Astronomy:66 Aquarii
Observation data Equinox J2000.0]] (ICRS) | |
---|---|
Constellation | Aquarius |
Right ascension | 22h 43m 35.23307s[1] |
Declination | –18° 49′ 49.3557″[1] |
Apparent magnitude (V) | 4.673[2] |
Characteristics | |
Spectral type | K3 III[3] |
U−B color index | +1.549[2] |
B−V color index | +1.376[2] |
Variable type | suspected[4] |
Astrometry | |
Radial velocity (Rv) | +21.6[5] km/s |
Proper motion (μ) | RA: –31.73[1] mas/yr Dec.: –28.54[1] mas/yr |
Parallax (π) | 7.53 ± 0.26[1] mas |
Distance | 430 ± 10 ly (133 ± 5 pc) |
Absolute magnitude (MV) | −0.93[6] |
Details | |
Radius | 37[7] R☉ |
Luminosity | 434.08[6] L☉ |
Surface gravity (log g) | 2.06[8] cgs |
Temperature | 4,170[8] K |
Metallicity [Fe/H] | –0.23[8] dex |
Rotational velocity (v sin i) | 10[9] km/s |
Other designations | |
Database references | |
SIMBAD | data |
66 Aquarii is a single[11] star in the equatorial constellation of Aquarius. 66 Aquarii is the Flamsteed designation though the star also bears the Bayer designation of g1 Aquarii.[12] It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.673.[2] Based upon an annual parallax shift of 7.53 milliarcseconds,[1] the distance to this star is about 430 light-years (130 parsecs).
This is an evolved giant star with a stellar classification of K3 III.[3] It has expanded to 37 times the radius of the Sun[7] and is radiating 434[6] times the luminosity of the Sun from its outer envelope at an effective temperature of 4,170 K.[8] This gives it the orange-hued glow of a K-type star.[13] It is a suspected variable star that ranges in magnitude between 4.66 and 4.71.[4]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, doi:10.1051/0004-6361:20078357, Bibcode: 2007A&A...474..653V.
- ↑ 2.0 2.1 2.2 2.3 Jennens, P. A.; Helfer, H. L. (September 1975), "A new photometric metal abundance and luminosity calibration for field G and K giants.", Monthly Notices of the Royal Astronomical Society 172 (3): 667–679, doi:10.1093/mnras/172.3.667, Bibcode: 1975MNRAS.172..667J.
- ↑ 3.0 3.1 Houk, Nancy (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, 4, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode: 1988mcts.book.....H.
- ↑ 4.0 4.1 Kazarovets, E. V.; Samus, N. N.; Durlevich, O. V. (December 1998), "New Catalogue of Suspected Variable Stars. Supplement", Information Bulletin on Variable Stars, 1.0 4655: 1, Bibcode: 1998IBVS.4655....1K
- ↑ Wilson, Ralph Elmer (1953), "General catalogue of stellar radial velocities", Carnegie Institute Washington D.C. Publication (Carnegie Institution of Washington), Bibcode: 1953GCRV..C......0W.
- ↑ 6.0 6.1 6.2 Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A.
- ↑ 7.0 7.1 Pasinetti Fracassini, L. E. et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics", Astronomy and Astrophysics 367 (2): 521–524, doi:10.1051/0004-6361:20000451, Bibcode: 2001A&A...367..521P.
- ↑ 8.0 8.1 8.2 8.3 McWilliam, Andrew (December 1990), "High-resolution spectroscopic survey of 671 GK giants. I - Stellar atmosphere parameters and abundances", Astrophysical Journal Supplement Series 74: 1075–1128, doi:10.1086/191527, Bibcode: 1990ApJS...74.1075M.
- ↑ Bernacca, P. L.; Perinotto, M. (1970), "A catalogue of stellar rotational velocities", Contributi Osservatorio Astronomico di Padova in Asiago 239 (1): 1, Bibcode: 1970CoAsi.239....1B.
- ↑ "* g Aqr". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=%2A+g+Aqr.
- ↑ Eggleton, P. P.; Tokovinin, A. A. (2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society 389 (2): 869, doi:10.1111/j.1365-2966.2008.13596.x, Bibcode: 2008MNRAS.389..869E.
- ↑ HD 215167, database record, HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index, N. D. Kostjuk, Institute of Astronomy of Russian Academy of Sciences, 2002; CDS ID IV/27A.
- ↑ "The Colour of Stars", Australia Telescope, Outreach and Education (Commonwealth Scientific and Industrial Research Organisation), December 21, 2004, http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html, retrieved 2012-01-16
External links
Original source: https://en.wikipedia.org/wiki/66 Aquarii.
Read more |