12 Boötis

12 Boötis is a spectroscopic binary[7] in the constellation Boötes. It is approximately 122 light years from Earth.[1]

12 Boötis
Location of 12 Boötis (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationBoötes
Right ascension14h 10m 23.93342s[1]
Declination25° 05′ 30.0394″[1]
Apparent magnitude (V)4.83[2]
Characteristics
Spectral typeF9IVw[3]
U−B color index+0.07[2]
B−V color index+0.54[2]
Astrometry
Radial velocity (Rv)+9.646±0.013[4] km/s
Proper motion (μ) RA: −23.43[1] mas/yr
Dec.: −59.79[1] mas/yr
Parallax (π)27.917 ± 0.044 mas[4]
Distance116.8 ± 0.2 ly
(35.82 ± 0.06 pc)
Absolute magnitude (MV)2.00[5]
Orbit[4]
Primary12 Boo Aa
Companion12 Boo Ab
Period (P)9.6045601±0.0000036 d
Semi-major axis (a)3.4706±0.0055 mas
Eccentricity (e)0.19214±0.00015
Inclination (i)107.95±0.12°
Longitude of the node (Ω)80.49±0.10°
Periastron epoch (T)2,454,100.43572±0.00070
Argument of periastron (ω)
(secondary)
286.832±0.029°
Semi-amplitude (K1)
(primary)
67.189±0.011 km/s
Semi-amplitude (K2)
(secondary)
69.311±0.014 km/s
Details
12 Boo Aa
Mass1.4109±0.0028[4] M
Radius2.450[6] R
Luminosity7.531 L
Surface gravity (log g)3.73[5] cgs
Temperature6115[6] K
Metallicity [Fe/H]−0.065[4] dex
12 Boo Ab
Mass1.3677±0.0028[4] M
Radius1.901[6] R
Luminosity4.692[6] L
Temperature6200[6] K
Metallicity [Fe/H]−0.065[6] dex
Other designations
d Boötis, 12 Boötis, FK5 522, GC 19127, HIP 69226, HR 5304, HD 123999, GJ 9470, BD+25°2737, SAO 83203, WDS J14104+2506AB, CCDM 14104+2505
Database references
SIMBADdata

12 Boötis is a yellow-white F-type subgiant with an apparent magnitude of +4.82. It is a spectroscopic binary pair which orbit around its centre of mass once every 9.6045 days,[3] with an estimated separation of 0.0035".[8] The two stars have similar masses around 1.4 M, both are slightly hotter than the Sun and about twice as large.[4]

A further companion, 12 Boötis B, was reported with a separation of approximately one arcsecond in 1989, but subsequent surveys have repeatedly failed to detect this companion.[3]

References

See also