Astronomy:Gliese 829

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Short description: Star system in the constellation Pegasus
Gliese 829
Observation data
Equinox J2000.0]] (ICRS)
Constellation Pegasus[1]
Right ascension  21h 29m 36.81197s[2]
Declination +17° 38′ 35.8655″[2]
Apparent magnitude (V) 10.35[3]
Characteristics
Spectral type M3.0Ve[4]
U−B color index +1.31[3]
B−V color index +1.61[3]
Astrometry
Radial velocity (Rv)−25.0[5] km/s
Proper motion (μ) RA: +1007.040[2] mas/yr
Dec.: +378.400[2] mas/yr
Parallax (π)147.4958 ± 0.0257[2] mas
Distance22.113 ± 0.004 ly
(6.780 ± 0.001 pc)
Absolute magnitude (MV)+11.20[6]
Orbit[7]
Period (P)53.221±0.004 d
Eccentricity (e)0.374±0.004
Periastron epoch (T)48980.2±0.2 JD
Argument of periastron (ω)
(secondary)
300±1°
Semi-amplitude (K1)
(primary)
18.7±0.1 km/s
Semi-amplitude (K2)
(secondary)
18.7±0.1 km/s
Details
Surface gravity (log g)5.0[4] cgs
Temperature3,400[4] K
Metallicity [Fe/H]−0.13[8] dex
Other designations
GJ 829, HIP 106106, G 145-40, G 126-4, LFT 1634, LHS 508, LTT 16285, PLX 5177, Ross 775[9]
Database references
SIMBADdata
ARICNSdata

Gliese 829 is a double-lined spectroscopic binary[7] system of two red dwarf stars in the constellation of Pegasus. They have a high proper motion of 1.08 arc seconds per year along a position angle of +69.58°.[10] Based upon parallax measurements, the stars are at a distance of 22.1 light-years from the Sun.[2] The system will make its closest approach to the Sun around 91,000 years from now when it achieves a perihelion distance of 17.65 ly (5.410 pc).[5]

Characteristics

The primary star has a temperature of 3400 K.[4] It is an M3.0Ve star with a B-V color index of 1.61 and it is also called Ross 775. It has an apparent magnitude of 10.35.[3]

References

  1. Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific 99 (617): 695. doi:10.1086/132034. Bibcode1987PASP...99..695R  Constellation record for this object at VizieR.
  2. 2.0 2.1 2.2 2.3 2.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  3. 3.0 3.1 3.2 3.3 Ianna, P. A.; Whitman, W. R. (April 1984), "Parallaxes and proper motions from the McCormick Observatory List 45", Astronomical Journal 89: 568–570, doi:10.1086/113550, Bibcode1984AJ.....89..568I. 
  4. 4.0 4.1 4.2 4.3 Lépine, Sébastien et al. (2013), "A Spectroscopic Catalog of the Brightest (J < 9) M Dwarfs in the Northern Sky", The Astronomical Journal 145 (4): 102, doi:10.1088/0004-6256/145/4/102, Bibcode2013AJ....145..102L. 
  5. 5.0 5.1 Bailer-Jones, C. A. L. (March 2015), "Close encounters of the stellar kind", Astronomy & Astrophysics 575: 13, doi:10.1051/0004-6361/201425221, A35, Bibcode2015A&A...575A..35B. 
  6. Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode2012AstL...38..331A  XHIP record for this object at VizieR.
  7. 7.0 7.1 Delfosse, Xavier et al. (April 1999), "New neighbours. I. 13 new companions to nearby M dwarfs", Astronomy and Astrophysics 344: 897–910, Bibcode1999A&A...344..897D. 
  8. Rojas-Ayala, Bárbara et al. (April 2012). "Metallicity and Temperature Indicators in M Dwarf K-band Spectra: Testing New and Updated Calibrations with Observations of 133 Solar Neighborhood M Dwarfs". The Astrophysical Journal 748 (2): 93. doi:10.1088/0004-637X/748/2/93. Bibcode2012ApJ...748...93R. http://authors.library.caltech.edu/31363/1/RojasAyala2012p18033Astrophys_J.pdf. Retrieved 2018-09-29. 
  9. "Ross 775". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Ross+775. 
  10. Dawson, P. C.; De Robertis, M. M. (January 2005), "High Proper Motion Stars. IV. Radial Velocities of 166 Luyten Half-Second Stars", The Publications of the Astronomical Society of the Pacific 117 (827): 1–12, doi:10.1086/427790, Bibcode2005PASP..117....1D.