atVizieR.
  2. ^abVallenari, A.; et al. (Gaia collaboration) (2023),"Gaia Data Release 3. Summary of the content and survey properties",Astronomy and Astrophysics,674: A1,arXiv:2208.00211,Bibcode:2023A&A...674A...1G,doi:10.1051/0004-6361/202243940,S2CID 244398875. Gaia DR3 record for this source atVizieR.
  3. ^abcGontcharov, G. A. (November 2006), "Pulkovo Compilation of Radial Velocities for 35,495 Hipparcos stars in a common system",Astronomy Letters,32 (11):759–771,arXiv:1606.08053,Bibcode:2006AstL...32..759G,doi:10.1134/S1063773706110065,S2CID 119231169.
  4. ^abAndersson, B.-G.; et al. (2002), "A Spectroscopic and Photometric Survey of Stars in the Field of L1457: A New Distance Determination",The Astronomical Journal,124 (4): 2164,Bibcode:2002AJ....124.2164A,doi:10.1086/342541.
  5. ^abOja, T. (1987), "UBV photometry of stars whose positions are accurately known",Astronomy and Astrophysics Supplement Series,71: 561,Bibcode:1987A&AS...71..561O.
  6. ^abcvan 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.
  7. ^abcdefStassun, Keivan G.; et al. (October 2019), "The Revised TESS Input Catalog and Candidate Target List",The Astronomical Journal,158 (4): 138,arXiv:1905.10694,Bibcode:2019AJ....158..138S,doi:10.3847/1538-3881/ab3467,hdl:1721.1/124721,ISSN 0004-6256,S2CID 166227927.
  8. ^"rho01 Ari",SIMBAD,Centre de données astronomiques de Strasbourg, retrieved2025-05-07.

External links

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