HD 92209
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Chamaeleon[1] |
| Right ascension | 10h 35m 24.7604s[2] |
| Declination | −76° 18′ 32.337″[2] |
| Apparent magnitude (V) | 6.29±0.01[3] |
| Characteristics | |
| Spectral type | K2 III[4] |
| U−B color index | +1.27[5] |
| B−V color index | +1.20[5] |
| Astrometry | |
| Radial velocity (Rv) | 17.8±2.3[6] km/s |
| Proper motion (μ) | RA: −16.952 mas/yr[2] Dec.: +6.489 mas/yr[2] |
| Parallax (π) | 5.4324±0.1144 mas[2] |
| Distance | 600 ± 10 ly (184 ± 4 pc) |
| Absolute magnitude (MV) | +0.53[1] |
| Details | |
| Mass | 1.22[7] M☉ |
| Radius | 14.39[8] R☉ |
| Luminosity | 81.3+9.9 −8.8[9] L☉ |
| Surface gravity (log g) | 1.76[7] cgs |
| Temperature | 4,460±90[9] K |
| Metallicity [Fe/H] | +0.06[10] dex |
| Rotational velocity (v sin i) | <1[11] km/s |
| Other designations | |
| 22 G. Chamaeleontis, CPD−75°678, FK5 2847, GC 14595, HD 92209, HIP 51835, HR 4170, SAO 256730[12][13] | |
| Database references | |
| SIMBAD | data |
HD 92209 (HR 4170) is a probable spectroscopic binary[11] in the southern circumpolar constellation Chamaeleon. It has an apparent magnitude of 6.29,[3] placing it near the max naked eye visibility. Parallax measurements place the system at a distance of 600 light years[2] and is currently receding with a heliocentric radial velocity of almost 18 km/s.[6]
The visible component has a stellar classification of K2 III,[4] indicating that it is a red giant. As a consequence, it has expanded to 14.39 times the radius of the Sun.[8] Nevertheless, it has 122% the mass of the Sun[7] and shines with a luminosity of 81.3 L☉,[9] yielding an effective temperature of 4,460 K[9] from its enlarged photosphere, which in turn gives an orange hue. HD 92209 has a metallicity 115% that of the Sun[10] and spins leisurely with a projected rotational velocity lower than 1 km/s.[11]
References
- ^ 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. XHIP record for this object at VizieR.
- ^ a b c d e Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ^ a b Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30. Bibcode:2000A&A...355L..27H. ISSN 0004-6361.
- ^ a b Houk, N.; Cowley, A. P. (1975). University of Michigan Catalogue of two-dimensional spectral types for the HD stars. Volume I. Declinations -90_ to -53_ƒ0. Bibcode:1975mcts.book.....H.
- ^ a b Johnson, H. L.; Mitchell, R. I.; Iriarte, B.; Wisniewski, W. Z. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory. 4: 99–110. Bibcode:1966CoLPL...4...99J.
- ^ a b Gontcharov, G. A. (November 2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. ISSN 1063-7737. S2CID 119231169.
- ^ a b c Anders, F.; et al. (August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy & Astrophysics. 628: A94. arXiv:1904.11302. Bibcode:2019A&A...628A..94A. doi:10.1051/0004-6361/201935765. ISSN 0004-6361.
- ^ a b Kervella, Pierre; Arenou, Frédéric; Thévenin, Frédéric (2022). "Stellar and substellar companions from Gaia EDR3". Astronomy & Astrophysics. 657: A7. arXiv:2109.10912. Bibcode:2022A&A...657A...7K. doi:10.1051/0004-6361/202142146. eISSN 1432-0746. ISSN 0004-6361.
- ^ a b c d Charbonnel, C.; Lagarde, N.; Jasniewicz, G.; North, P. L.; Shetrone, M.; Krugler Hollek, J.; Smith, V. V.; Smiljanic, R.; Palacios, A.; Ottoni, G. (January 2020). "Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era". Astronomy & Astrophysics. 633: A34. arXiv:1910.12732. Bibcode:2020A&A...633A..34C. doi:10.1051/0004-6361/201936360. eISSN 1432-0746. ISSN 0004-6361.
- ^ a b Eggen, O. J. (February 1994). "Evolved GK stars near the Sun. 2: The young disk population". The Astronomical Journal. 107: 594. Bibcode:1994AJ....107..594E. doi:10.1086/116879. ISSN 0004-6256.
- ^ a b c De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (January 2014). "A catalog of rotational and radial velocities for evolved stars: V. Southern stars". Astronomy & Astrophysics. 561: A126. arXiv:1312.3474. Bibcode:2014A&A...561A.126D. doi:10.1051/0004-6361/201220762. ISSN 0004-6361.
- ^ "HD 92209". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved June 13, 2022.
- ^ Gould, Benjamin Apthorp (1878). "Uranometria Argentina : brillantez y posicion de las estrellas fijas, hasta la septima magnitud, comprendidas dentro de cien grados del polo austral : con atlas". Resultados del Observatorio Nacional Argentino. 1. Bibcode:1879RNAO....1.....G.