Xi Pegasi

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Xi Pegasi
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[1] mas
Distance 53.2 ± 0.2 ly
(16.30 ± 0.05 pc)
Details
Xi Peg A
Mass 1.17[7] M
Radius 1.86[7] R
Luminosity 4.5[7] L
Surface gravity (log g) 3.97 ± 0.07[7] cgs
Temperature 6,178 ± 26[7] K
Metallicity [Fe/H] −0.27 ± 0.03[7] dex
Rotational velocity (v sin i) 12.67[8] km/s
Age 5.0±0.5[7] Gyr
Xi Peg B
Mass 0.32[9] M
Temperature 3,569[3] K
Metallicity [Fe/H] −0.25[3] dex
Other designations
46 Peg, GJ 872, HD 215648, HIP 112447, HR 8665, SAO 108165.[10]

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.[7] 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.[11] 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°.[12] This corresponds to a projected physical separation of 192.3 AU.[11]

References

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External links

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