Astronomy:HD 163145
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Scorpius[1] |
| Right ascension | 17h 56m 47.41221s[2] |
| Declination | −44° 20′ 31.9504″[2] |
| Apparent magnitude (V) | 4.85[1] |
| Characteristics | |
| Spectral type | K2 III[3] |
| B−V color index | 1.176±0.062[1] |
| Astrometry | |
| Radial velocity (Rv) | +35.60±0.45[2] km/s |
| Proper motion (μ) | RA: −0.825±0.370[2] mas/yr Dec.: −27.277±0.317[2] mas/yr |
| Parallax (π) | 10.6395 ± 0.2141[2] mas |
| Distance | 307 ± 6 ly (94 ± 2 pc) |
| Absolute magnitude (MV) | 0.12[1] |
| Details | |
| Mass | 1.5[4] M☉ |
| Radius | 20.40+0.41 −0.66[2] R☉ |
| Luminosity | 147.0±3.4[2] L☉ |
| Surface gravity (log g) | 2.17[4] cgs |
| Temperature | 4,450+74 −46[2] K |
| Metallicity [Fe/H] | −0.04[4] dex |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 163145 is a single[6] star in the constellation Scorpius, near the southeast constellation border with Corona Australis. It has an orange hue and is faintly visible to the naked eye with an apparent visual magnitude of 4.85.[1] Based on parallax measurements, it is located at a distance of approximately 307 light years from the Sun. The star is drifting further away with a radial velocity of +35.6 km/s,[2] having come to within 49.2 light-years of the Sun some 1.871 million years ago.[1] It has an absolute magnitude of 0.12.[2]
This object is an aging giant star with a stellar classification of K2 III.[3] With the supply of hydrogen exhausted at its core, the star has cooled and expanded off the main sequence. At present it has 20 times the radius of the Sun. The star is radiating 147 times the Sun's luminosity from its swollen photosphere at an effective temperature of 4,450 K.[2]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A.
- ↑ 2.00 2.01 2.02 2.03 2.04 2.05 2.06 2.07 2.08 2.09 2.10 2.11 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.
- ↑ 3.0 3.1 Houk, N. (1978). Michigan catalogue of two-dimensional spectral types for the HD stars. 2. Dept. of Astronomy, University of Michigan. Bibcode: 1978mcts.book.....H.
- ↑ 4.0 4.1 4.2 Khalatyan, A.; Anders, F.; Chiappini, C.; Queiroz, A. B. A.; Nepal, S.; Dal Ponte, M.; Jordi, C.; Guiglion, G. et al. (2024). "Transferring spectroscopic stellar labels to 217 million Gaia DR3 XP stars with SHBoost". Astronomy and Astrophysics 691: A98. doi:10.1051/0004-6361/202451427. Bibcode: 2024A&A...691A..98K.
- ↑ "HD 163145". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+163145.
- ↑ 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.
 |  |
