Astronomy:HD 166006

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Short description: Double star in the constellation Telescopium
HD 166006
Observation data
Equinox J2000.0]] (ICRS)
Constellation Telescopium
Right ascension  18h 11m 04.40s[1]
Declination −47° 30′ 47.24″[1]
Apparent magnitude (V) 6.07±0.01[2]
Characteristics
Spectral type K1 III CN2[3]
B−V color index +1.20[4]
Astrometry
Radial velocity (Rv)−14.9±2.9[5] km/s
Proper motion (μ) RA: −3.69±0.39[6] mas/yr
Dec.: −29.50±0.23[6] mas/yr
Parallax (π)5.6048 ± 0.0652[1] mas
Distance582 ± 7 ly
(178 ± 2 pc)
Absolute magnitude (MV)−0.12[7]
Details
Mass1.24[8] M☉
Radius20.1[9] R☉
Luminosity165[7] L☉
Surface gravity (log g)1.89[8] cgs
Temperature4,529±93[10] K
Metallicity [Fe/H]−0.07[8] dex
Rotational velocity (v sin i)<1[11] km/s
Other designations
CD−47 12098, HD 166006, HIP 89096, HR 6778, WDS J18111-4731A[12]
Database references
SIMBADdata

HD 166006, also known as HR 6778, is a solitary orange-hued star located in the southern constellation Telescopium. It has an apparent magnitude of 6.07, making it barely visible to the naked eye. Based on Gaia DR2 parallax measurements, the object is located 582 light years away. It is currently approaching the Solar System with a somewhat constrained heliocentric radial velocity of −15 km/s.

HD 166006 has a stellar classification of K1 III CN2,[3] which indicates that it is an evolved red giant with a strong overabundance of cyano radicals in its spectrum, making it a CN star. At the estimated distance of HD 166006, the star has an angular diameter of 1.05 mas.[10] This yields a radius of 20.1 R☉.[9] It has 1.24 times the mass of the Sun[8] and radiates 165 times the luminosity of the Sun[7] from its enlarged photosphere at an effective temperature of 4,529 K.[10] The star is slightly metal deficient ([Fe/H] = −0.07[8]) and spins a little too slowly to be accurately measured.[11]HD 166006 has an optical 11th magnitude companion located 1.8" away along a position angle of 271° as of 2015.[13]

References

  1. ↑ 1.0 1.1 1.2 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.
  2. ↑ Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P. et al. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics 355: L27–L30. ISSN 0004-6361. Bibcode: 2000A&A...355L..27H. 
  3. ↑ 3.0 3.1 Houk, Nancy (1978). Michigan catalogue of two-dimensional spectral types for the HD stars Volume II: Declinations −53° to −40°. Bibcode: 1978mcts.book.....H. 
  4. ↑ Johnson, H. L.; Mitchell, R. I.; Iriarte, B.; Wisniewski, W. Z. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory 4: 99–110. Bibcode: 1966CoLPL...4...99J. 
  5. ↑ Gontcharov, G. A. (November 2006). "Pulkovo Compilation of Radial Velocities for 35,495 Hipparcos stars in a common system". Astronomy Letters 32 (11): 759–771. doi:10.1134/S1063773706110065. ISSN 1063-7737. Bibcode: 2006AstL...32..759G. 
  6. ↑ Template:Cite New HIP red.
  7. ↑ 7.0 7.1 7.2 Anderson, E.; Francis, Ch. (1 May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331–346. doi:10.1134/S1063773712050015. ISSN 1063-7737. Bibcode: 2012AstL...38..331A. 
  8. ↑ 8.0 8.1 8.2 8.3 8.4 Anders, F. et al. (1 August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy and Astrophysics 628: A94. doi:10.1051/0004-6361/201935765. ISSN 0004-6361. Bibcode: 2019A&A...628A..94A. http://pure-oai.bham.ac.uk/ws/files/81053961/aa35765_19.pdf. 
  9. ↑ 9.0 9.1 Lang, Kenneth R. (2006), Astrophysical formulae, Astronomy and astrophysics library, 1 (3 ed.), Birkhäuser, ISBN 3-540-29692-1, https://books.google.com/books?id=OvTjLcQ4MCQC&pg=PA41 . The radius (R*) is given by:
    [math]\displaystyle{ \begin{align} 2\cdot R_* & = \frac{(178\cdot 1.05\cdot 10^{-3})\ \text{AU}}{0.0046491\ \text{AU}/R_{\bigodot}} \\ & \approx 40.2\cdot R_{\bigodot} \end{align} }[/math]
  10. ↑ 10.0 10.1 10.2 Stevens, Daniel J.; Stassun, Keivan G.; Gaudi, B. Scott (1 December 2017). "Empirical Bolometric Fluxes and Angular Diameters of 1.6 Million Tycho-2 Stars and Radii of 350,000 Stars with Gaia DR1 Parallaxes". The Astronomical Journal 154 (6): 259. doi:10.3847/1538-3881/aa957b. ISSN 0004-6256. Bibcode: 2017AJ....154..259S. 
  11. ↑ 11.0 11.1 De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (1 January 2014). "A catalog of rotational and radial velocities for evolved stars. V. Southern stars". Astronomy and Astrophysics 561: A126. doi:10.1051/0004-6361/201220762. ISSN 0004-6361. Bibcode: 2014A&A...561A.126D. 
  12. ↑ "HR 6778". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HR+6778. 
  13. ↑ Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (1 December 2001). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog". The Astronomical Journal 122 (6): 3466–3471. doi:10.1086/323920. ISSN 0004-6256. Bibcode: 2001AJ....122.3466M. 



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