Astronomy:HD 169405
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Telescopium |
| Right ascension | 18h 26m 54.01379s[1] |
| Declination | −48° 07′ 02.0638″[1] |
| Apparent magnitude (V) | +5.44[2] |
| Characteristics | |
| Spectral type | K0.5III + F/G[3] |
| B−V color index | 0.855±0.004[2] |
| Astrometry | |
| Radial velocity (Rv) | +2.11±3.42[1] km/s |
| Proper motion (μ) | RA: +3.041±0.182[1] mas/yr Dec.: −54.895±0.169[1] mas/yr |
| Parallax (π) | 12.2045 ± 0.2664[1] mas |
| Distance | 267 ± 6 ly (82 ± 2 pc) |
| Absolute magnitude (MV) | 1.14[4] |
| Details | |
| Mass | 2.4[4] M☉ |
| Radius | 9.8[1] R☉ |
| Luminosity | 35[4] L☉ |
| Surface gravity (log g) | 2.94[4] cgs |
| Temperature | 5,062[4] K |
| Metallicity [Fe/H] | +0.04[4] dex |
| Rotational velocity (v sin i) | 2.7±1.7[5] km/s |
| Age | 557[1] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 169405 (HR 6894), is a suspected binary star[7] system in the southern constellation Telescopium, about a degree to the north of Zeta Telescopii.[8] It has an apparent magnitude of 5.44,[2] making it faintly visible to the naked eye under ideal conditions. HD 169405 is located at a distance of 267 light years[1] and is drifting away with a heliocentric radial velocity of 3.8 km/s.[2]
The visible component has a spectral classification K0.5III[3] which indicates that it is an evolved star between a K0 and K1 giant. It has expanded to ten times the Sun's radius, shines at 35 solar luminosities, and has an effective temperature of 5,062 K.[4] This temperature gives it the yellowish-orange glow of a K-type star, and it spins slowly with a projected rotational velocity of 2.7 km/s.[5]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940 Gaia DR3 record for this source at VizieR.
- ↑ 2.0 2.1 2.2 2.3 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 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 4.3 4.4 4.5 4.6 Ottoni, G.; Udry, S.; Ségransan, D.; Buldgen, G.; Lovis, C.; Eggenberger, P.; Pezzotti, C.; Adibekyan, V. et al. (2022). "CORALIE radial-velocity search for companions around evolved stars (CASCADES). I. Sample definition and first results: Three new planets orbiting giant stars". Astronomy and Astrophysics 657: A87. doi:10.1051/0004-6361/202040078. Bibcode: 2022A&A...657A..87O.
- ↑ 5.0 5.1 De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (2014). "A catalog of rotational and radial velocities for evolved stars". Astronomy & Astrophysics 561: A126. doi:10.1051/0004-6361/201220762. Bibcode: 2014A&A...561A.126D.
- ↑ "HD 169405". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+169405.
- ↑ 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. ISBN 0-933346-84-0.
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