Astronomy:9 Lacertae
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Lacerta |
| Right ascension | 22h 37m 22.41727s[1] |
| Declination | +51° 32′ 42.4383″[1] |
| Apparent magnitude (V) | 4.64[2] |
| Characteristics | |
| Evolutionary stage | main sequence |
| Spectral type | A9VkA7mA6[3] |
| B−V color index | 0.254±0.006[2] |
| Astrometry | |
| Radial velocity (Rv) | +10.1±1.5[2] km/s |
| Proper motion (μ) | RA: −51.83[1] mas/yr Dec.: −103.80[1] mas/yr |
| Parallax (π) | 19.00 ± 0.19[1] mas |
| Distance | 172 ± 2 ly (52.6 ± 0.5 pc) |
| Absolute magnitude (MV) | 1.03[2] |
| Details | |
| Mass | 1.59[4] M☉ |
| Radius | 2.1[5] R☉ |
| Luminosity | 34.6+0.9 −1.0[6] L☉ |
| Surface gravity (log g) | 3.77±0.14[4] cgs |
| Temperature | 7,614±259[4] K |
| Metallicity [Fe/H] | −0.20[7] dex |
| Rotational velocity (v sin i) | 105[6] km/s |
| Age | 513[4] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
9 Lacertae is a single[9] star in the northern constellation Lacerta, located 172 light years away from Sun.[1] It is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 4.64.[2] This object is moving further from the Earth with a heliocentric radial velocity of +10 km/s.[2]
This is an A-type main-sequence star with a stellar classification of A9VkA7mA6.[3] This notation indicates it has the Hydrogen lines of an A9 star, the Calcium K line of an A7 star, and the metal lines of an A6. It is 513[4] million years old with a high projected rotational velocity of 105 km/s.[6] The star has 1.59[4] times the mass of the Sun and about 2.1[5] times the Sun's radius. It is radiating 34.6[6] times the Sun's luminosity from its photosphere at an effective temperature of 7,614 K.[4]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, doi:10.1051/0004-6361:20078357, Bibcode: 2007A&A...474..653V.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A.
- ↑ 3.0 3.1 Gray, R. O. et al. (2001), "The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. I. Precise Spectral Types for 372 Stars", The Astronomical Journal 121 (4): 2148, doi:10.1086/319956, Bibcode: 2001AJ....121.2148G.
- ↑ 4.0 4.1 4.2 4.3 4.4 4.5 4.6 David, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets", The Astrophysical Journal 804 (2): 146, doi:10.1088/0004-637X/804/2/146, Bibcode: 2015ApJ...804..146D.
- ↑ 5.0 5.1 Pasinetti Fracassini, L. E. et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)", Astronomy and Astrophysics 367: 521–524, doi:10.1051/0004-6361:20000451, Bibcode: 2001A&A...367..521P.
- ↑ 6.0 6.1 6.2 6.3 Zorec, J. et al. (2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy and Astrophysics 537: A120, doi:10.1051/0004-6361/201117691, Bibcode: 2012A&A...537A.120Z.
- ↑ Erspamer, D.; North, P. (February 2003), "Automated spectroscopic abundances of A and F-type stars using echelle spectrographs. II. Abundances of 140 A-F stars from ELODIE", Astronomy and Astrophysics 398 (3): 1121–1135, doi:10.1051/0004-6361:20021711, Bibcode: 2003A&A...398.1121E.
- ↑ "9 Lac". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=9+Lac.
- ↑ Eggleton, P. P.; Tokovinin, A. A. (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.
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