Observation data Epoch J2000 Equinox J2000 | |
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Constellation | Ara |
Right ascension | 17 10 10.35091 |
Declination | −60° 43′ 43.5757″ |
Apparent magnitude (V) | 7.385 |
Characteristics | |
Spectral type | K2.5Vk: |
U−B color index | +0.53 |
B−V color index | +0.89 |
Astrometry | |
Radial velocity (Rv) | +8.8 km/s |
Proper motion (μ) | RA: 70.96 mas/yr Dec.: 589.86 mas/yr |
Parallax (π) | 73.41 ± 0.70 mas |
Distance | 44.4 ± 0.4 ly (13.6 ± 0.1 pc) |
Absolute magnitude (MV) | 6.71 |
Details | |
Mass | 0.68 M☉ |
Radius | 0.68 R☉ |
Luminosity | 0.24 L☉ |
Surface gravity (log g) | 4.70 cgs |
Temperature | 4,850 K |
Metallicity | −0.70 dex |
Rotational velocity (v sin i) | 0.2 km/s |
Age | 3.2 Gyr |
Other designations | |
CD-60 6576, GCTP, GJ 656, HD 154577, HIP 83990, LHS 3268, LTT 6833, SAO 253819. | |
Database references | |
SIMBAD | data |
ARICNS | data |
HD 154577 (Gliese 656) is a solar-type star in the southern constellation of Ara. It is a high proper motion star and, based upon an annual parallax shift of 73.41 mas, is located about 44 light years from the Sun. The star is too faint to be readily visible to the naked eye, having an apparent visual magnitude of 7.4. It is moving away from the Sun with a radial velocity of +9 km/s.
This star has only 68% of the Sun's mass and radius, an effective temperature of 4,850 K and a stellar classification of K2.5Vk:, which indicates it is a K-type main sequence star. (The 'k' suffix indicates there are interstellar absorption features in the spectra, while ':' means there is some uncertainty about the classification.) It is about 3.2 billion years old and appears to be spinning slowly with a projected rotational velocity of 0.2 km/s. The star is radiating 24% of the Sun's luminosity from its photosphere at an effective temperature of 4,850 K.
As of 2005, this star is not known to host any planets. No excess of infrared radiation has been detected of the type that would indicate the presence of an orbiting debris disk.
References
- ^ van Leeuwen, F. (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.
- ^ Holmberg, J.; Nordström, B.; Andersen, J. (July 2009). "The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics". Astronomy and Astrophysics Supplement Series. 501 (3): 941–947. arXiv:0811.3982. Bibcode:2009A&A...501..941H. doi:10.1051/0004-6361/200811191. S2CID 118577511. Note: see VizieR catalogue V/130.
- ^ Gray, R. O.; et al. (July 2006). "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 pc-The Southern Sample". The Astronomical Journal. 132 (1): 161–170. arXiv:astro-ph/0603770. Bibcode:2006AJ....132..161G. doi:10.1086/504637. S2CID 119476992.
- ^ Cousins, A. W. J. (1973). "UBV photometry of some southern stars". Monthly Notes of the Astronomical Society of Southern Africa. 32: 11. Bibcode:1973MNSSA..32...11C.
- ^ Evans, D. S. (June 20–24, 1966). "The Revision of the General Catalogue of Radial Velocities". In Batten, Alan Henry; Heard, John Frederick (eds.). Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30. University of Toronto: International Astronomical Union. Bibcode:1967IAUS...30...57E.
- ^ Santos, N. C.; et al. (July 2005). "Spectroscopic metallicities for planet-host stars: Extending the samples". Astronomy and Astrophysics. 437 (3): 1127–1133. arXiv:astro-ph/0504154. Bibcode:2005A&A...437.1127S. doi:10.1051/0004-6361:20052895. S2CID 16256304.
- Takeda, Genya; et al. (February 2007), "Structure and Evolution of Nearby Stars with Planets. II. Physical Properties of ~1000 Cool Stars from the SPOCS Catalog", The Astrophysical Journal Supplement Series, 168 (2): 297–318, arXiv:astro-ph/0607235, Bibcode:2007ApJS..168..297T, doi:10.1086/509763, S2CID 18775378.
- ^ 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, S2CID 119257644.
- Adibekyan, V. Zh.; et al. (September 2012), "Chemical abundances of 1111 FGK stars from the HARPS GTO planet search program. Galactic stellar populations and planets", Astronomy & Astrophysics, 545: 15, arXiv:1207.2388, Bibcode:2012A&A...545A..32A, doi:10.1051/0004-6361/201219401, S2CID 118300756, A32.
- ^ Valenti, Jeff A.; Fischer, Debra A. (July 2005), "Spectroscopic Properties of Cool Stars (SPOCS). I. 1040 F, G, and K Dwarfs from Keck, Lick, and AAT Planet Search Programs", The Astrophysical Journal Supplement Series, 159 (1): 141–166, Bibcode:2005ApJS..159..141V, doi:10.1086/430500.
- ^ Lawler, S. M.; et al. (November 2009). "Explorations Beyond the Snow Line: Spitzer/IRS Spectra of Debris Disks Around Solar-type Stars". The Astrophysical Journal. 705 (1): 89–111. arXiv:0909.0058. Bibcode:2009ApJ...705...89L. doi:10.1088/0004-637X/705/1/89. S2CID 1272803.
- "LHS 3268 -- High proper-motion star". SIMBAD. Centre de Données astronomiques de Strasbourg. Retrieved 2010-12-06.
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