Alpha Chamaeleontis
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Chamaeleon |
Right ascension | 08h 18m 31.55319s[1] |
Declination | −76° 55′ 10.9964″[1] |
Apparent magnitude (V) | 4.06[2] |
Characteristics | |
Spectral type | F5 V Fe-0.8[3] |
U−B color index | −0.04[2] |
B−V color index | +0.40[2] |
Astrometry | |
Proper motion (μ) | RA: −0.13[1] mas/yr Dec.: +6.89[1] mas/yr |
Parallax (π) | 51.12 ± 0.12 mas[1] |
Distance | 63.8 ± 0.1 ly (19.56 ± 0.05 pc) |
Absolute magnitude (MV) | +2.59[4] |
Details | |
Mass | 1.42[5] M☉ |
Luminosity | 7.64[6] L☉ |
Surface gravity (log g) | 4.28±0.14[5] cgs |
Temperature | 6,776±230[5] K |
Metallicity [Fe/H] | −0.26[3] dex |
Rotational velocity (v sin i) | 0[7] km/s |
Age | 1.8[5] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Alpha Chamaeleontis, Latinized from α Chamaeleontis, is a solitary[9] star in the southern circumpolar constellation of Chamaeleon. It has an apparent visual magnitude of 4.06[2] and thus is bright enough to be seen with the naked eye. With an annual parallax shift of 51.12 mas,[1] it is located 63.8 light years from the Sun.
This is an F-type main sequence star with a stellar classification of F5 V Fe−0.8,[3] where 'Fe−0.8' indicates an anomalously low abundance of iron. It has an estimated 1.4 times the mass of the Sun,[5] and radiates 7.64[6] times the solar luminosity from its outer atmosphere at an effective temperature of 6,776 K.[5] The star is around 1.8[5] billion years old with a projected rotational velocity that is too low to be measured.[7] The star has been examined for an infrared excess that would suggest the presence of an orbiting debris disk, but none was found.[10]
References
- ^ a b c d e f van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357.
- ^ a b c d Mermilliod, J.-C. (1986), Compilation of Eggen's UBV data, transformed to UBV (unpublished), SIMBAD, Bibcode:1986EgUBV........0M.
- ^ a b c Gray, R. O.; et al. (2006), "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample", The Astronomical Journal, 132 (1): 161–70, arXiv:astro-ph/0603770, Bibcode:2006AJ....132..161G, doi:10.1086/504637.
- ^ 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 David, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets", The Astrophysical Journal, 804 (2): 146, arXiv:1501.03154, Bibcode:2015ApJ...804..146D, doi:10.1088/0004-637X/804/2/146.
- ^ a b McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–57, arXiv:1208.2037, Bibcode:2012MNRAS.427..343M, doi:10.1111/j.1365-2966.2012.21873.x.
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: CS1 maint: unflagged free DOI (link) - ^ a b Uesugi, Akira; Fukuda, Ichiro (1970), "Catalogue of rotational velocities of the stars", Contributions from the Institute of Astrophysics and Kwasan Observatory, University of Kyoto, Bibcode:1970crvs.book.....U.
- ^ "alf Cha". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2016-12-10.
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: CS1 maint: postscript (link) - ^ 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.
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: CS1 maint: unflagged free DOI (link) - ^ Gáspár, András; et al. (May 2013), "The Collisional Evolution of Debris Disks", The Astrophysical Journal, 768 (1): 29, arXiv:1211.1415, Bibcode:2013ApJ...768...25G, doi:10.1088/0004-637X/768/1/25, 25.