Astronomy:HD 173417
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Lyra |
| Right ascension | 18h 43m 51.59217s[1] |
| Declination | +31° 55′ 35.8058″[1] |
| Apparent magnitude (V) | 5.68[2] |
| Characteristics | |
| Spectral type | F1III-IV[3] |
| B−V color index | +0.360±0.004[2] |
| Variable type | Constant[4] |
| Astrometry | |
| Radial velocity (Rv) | −3.26±0.57[1] km/s |
| Proper motion (μ) | RA: −32.768[1] mas/yr Dec.: −125.812[1] mas/yr |
| Parallax (π) | 19.27 ± 0.60[1] mas |
| Distance | 169 ± 5 ly (52 ± 2 pc) |
| Absolute magnitude (MV) | 2.17[5] |
| Details | |
| Mass | 1.60[6] M☉ |
| Radius | 2.243[2] R☉ |
| Luminosity | 10.407[2] L☉ |
| Surface gravity (log g) | 3.91[6] cgs |
| Temperature | 6,928[2] K |
| Metallicity [Fe/H] | −0.21[6] dex |
| Rotational velocity (v sin i) | 53.9±2.7[7] km/s |
| Age | 1.70[6] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 173417 is a single[9] star in the northern constellation of Lyra. It is dimly visible to the naked eye with an apparent visual magnitude of 5.68,[2] positioned about two degrees to the southwest of the bright star Sheliak.[10] The distance to this star is approximately 169 light years based on parallax measurements, and it is slowly drifting closer with a radial velocity of −3 km/s.[1]
The stellar classification of this star is F1III-IV,[3] matching an evolving star with the mixed luminosity traits of a subgiant and giant star. It is 1.7 billion years old with a low metallicity and a relatively high projected rotational velocity of 54 km/s.[7] The star has 1.6[6] times the mass of the Sun and 2.2 times the Sun's radius. It is radiating over 10 times the luminosity of the Sun from its photosphere at an effective temperature of 6,928 K.[2]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 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.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 Schofield, Mathew et al. (2019), "The Asteroseismic Target List for Solar-like Oscillators Observed in 2 minute Cadence with the Transiting Exoplanet Survey Satellite", The Astrophysical Journal Supplement Series 241 (1): 12, doi:10.3847/1538-4365/ab04f5, Bibcode: 2019ApJS..241...12S.
- ↑ 3.0 3.1 Cowley, Anne; Fraquelli, Dorothy (February 1974), "MK Spectral Types for Some Bright F Stars", Publications of the Astronomical Society of the Pacific 86 (509): 70, doi:10.1086/129562, Bibcode: 1974PASP...86...70C.
- ↑ Breger, M. et al. (May 1981), "A Search for Maia Variables", Information Bulletin on Variable Stars 1966: 1, Bibcode: 1981IBVS.1966....1B.
- ↑ Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A.
- ↑ 6.0 6.1 6.2 6.3 6.4 Casagrande, L. et al. (June 1, 2011), "New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey", Astronomy and Astrophysics 530: A138, doi:10.1051/0004-6361/201016276, ISSN 0004-6361, Bibcode: 2011A&A...530A.138C.
- ↑ 7.0 7.1 Reiners, Ansgar (January 2006), "Rotation- and temperature-dependence of stellar latitudinal differential rotation", Astronomy and Astrophysics 446 (1): 267–277, doi:10.1051/0004-6361:20053911, Bibcode: 2006A&A...446..267R.
- ↑ "HD 173417". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+173417.
- ↑ 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, doi:10.1111/j.1365-2966.2008.13596.x, Bibcode: 2008MNRAS.389..869E.
- ↑ Sinnott, Roger W.; Perryman, Michael A. C. (1997), Millennium Star Atlas, 3, Sky Publishing Corporation and the European Space Agency, p. 1175, ISBN 0-933346-84-0.
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