Astronomy:31 Leonis
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Leo |
| Right ascension | 10h 07m 54.27057s[1] |
| Declination | +09° 59′ 51.0230″[1] |
| Apparent magnitude (V) | 4.39[2] |
| Characteristics | |
| Spectral type | K3.5 IIIb Fe-1:[3] |
| B−V color index | 1.447[4] |
| Astrometry | |
| Radial velocity (Rv) | +39.84±0.20[5] km/s |
| Proper motion (μ) | RA: −128.69[1] mas/yr Dec.: −113.60[1] mas/yr |
| Parallax (π) | 20.44 ± 1.68[1] mas |
| Distance | 160 ± 10 ly (49 ± 4 pc) |
| Absolute magnitude (MV) | −0.39[2] |
| Details | |
| Radius | 30.40±1.88[6] R☉ |
| Luminosity (bolometric) | 227±31[6] L☉ |
| Surface gravity (log g) | 1.81[6] cgs |
| Temperature | 4,074±8[4] K |
| Metallicity [Fe/H] | −0.02[6] dex |
| Rotational velocity (v sin i) | 5.1[4] km/s |
| Other designations | |
| Database references | |
| SIMBAD | data |
31 Leonis is a binary star[8] system in the equatorial constellation of Leo. The system is visible to the naked eye in unresolved form, having a combined apparent visual magnitude of 4.39.[2] An estimated distance of around 160 light years is obtained from the annual parallax shift of 20.44 mas as seen from Earth's orbit.[1] It is moving away from the Sun with a radial velocity of +39.8 km/s.[5]
The primary member of 31 Leonis, component A, is an evolved K-type red giant[9] with a stellar classification of K3.5 IIIb Fe-1:,[3] where the suffix notation indicates an underabundance of iron in the spectrum. It has expanded to 30[6] times the Solar radius and is radiating around 227[6] times the Sun's luminosity from its photosphere at an effective temperature of 4,074 K.[4] The magnitude 13.6 secondary, component B, lies at an angular separation of 7.9 arcseconds, as of 2008.[8]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, doi:10.1051/0004-6361:20078357, Bibcode: 2007A&A...474..653V.
- ↑ 2.0 2.1 2.2 Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A.
- ↑ 3.0 3.1 Keenan, Philip C; McNeil, Raymond C (1989), "The Perkins catalog of revised MK types for the cooler stars", Astrophysical Journal Supplement Series 71: 245, doi:10.1086/191373, Bibcode: 1989ApJS...71..245K.
- ↑ 4.0 4.1 4.2 4.3 Massarotti, Alessandro et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 Hipparcos Giants and the Role of Binarity", The Astronomical Journal 135 (1): 209–231, doi:10.1088/0004-6256/135/1/209, Bibcode: 2008AJ....135..209M.
- ↑ 5.0 5.1 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.
- ↑ 6.0 6.1 6.2 6.3 6.4 6.5 Piau, L. et al. (February 2011), "Surface convection and red-giant radius measurements", Astronomy and Astrophysics 526: A100, doi:10.1051/0004-6361/201014442, Bibcode: 2011A&A...526A.100P.
- ↑ "31 Leo". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=31+Leo.
- ↑ 8.0 8.1 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.
- ↑ Wood, Brian E. et al. (October 2016), "Hubble Space Telescope Constraints on the Winds and Astrospheres of Red Giant Stars", The Astrophysical Journal 829 (2): 13, doi:10.3847/0004-637X/829/2/74, 74, Bibcode: 2016ApJ...829...74W.
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