Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Pegasus |
Right ascension | 22h 46m 41.58118s[1] |
Declination | +12° 10′ 22.3854″[1] |
Apparent magnitude (V) | 4.195[2] + 11.70[3] |
Characteristics | |
Spectral type | F6V[4] + M3.5[5] |
U−B color index | −0.015[2] |
B−V color index | +0.502[2] |
Astrometry | |
Radial velocity (Rv) | −5.3[6] km/s |
Proper motion (μ) | RA: +234.18[1] mas/yr Dec.: −493.29[1] mas/yr |
Parallax (π) | 61.36 ± 0.19 mas[1] |
Distance | 53.2 ± 0.2 ly (16.30 ± 0.05 pc) |
Absolute magnitude (MV) | 3.25[7] |
Details | |
Xi Peg A | |
Mass | 1.17[8] M☉ |
Radius | 1.86[8] R☉ |
Luminosity | 4.5[8] L☉ |
Surface gravity (log g) | 3.97±0.07[8] cgs |
Temperature | 6,178±26[8] K |
Metallicity [Fe/H] | −0.27±0.03[8] dex |
Rotational velocity (v sin i) | 12.67[9] km/s |
Age | 5.0±0.5[8] Gyr |
Xi Peg B | |
Mass | 0.32[10] M☉ |
Temperature | 3,569[3] K |
Metallicity [Fe/H] | −0.25[3] dex |
Other designations | |
Database references | |
SIMBAD | data |
Xi Pegasi (ξ Peg, ξ Pegasi) is the Bayer designation for a double star in the northern constellation of Pegasus, the winged horse. Located in the horse's neck, the primary component is an F-type main sequence star that is visible to the naked eye with an apparent visual magnitude of 4.2.[2] It is 86% larger and 17% more massive that the Sun, radiating 4.5 times the solar luminosity.[8] Based upon parallax measurements taken with the Hipparcos spacecraft, it is located 53.2 ± 0.2 light years from the Sun.[1]
The primary has been examined for the presence of an infrared excess that might indicate the presence of a debris disk, but none has been discovered.[12] The common proper motion companion, NLTT 54820, is a twelfth magnitude red dwarf located at an angular separation of 11.4″ along a position angle of 96.9°.[13] This corresponds to a projected physical separation of 192.3 AU.[12]
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