32 Boötis

Star in the constellation Boötes From Wikipedia, the free encyclopedia

32 Boötis is a single[8] star in the northern constellation of Boötes,[7] located 360 light years away from the Sun.[1] It is visible to the naked eye as a faint, yellow-hued star with an apparent visual magnitude of 5.55.[2] This object is moving closer to the Earth with a heliocentric radial velocity of −23 km/s.[2] It has a relatively high proper motion, traversing the celestial sphere at the rate of 0.195 arc seconds per annum.[9]

Right ascension14h 41m 43.52071s[1]
Declination+11° 39 38.3820[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
32 Boötis
Observation data
Epoch J2000      Equinox J2000
Constellation Boötes
Right ascension 14h 41m 43.52071s[1]
Declination +11° 39 38.3820[1]
Apparent magnitude (V) 5.55[2]
Characteristics
Evolutionary stage red clump[3]
Spectral type G8 III[4]
B−V color index 0.941±0.002[2]
Astrometry
Radial velocity (Rv)−23.3±0.3[2] km/s
Proper motion (μ) RA: −159.787[1] mas/yr
Dec.: −112.732[1] mas/yr
Parallax (π)9.0120±0.2578 mas[1]
Distance360 ± 10 ly
(111 ± 3 pc)
Absolute magnitude (MV)0.09[2]
Details
Mass2.15[5] M
Radius12.06+0.09
−0.24
[1] R
Luminosity79.14±2.57[1] L
Surface gravity (log g)2.6±0.3[3] cgs
Temperature4,957.5+50.0
−17.5
[1] K
Metallicity [Fe/H]−23.3±0.3[2] dex
Rotational velocity (v sin i)2.6[6] km/s
Age1.46[5] Gyr
Other designations
32 Boo, BD+12°2729, FK5 1382, HD 129336, HIP 71837, HR 5481, SAO 120601, LTT 14344[7]
Database references
SIMBADdata
Close

This is an aging giant star with a stellar classification of G8 III.[4] It is most likely on the horizontal branch and is a candidate red clump giant.[3] The star is an estimated 1.46[5] billion years old with 2.15[5] times the mass of the Sun. With the hydrogen at its core exhausted, it has expanded to 12[1] times the Sun's radius. 32 Boötis is radiating 79[1] times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4958 K.[1]

References

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