Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Pegasus |
Right ascension | 21h 29m 36.81225s[1] |
Declination | +17° 38′ 35.8542″[1] |
Apparent magnitude (V) | 10.35[2] |
Characteristics | |
Spectral type | M3.0Ve[3] |
U−B color index | +1.31[2] |
B−V color index | +1.61[2] |
Astrometry | |
Radial velocity (Rv) | −25.0[4] km/s |
Proper motion (μ) | RA: +1007.13[1] mas/yr Dec.: +377.27[1] mas/yr |
Parallax (π) | 147.4958 ± 0.0257 mas[5] |
Distance | 22.113 ± 0.004 ly (6.780 ± 0.001 pc) |
Orbit[6] | |
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[3] cgs |
Temperature | 3,400[3] K |
Metallicity [Fe/H] | −0.13[7] dex |
Other designations | |
Database references | |
SIMBAD | data |
ARICNS | data |
Gliese 829 is a double-lined spectroscopic binary[6] 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°.[9] Based upon parallax measurements, the stars are at a distance of about 22 light years from the Sun.[1] 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).[4]
vanLeeuwen2007
was invoked but never defined (see the help page).Ianna1984
was invoked but never defined (see the help page).lepine2013
was invoked but never defined (see the help page).Bailer-Jones2015
was invoked but never defined (see the help page).Delfosse1999
was invoked but never defined (see the help page).RojasAyala2012
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).Dawson2005
was invoked but never defined (see the help page).