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HD 166066

From Wikipedia, the free encyclopedia
Star in the constellation Octans
HD 166066
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationOctans
Right ascension18h 38m 51.0741s[1]
Declination−85° 42′ 32.2260″[1]
Apparent magnitude (V)8.10±0.01[2]
Characteristics
Spectral typeG0 V[3]
B−Vcolor index+0.59[2]
Astrometry
Radial velocity (Rv)2.93±2.55[4] km/s
Proper motion (μ)RA: +147.318mas/yr[1]
Dec.: −43.097mas/yr[1]
Parallax (π)14.5962±0.1186 mas[1]
Distance223 ± 2 ly
(68.5 ± 0.6 pc)
Absolute magnitude (MV)4.09[5]
Details
Mass1.13[6] M
Radius1.39+0.07
−0.05
[7] R
Luminosity2.12[5] L
Surface gravity (log g)4.25[6] cgs
Temperature6,054±80[6] K
Metallicity [Fe/H]−0.03[6] dex
Rotational velocity (v sin i)5[8] km/s
Age7.0+2.5
−1.2
[9] Gyr
Other designations
CD−85°150,CPD−85°478,HD 166066,HIP 91434,GSC 09527-01174[10]
Database references
SIMBADdata

HD 166066 is a solitarystar located in the southerncircumpolar constellationOctans. It has anapparent magnitude of 8.10,[2] making it readily visible in binoculars, but not to thenaked eye. The object is located 223light years away from theSolar System,[1] but is drifting away with a poorly constrainedradial velocity of about2.93 km/s.[4]

HD 166066 has astellar classification of G0 V, indicating that it is aG-type main sequence star similar to theSun.[3] However, thecalcium H & K lines are narrow and weak for its class.[3] It has 113% themass of the Sun[6] and 139% its radius, along with twice itsluminosity.[5][7]

Theiron abundance is 93% that of the Sun, and is slightly hotter, with aneffective temperature of 6,054K[6] compared to the Sun's 5,778 K. HD 166066 is significantly older, with an age of 7billion years,[9] and rotates modestly with aprojected rotational velocity ofkm/s.[8]

References

[edit]
  1. ^abcdeBrown, A. G. A.; et al. (Gaia collaboration) (2021)."Gaia Early Data Release 3: Summary of the contents and survey properties".Astronomy & Astrophysics.649: A1.arXiv:2012.01533.Bibcode:2021A&A...649A...1G.doi:10.1051/0004-6361/202039657.S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source atVizieR.
  2. ^abcHøg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars".Astronomy and Astrophysics.355:L27 –L30.Bibcode:2000A&A...355L..27H.ISSN 0004-6361.
  3. ^abcHouk, N.; Cowley, A. P. (1975).University of Michigan Catalogue of two-dimensional spectral types for the HD stars. Volume I. Declinations -90_ to -53_ƒ0.Bibcode:1975mcts.book.....H.
  4. ^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. Gaia DR2 record for this source atVizieR.
  5. ^abcAnderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation".Astronomy Letters.38 (5):331–346.arXiv:1108.4971.Bibcode:2012AstL...38..331A.doi:10.1134/S1063773712050015.ISSN 1063-7737.S2CID 255204555.
  6. ^abcdefCasagrande, L.; Schönrich, R.; Asplund, M.; Cassisi, S.; Ramírez, I.; Meléndez, J.; Bensby, T.; Feltzing, S. (June 2011)."New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s): Improved astrophysical parameters for the Geneva-Copenhagen Survey⋆".Astronomy & Astrophysics.530: A138.arXiv:1103.4651.Bibcode:2011A&A...530A.138C.doi:10.1051/0004-6361/201016276.ISSN 0004-6361.
  7. ^abStassun, Keivan G.; et al. (9 September 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.ISSN 0004-6256.
  8. ^abNordström, B.; Mayor, M.; Andersen, J.; Holmberg, J.; Pont, F.; Jørgensen, B. R.; Olsen, E. H.; Udry, S.; Mowlavi, N. (May 2004)."The Geneva-Copenhagen survey of the Solar neighbourhood: Ages, metallicities, and kinematic properties of ~14 000 F and G dwarfs".Astronomy & Astrophysics.418 (3):989–1019.arXiv:astro-ph/0405198.Bibcode:2004A&A...418..989N.doi:10.1051/0004-6361:20035959.ISSN 0004-6361.
  9. ^abHolmberg, J.; Nordström, B.; Andersen, J. (July 2009)."The Geneva-Copenhagen survey of the solar neighbourhood: III. Improved distances, ages, and kinematics".Astronomy & Astrophysics.501 (3):941–947.arXiv:0811.3982.Bibcode:2009A&A...501..941H.doi:10.1051/0004-6361/200811191.ISSN 0004-6361.
  10. ^"HD 166066".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedJune 25, 2022.
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