Astronomy:Zeta Mensae
Observation data Equinox J2000.0]] (ICRS) | |
---|---|
Constellation | Mensa |
Right ascension | 06h 40m 02.89197s[1] |
Declination | −80° 48′ 48.9391″[1] |
Apparent magnitude (V) | +5.64[2] |
Characteristics | |
Spectral type | A5 III[3][4] |
U−B color index | +0.15[2] |
B−V color index | +0.20[2] |
Astrometry | |
Radial velocity (Rv) | +7.0±7.4[5] km/s |
Proper motion (μ) | RA: −4.801[1] mas/yr Dec.: +53.158[1] mas/yr |
Parallax (π) | 8.2879 ± 0.0870[1] mas |
Distance | 394 ± 4 ly (121 ± 1 pc) |
Absolute magnitude (MV) | +0.09[6] |
Details | |
Radius | 4.65±0.27[1] R☉ |
Luminosity | 66.39±0.86[1] L☉ |
Temperature | 7,555±43[4] K |
Rotational velocity (v sin i) | 200[7] km/s |
Other designations | |
Database references | |
SIMBAD | data |
Zeta Mensae, Latinized from ζ Mensae, is a solitary,[9] white-hued star in the southern constellation of Mensa. It is faintly visible to the naked eye, having an apparent visual magnitude of +5.64.[2] Based upon an annual parallax shift of 8.2879 mas as seen from GAIA, it is located around 394 light years from the Sun.[1] At that distance, the visual magnitude is diminished by an extinction factor of 0.088 due to interstellar dust.[4] Eggen (1995) listed it as a proper motion candidate for membership in the IC 2391 supercluster.[10]
The stellar classification of A5 III[3] suggests this is an A-type giant star. It is spinning rapidly, showing a projected rotational velocity of 200 km/s,[7] giving the star an oblate shape with an equatorial bulge that is an estimated 26% larger than the polar radius.[3] The star is radiating about 69[11] times the Sun's luminosity from its photosphere at an effective temperature of around 7,555 K.[4] It displays a faint infrared excess at a wavelength of 18μm, indicating that it is being orbited by a debris disk.[12]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G. Gaia DR2 record for this source at VizieR.
- ↑ 2.0 2.1 2.2 2.3 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.
- ↑ 3.0 3.1 3.2 Belle, G. T. (2012), "Interferometric observations of rapidly rotating stars", The Astronomy and Astrophysics Review 20 (1): 51, doi:10.1007/s00159-012-0051-2, Bibcode: 2012A&ARv..20...51V.
- ↑ 4.0 4.1 4.2 4.3 Paunzen, E. et al. (October 2006), "An empirical temperature calibration for the Δ a photometric system. II. The A-type and mid F-type stars", Astronomy and Astrophysics 458 (1): 293–296, doi:10.1051/0004-6361:20064889, Bibcode: 2006A&A...458..293P.
- ↑ de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics 546: 14, doi:10.1051/0004-6361/201219219, A61, Bibcode: 2012A&A...546A..61D.
- ↑ 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 Levato, O. H. (August 1972). "Rotational Velocities and Spectral Types of Some A-Type Stars". Publications of the Astronomical Society of the Pacific 84 (500): 584. doi:10.1086/129336. ISSN 0004-6280. Bibcode: 1972PASP...84..584L.
- ↑ "zet Men". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=zet+Men.
- ↑ 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.
- ↑ Eggen, Olin J. (December 1995), "Reality Tests of Superclusters in the Young Disk Population", Astronomical Journal 110: 2862, doi:10.1086/117734, Bibcode: 1995AJ....110.2862E.
- ↑ McDonald, I. et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society 427 (1): 343–57, doi:10.1111/j.1365-2966.2012.21873.x, Bibcode: 2012MNRAS.427..343M.
- ↑ Ishihara, Daisuke et al. (May 2017), "Faint warm debris disks around nearby bright stars explored by AKARI and IRSF", Astronomy & Astrophysics 601: 18, doi:10.1051/0004-6361/201526215, A72, Bibcode: 2017A&A...601A..72I.
Original source: https://en.wikipedia.org/wiki/Zeta Mensae.
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