Psi8 Aurigae
  | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Auriga[1] |
| Right ascension | 06h 53m 57.073s[2] |
| Declination | +38° 30′ 18.07″[2] |
| Apparent magnitude (V) | 6.46[1] |
| Characteristics | |
| Spectral type | B9.5p[3] |
| Apparent magnitude (J) | 6.471±0.034[4] |
| Apparent magnitude (H) | 6.532±0.036[4] |
| Apparent magnitude (K) | 6.514±0.018[4] |
| B−V color index | −0.044±0.007[1] |
| Variable type | Constant[1] |
| Astrometry | |
| Radial velocity (Rv) | 27.1±1.0[1] km/s |
| Proper motion (μ) | RA: −1.307 mas/yr[2] Dec.: −27.406 mas/yr[2] |
| Parallax (π) | 4.8897±0.0602 mas[2] |
| Distance | 667 ± 8 ly (205 ± 3 pc) |
| Absolute magnitude (MV) | −0.31[1] |
| Details | |
| Mass | 2.0[5] M☉ |
| Radius | 3.1[5] R☉ |
| Luminosity | 100[5] L☉ |
| Surface gravity (log g) | 3.68[5] cgs |
| Temperature | 10,200[5] K |
| Metallicity [Fe/H] | −0.161[6] dex |
| Rotational velocity (v sin i) | 40±9[7] km/s |
| Age | 234[5] Myr |
| Other designations | |
| ψ8 Aurigae, 61 Aurigae, BD+38°1638, HD 50204, HIP 33133, HR 2547, SAO 59589[8] | |
| Database references | |
| SIMBAD | data |
Psi8 Aurigae is a star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ψ8 Aurigae, and abbreviated Psi8 Aur or ψ8 Aur. This star is just visible to the naked eye with an apparent visual magnitude of 6.443. Based upon parallax measurements,[2] it is approximately 667 light-years (205 parsecs) distant from the Earth. It is receding from the Sun with a radial velocity of 27 km/s.[1]
The spectrum of the star has a stellar classification of B9.5p, matching a very late B-type star with unspecified luminosity class. The "p" indicates a peculiarity in the spectrum.[3] φ8 Aurigae has been reported to be an Ap star with unusually string silicon lines in its spectrum, or a mercury-manganese star,[9] but it is now considered doubtful whether it is actually a chemically peculiar star.[10]
This star has double the mass of the Sun and more than triple the Sun's radius. It is an estimated 234[5] million years old and is spinning with a projected rotational velocity of 40 km/s.[7] The star is radiating 100 times the luminosity of the Sun from its photosphere at an effective temperature of 10,200 K.[5]
References
[edit]- ^ a b c d e f g 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. XHIP record for this object at VizieR.
- ^ a b c d e 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.
- ^ a b Cowley, A.; et al. (1969). "A study of the bright stars. I. A catalogue of spectral classifications". The Astronomical Journal. 74: 375–406. Bibcode:1969AJ.....74..375C. doi:10.1086/110819.
- ^ a b c Skrutskie, Michael F.; et al. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. ISSN 0004-6256. S2CID 18913331. Vizier catalog entry
- ^ a b c d e f g h Glagolevskij, Yu. V. (2019). "On Properties of Main Sequence Magnetic Stars". Astrophysical Bulletin. 74 (1): 66. Bibcode:2019AstBu..74...66G. doi:10.1134/S1990341319010073.
- ^ Cardiel, Nicolás; et al. (2021). "RGB photometric calibration of 15 million Gaia stars". Monthly Notices of the Royal Astronomical Society. 507 (1): 318. arXiv:2107.08734. Bibcode:2021MNRAS.507..318C. doi:10.1093/mnras/stab2124.
- ^ a b Abt, Helmut A.; et al. (2002). "Rotational Velocities of B Stars". The Astrophysical Journal. 573 (1): 359–365. Bibcode:2002ApJ...573..359A. doi:10.1086/340590.
- ^ "* psi08 Aur". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2012-08-24.
- ^ Osawa, Kiyoteru (1965). "Spectral classification and three-color photometry of A-type peculiar stars". Annals of the Tokyo Astronomical Observatory. 9 (3): 121. Bibcode:1965AnTok...9..121O.
- ^ Renson, P.; Manfroid, J. (2009). "Catalogue of Ap, HGMN and Am stars". Astronomy and Astrophysics. 498 (3): 961. Bibcode:2009A&A...498..961R. doi:10.1051/0004-6361/200810788.
External links
[edit]- HR 2541 Bright Star Catalog entry
- φ8 Aurigae image
