Astronomy:HD 193664
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Draco |
| Right ascension | 20h 17m 31.328s[1] |
| Declination | +66° 51′ 13.28″[1] |
| Apparent magnitude (V) | 5.93[2] |
| Characteristics | |
| Spectral type | G3 V[3] |
| U−B color index | +0.06[2] |
| B−V color index | +0.58[2] |
| Astrometry | |
| Radial velocity (Rv) | −4.7[4] km/s |
| Proper motion (μ) | RA: +468.684[1] mas/yr Dec.: +297.589[1] mas/yr |
| Parallax (π) | 57.2041 ± 0.0208[1] mas |
| Distance | 57.02 ± 0.02 ly (17.481 ± 0.006 pc) |
| Absolute magnitude (MV) | 4.65[2] |
| Details | |
| Mass | 1.04[5] M☉ |
| Radius | 1.03[6] R☉ |
| Luminosity | 1.1[5] L☉ |
| Surface gravity (log g) | 4.45[5] cgs |
| Temperature | 5,922[5] K |
| Metallicity [Fe/H] | −0.13[4] dex |
| Rotational velocity (v sin i) | 1.3[7] km/s |
| Age | 3.18[5] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 193664 a star in the northern constellation of Draco. HD 193664 is its Henry Draper Catalogue designation. With an apparent magnitude of 5.93,[2] according to the Bortle Scale it is visible to the naked eye from suburban skies. Parallax measurements yield an estimated distance of 57 light years.[1] It has a relatively large proper motion of 0.558 arc seconds per year across the sky,[9] and is drifting closer to the Sun with a radial velocity of −4.7 km/s.[4]
This star is considered a solar analog—meaning that it is photometrically analogous to the Sun—and it displays no significant variability.[10] It is a G-type main sequence star with a stellar classification of G3V.[3] Both the mass and radius of HD 193664 differ from those of the Sun by just a few percent, although it has a somewhat lower metallicity.[4] It may be around the same age as the Sun, being an estimated 3.2 billion years old.[5] The effective temperature of the stellar atmosphere is 5,922 K,[5] giving it the yellow-hued glow of a G-type star.[11]
HD 193664 has been examined for signs of an infrared excess that could indicate the presence of a circumstellar disk of dust, but none has been found (as of 2012).[12] This is member of the thin disk population of stars that lie near the galactic plane.[4]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 Brown, A. G. A. (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics 649: A1. doi:10.1051/0004-6361/202039657. Bibcode: 2021A&A...649A...1G. Gaia EDR3 record for this source at VizieR.
- ↑ 2.0 2.1 2.2 2.3 2.4 Karatas, Y.; Schuster, W. J. (October 2006), "Metallicity and absolute magnitude calibrations for UBV photometry", Monthly Notices of the Royal Astronomical Society 371 (4): 1793–1812, doi:10.1111/j.1365-2966.2006.10800.x, Bibcode: 2006MNRAS.371.1793K.
- ↑ 3.0 3.1
- ↑ 4.0 4.1 4.2 4.3 4.4 Ramírez, I. et al. (February 2013), "Oxygen abundances in nearby FGK stars and the galactic chemical evolution of the local disk and halo", The Astrophysical Journal 764 (1): 78, doi:10.1088/0004-637X/764/1/78, Bibcode: 2013ApJ...764...78R.
- ↑ 5.0 5.1 5.2 5.3 5.4 5.5 5.6 Luck, R. Earle (January 2017), "Abundances in the Local Region II: F, G, and K Dwarfs and Subgiants", The Astronomical Journal 153 (1): 19, doi:10.3847/1538-3881/153/1/21, 21, Bibcode: 2017AJ....153...21L.
- ↑ Takeda, Genya et al. (February 2007), "Structure and Evolution of Nearby Stars with Planets. II. Physical Properties of ~1000 Cool Stars from the SPOCS Catalog", The Astrophysical Journal Supplement Series 168 (2): 297–318, doi:10.1086/509763, Bibcode: 2007ApJS..168..297T.
- ↑ Valenti, Jeff A.; Fischer, Debra A. (July 2005), "Spectroscopic Properties of Cool Stars (SPOCS). I. 1040 F, G, and K Dwarfs from Keck, Lick, and AAT Planet Search Programs", The Astrophysical Journal Supplement Series 159 (1): 141–166, doi:10.1086/430500, Bibcode: 2005ApJS..159..141V.
- ↑ "HD 193664". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+193664.
- ↑ Lépine, Sébastien; Shara, Michael M. (March 2005), "A Catalog of Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog)", The Astronomical Journal 129 (3): 1483–1522, doi:10.1086/427854, Bibcode: 2005AJ....129.1483L.
- ↑ Metlov, V. G. (January 2003), "Photoelectric Observations of Bright Solar Type Stars", Astronomical and Astrophysical Transactions 22 (1): 47–50, doi:10.1080/1055679021000020020, Bibcode: 2003A&AT...22...47M.
- ↑ "The Colour of Stars", Australia Telescope, Outreach and Education (Commonwealth Scientific and Industrial Research Organisation), December 21, 2004, http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html, retrieved 2012-01-16.
- ↑ Maldonado, J. et al. (May 2012), "Metallicity of solar-type stars with debris discs and planets⋆", Astronomy & Astrophysics 541: 10, doi:10.1051/0004-6361/201218800, A40, Bibcode: 2012A&A...541A..40M.
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