HD 170657
From Wikipedia, the free encyclopedia
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Sagittarius |
Right ascension | 18h 31m 18.9597s[1] |
Declination | –18° 54′ 31.722″[1] |
Apparent magnitude (V) | 6.82 |
Characteristics | |
Spectral type | K2V[2] |
U−B color index | +0.56[3] |
B−V color index | +0.87[3] |
Variable type | Suspected[4] |
Astrometry | |
Radial velocity (Rv) | –35[5] km/s |
Proper motion (μ) | RA: –140.14[1] mas/yr Dec.: –194.60[1] mas/yr |
Parallax (π) | 75.71 ± 0.89[1] mas |
Distance | 43.1 ± 0.5 ly (13.2 ± 0.2 pc) |
Details | |
Mass | 0.79 ± 0.11[6] M☉ |
Surface gravity (log g) | 4.61[6] cgs |
Temperature | 5,156[6][7] K |
Rotational velocity (v sin i) | 1.5[6] km/s |
Age | 1.6–6.1[7] Gyr |
Other designations | |
HD 170657 is a star in the constellation Sagittarius. It is located at a distance of about 43 light years. It has 0.79 solar masses and is a suspected variable star that varies in apparent magnitude from 6.82−6.88.[4]
When observed with the Spitzer Space Telescope, this star did not display an excess emission of infrared radiation, which may otherwise indicate the presence of an orbiting debris disk.[7] The space velocity components of this star are (U, V, W) = (–41, –26, +6) km/s.[9]
Sources give contradictory measurements for the abundance of elements in this star. Lawler et al (2009) lists an iron abundance of [Fe/H] = 0.27 dex,[7] while Valenti et al (2005) has an iron abundance of [Fe/H] = –0.15.[6]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 Perryman, M. A. C.; et al. (April 1997). "The HIPPARCOS Catalogue". Astronomy & Astrophysics 323: L49–L52. Bibcode:1997A&A...323L..49P.
- ↑ 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.
- ↑ 3.0 3.1 Corben, P. M.; Carter, B. S.; Banfield, R. M.; Harvey, G. M. (1972). "UBV Photometry of 500 Southern Stars [erratum: 1973MNSSA..32...48C]". Monthly Notes of the Astronomical Society of Southern Africa 31: 7. Bibcode:1972MNSSA..31....7C.
- ↑ 4.0 4.1 Kukarkin, B. V.; et al. (1981). Nachrichtenblatt der Vereinigung der Sternfreunde e.V. (Catalogue of suspected variable stars). Moscow: Academy of Sciences USSR Shternberg. Bibcode:1981NVS...C......0K.
- ↑ Evans, D. S. (June 20–24, 1966). "The Revision of the General Catalogue of Radial Velocities". In Batten, Alan Henry; Heard, John Frederick. Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30. University of Toronto: International Astronomical Union. Retrieved 2009-09-10.
- ↑ 6.0 6.1 6.2 6.3 6.4 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.
- ↑ 7.0 7.1 7.2 7.3 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.
- ↑ "HD 170657 -- Variable Star". Centre de Données astronomiques de Strasbourg. Retrieved 2010-07-21.
- ↑ Gliese, W. (1969). Catalogue of Nearby Stars. Heidelberg: Veröffentlichungen des Astronomischen Rechen-Instituts. Bibcode:1969VeARI..22....1G.
|
|
This article is issued from Wikipedia. The text is available under the Creative Commons Attribution/Share Alike; additional terms may apply for the media files.