Tau6 Serpentis
Appearance
(Redirected from BD+16 2816)
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Serpens[1] |
Right ascension | 15h 40m 59.1008s[2] |
Declination | +16° 01′ 28.517″[2] |
Apparent magnitude (V) | 6.000[2] |
Characteristics | |
Spectral type | G8III[2] |
U−B color index | +0.61[3] |
B−V color index | +0.90[3] |
R−I color index | +0.46[3] |
Astrometry | |
Radial velocity (Rv) | 3.4±0.9[2] km/s |
Proper motion (μ) | RA: 22.16[2] mas/yr Dec.: −16.80[2] mas/yr |
Parallax (π) | 7.24±0.79 mas[2] |
Distance | approx. 450 ly (approx. 140 pc) |
Absolute magnitude (MV) | −0.33[1] |
Details | |
Mass | 3.2[4] M☉ |
Radius | 15[4] R☉ |
Luminosity | 137[4] L☉ |
Surface gravity (log g) | 2.64[4] cgs |
Temperature | 5,126[4] K |
Metallicity [Fe/H] | −0.01[4] dex |
Rotational velocity (v sin i) | 4,5[5] km/s |
Age | 310[4] Myr |
Other designations | |
τ6 Ser, 19 Serpentis, BD+16°2816, GC 21089, HD 140027, HIP 76810, HR 5840, SAO 101678, PPM 131601 τ6 Ser, Tau6 Serpentis, Tau6 Ser, 19 Serpentis, 19 Ser, BD+16 2816, GC 21089, HD 140027, HIP 76810, HR 5840, PPM 131601, SAO 101678.[2] | |
Database references | |
SIMBAD | data |
Tau6 Serpentis, Latinized from τ6 Serpentis, is a G-type giant star in the constellation of Serpens, approximately 450 light-years from the Earth.[2] It has an apparent visual magnitude of approximately 6.000,[2] and is a member of the Ursa Major Stream.[3]
References
[edit]- ^ a b Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv:1108.4971, Bibcode:2012AstL...38..331A, doi:10.1134/S1063773712050015, S2CID 119257644.
- ^ a b c d e f g h i j k * 19 Ser -- Star, database entry, SIMBAD. Accessed on line September 19, 2008.
- ^ a b c d HR 5840, database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr., CDS ID V/50. Accessed September 19, 2008.
- ^ a b c d e f g Reffert, Sabine; Bergmann, Christoph; Quirrenbach, Andreas; Trifonov, Trifon; Künstler, Andreas (2015). "Precise radial velocities of giant stars. VII. Occurrence rate of giant extrasolar planets as a function of mass and metallicity". Astronomy and Astrophysics. 574: A116. arXiv:1412.4634. Bibcode:2015A&A...574A.116R. doi:10.1051/0004-6361/201322360.
- ^ Hekker, S.; Meléndez, J. (2007). "Precise radial velocities of giant stars. III. Spectroscopic stellar parameters". Astronomy and Astrophysics. 475 (3): 1003. arXiv:0709.1145. Bibcode:2007A&A...475.1003H. doi:10.1051/0004-6361:20078233.