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16 Arietis

From Wikipedia, the free encyclopedia
Star in the constellation Aries
16 Arietis
Observation data
EpochJ2000.0      EquinoxJ2000.0
ConstellationAries
Right ascension02h 11m 12.055s[1]
Declination+25° 56′ 12.99″[1]
Apparent magnitude (V)6.016[2]
Characteristics
Evolutionary stagered giant branch[1]
Spectral typeK3 III[3]
B−Vcolor index1.365±0.006[4]
Astrometry
Radial velocity (Rv)−15.10±0.17[5] km/s
Proper motion (μ)RA: −8.211mas/yr[1]
Dec.: −4.866mas/yr[1]
Parallax (π)6.394±0.0528 mas[1]
Distance510 ± 4 ly
(156 ± 1 pc)
Absolute magnitude (MV)−0.82[4]
Details
Luminosity359.63[6] L
Temperature4,244[6] K
Other designations
BD+25 362,GC 2609,HD 13363,HIP 10203,HR 633,SAO 75188[2]
Database references
SIMBADdata

16 Arietis (abbreviated16 Ari) is astar in the northernconstellation ofAries.16 Arietis is theFlamsteed designation. Itsapparent magnitude is 6.01. Based upon the annualparallax shift of6.27 ± 0.07mas,[5] this star is approximately 520light-years (160parsecs) distant from Earth. The brightness of this star is diminished by 0.40 in magnitude fromextinction caused byinterstellar gas and dust.[7] This is anevolvedgiant star with astellar classification of K3 III.[3]

References

[edit]
  1. ^abcdeVallenari, 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.
  2. ^ab"16 Ari -- Star",SIMBAD Astronomical Database,Centre de Données astronomiques de Strasbourg, retrieved2012-08-13.
  3. ^abSato, K.; Kuji, S. (November 1990), "MK classification and photometry of stars used for time and latitude observations at Mizusawa and Washington",Astronomy and Astrophysics Supplement Series,85 (3):1069–1087,Bibcode:1990A&AS...85.1069S.
  4. ^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.S2CID 119257644.
  5. ^abBrown, 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.
  6. ^abMcDonald, I.; Zijlstra, A. A.; Boyer, M. L. (2012)."Fundamental Parameters and Infrared Excesses of Hipparcos Stars".Monthly Notices of the Royal Astronomical Society.427 (1):343–57.arXiv:1208.2037.Bibcode:2012MNRAS.427..343M.doi:10.1111/j.1365-2966.2012.21873.x.S2CID 118665352.
  7. ^Famaey, B.; et al. (January 2005), "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters",Astronomy and Astrophysics,430 (1):165–186,arXiv:astro-ph/0409579,Bibcode:2005A&A...430..165F,doi:10.1051/0004-6361:20041272,S2CID 17804304.

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