HD 211392
Appearance
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aquarius[1] |
Right ascension | 22h 16m 52.56734s[2] |
Declination | −09° 02′ 24.1971″[2] |
Apparent magnitude (V) | 5.96[3] |
Characteristics | |
Spectral type | K3III[3] |
U−B color index | +1.14[4] |
B−V color index | +1.16[4] |
Astrometry | |
Radial velocity (Rv) | 12.1[5] km/s |
Proper motion (μ) | RA: −57.013[2] mas/yr Dec.: −10.167[2] mas/yr |
Parallax (π) | 9.4163±0.0629 mas[2] |
Distance | 346 ± 2 ly (106.2 ± 0.7 pc) |
Absolute magnitude (MV) | +0.54[1] |
Details | |
Mass | 1.5[6] M☉ |
Radius | 13[2] R☉ |
Luminosity | 69[6] L☉ |
Surface gravity (log g) | 2.11[7] cgs |
Temperature | 4,540[6] K |
Metallicity [Fe/H] | 0.01[7] dex |
Age | 3.1[2] Gyr |
Other designations | |
BD−09°5948, HD 211392, HIP 110009, HR 8500, SAO 145992 | |
Database references | |
SIMBAD | data |
Data sources: | |
Hipparcos Catalogue, CCDM (2002), Bright Star Catalogue (5th rev. ed.) |
HD 211392 is a suspected[8] variable star in the equatorial constellation of Aquarius, positioned about 346 light-years away.[2] With an apparent magnitude close to six, according to the Bortle scale it is just visible to the naked eye from dark, rural skies. It is a giant star with a stellar classification of K3III.[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.
- ^ a b c d e f g h 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 c 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, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976
- ^ a b Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory, 4 (99): 99, Bibcode:1966CoLPL...4...99J
- ^ Wilson, R. E. (1953), "General Catalogue of Stellar Radial Velocities", Carnegie Institute Washington D.C. Publication, Carnegie Institute of Washington D.C., Bibcode:1953GCRV..C......0W
- ^ a b c Charbonnel, C.; Lagarde, N.; Jasniewicz, G.; North, P. L.; Shetrone, M.; Krugler Hollek, J.; Smith, V. V.; Smiljanic, R.; Palacios, A.; Ottoni, G. (2020). "Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era". Astronomy and Astrophysics. 633: A34. arXiv:1910.12732. Bibcode:2020A&A...633A..34C. doi:10.1051/0004-6361/201936360.
- ^ a b Soubiran, C.; Brouillet, N.; Casamiquela, L. (2022). "Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys". Astronomy and Astrophysics. 663: A4. arXiv:2112.07545. Bibcode:2022A&A...663A...4S. doi:10.1051/0004-6361/202142409.
- ^ Kukarkin, B. V.; et al. (1981), "Nachrichtenblatt der Vereinigung der Sternfreunde e.V. (Catalogue of suspected variable stars)", Nachrichtenblatt der Vereinigung der Sternfreunde E.V. (1981), Moscow: Academy of Sciences USSR Shternberg, Bibcode:1981NVS...C......0K