Zeta1 Antliae
 | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Antlia |
| Right ascension | 09h 30m 46.09678s[1] |
| Declination | –31° 53′ 21.1911″[1] |
| Apparent magnitude (V) | 5.76[2] (6.20/7.01)[3] |
| Characteristics | |
| Spectral type | A0 V + A2 V[3] |
| U−B color index | +0.05[2] |
| B−V color index | +0.05[2] |
| Astrometry | |
| Proper motion (μ) | RA: +22.31[1] mas/yr Dec.: –20.12[1] mas/yr |
| Parallax (π) | 8.04 ± 0.72 mas[1] |
| Distance | 410 ± 40 ly (120 ± 10 pc) |
| Details | |
| zet1 Ant A | |
| Rotational velocity (v sin i) | 204[4] km/s |
| zet1 Ant B | |
| Rotational velocity (v sin i) | 50[4] km/s |
| Other designations | |
| zet1 Ant A: GC 13137, HD 82384, HR 3781, SAO 200445. | |
| zet1 Ant B: GC 13135, HD 82383, HR 3780, SAO 200444 | |
| Database references | |
| SIMBAD | data |
| Database references | |
| SIMBAD | data |
Zeta1 Antliae is the Bayer designation for a binary star[3] system in the southern constellation of Antlia. Based upon parallax measurements, the pair are located at a distance of roughly 410 light-years (130 parsecs) from Earth.[1] Both components are rapidly rotating[4] A-type main sequence stars.[3] They have apparent magnitudes of +6.20 and 7.01 and are separated by 8.042 arcseconds.[3] The apparent magnitude of the combined system is +5.76,[2] which is bright enough to be seen with the naked eye in suitably dark skies.
References
- ^ a b c d e f van Leeuwen, F. (November 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 Hurly, P. R. (1975), "Combined-light UBV Photometry of 103 Bright Southern Visual Doubles", Monthly Notes of the Astronomical Society of Southern Africa, 34: 7, Bibcode:1975MNSSA..34....7H.
- ^ a b c d e 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.
{{citation}}: CS1 maint: unflagged free DOI (link) - ^ a b c Royer, F.; et al. (January 2012), "Rotational velocities of A-type stars. I. Measurement of v sin i in the southern hemisphere", Astronomy and Astrophysics, 381: 105–121, arXiv:astro-ph/0110490, Bibcode:2002A&A...381..105R, doi:10.1051/0004-6361:20011422.
- ^ "IDS 09265-3127 AB -- Double or multiple star", SIMBAD Astronomical Object Database, Centre de Données astronomiques de Strasbourg, retrieved 2012-06-27.
 | This binary or multiple star system-related article is a stub. You can help Wikipedia by expanding it. |