6 Equulei
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Equuleus |
| Right ascension | 21h 10m 31.31410s[1] |
| Declination | 10° 02′ 56.1112″[1] |
| Apparent magnitude (V) | 6.07[2] |
| Characteristics | |
| Evolutionary stage | main sequence[3][4] |
| Spectral type | A2 Vs[3] (A1 Si Sr Cr)[5] |
| U−B color index | +0.04[2] |
| B−V color index | +0.02[2] |
| Astrometry | |
| Radial velocity (Rv) | +6.9[6] km/s |
| Proper motion (μ) | RA: –0.982 mas/yr[4] Dec.: +17.687 mas/yr[4] |
| Parallax (π) | 7.36±0.81 mas[1] |
| Distance | approx. 440 ly (approx. 140 pc) |
| Absolute magnitude (MV) | +0.236[7] |
| Details | |
| Mass | 2.412+0.045 −0.047[4] M☉ |
| Radius | 2.68±0.08[4] R☉ |
| Luminosity | 48.7+1.9 −2.0[4] L☉ |
| Surface gravity (log g) | 3.738+0.006 −0.019[4] cgs |
| Temperature | 9,339+32 −118[4] K |
| Rotational velocity (v sin i) | 65[3] km/s |
| Age | 462+75 −71[4] Myr |
| Other designations | |
| BD+09°4735, HD 201616, HIP 104538, HR 8098, SAO 126597[8] | |
| Database references | |
| SIMBAD | data |
6 Equulei is a probable (95% chance) astrometric binary[9] star system in the northern constellation of Equuleus, located 440 light years away.[1] It is barely visible to the naked eye as a dim, white-hued star with an apparent visual magnitude of 6.07.[2] The system is moving further away from the Earth with a heliocentric radial velocity of +6.9 km/s.[6] It forms a wide optical double with γ Equulei, at an angular separation of 336 arcseconds in 2011.[10]
The visible component is an Ap star[3] with a stellar classification of A2Vs,[3] matching the evolutionary state of an A-type main sequence star while displaying "sharp" absorption lines. It is an estimated 460 million years old[4] with a projected rotational velocity of 65 km/s.[3] The star has 2.4 times the mass of the Sun and around 2.7 times the Sun's radius. It is radiating 49 times the luminosity of the Sun from its photosphere at an effective temperature of 9,339 K.[4]
References
- ^ a b c d 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, S2CID 18759600.
- ^ a b c d 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
- ^ a b c d e f Zorec, J.; et al. (2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy and Astrophysics, 537: A120, arXiv:1201.2052, Bibcode:2012A&A...537A.120Z, doi:10.1051/0004-6361/201117691, S2CID 55586789.
- ^ a b c d e f g h i j 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.
- ^ Renson, P.; Manfroid, J. (May 2009), "Catalogue of Ap, HgMn and Am stars", Astronomy and Astrophysics, 498 (3): 961–966, Bibcode:2009A&A...498..961R, doi:10.1051/0004-6361/200810788.
- ^ a b Wilson, Ralph Elmer (1953), "General Catalogue of Stellar Radial Velocities", Carnegie Institute Washington D.C. Publication, Washington: Carnegie Institution of Washington, Bibcode:1953GCRV..C......0W.
- ^ "HD 104538", WolframAlpha, retrieved 2012-08-05
- ^ "6 Equ -- Star in double system", SIMBAD Astronomical Database, Centre de Données astronomiques de Strasbourg, retrieved 2012-07-25.
- ^ Frankowski, A.; Jancart, S.; Jorissen, A. (March 2007), "Proper-motion binaries in the Hipparcos catalogue. Comparison with radial velocity data", Astronomy and Astrophysics, 464 (1): 377–392, arXiv:astro-ph/0612449, Bibcode:2007A&A...464..377F, doi:10.1051/0004-6361:20065526, S2CID 14010423
- ^ Mason, Brian D.; et al. (2001), "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog", The Astronomical Journal, 122 (6): 3466–3471, Bibcode:2001AJ....122.3466M, doi:10.1086/323920.