40 Boötis

Star in the constellation Boötes From Wikipedia, the free encyclopedia

40 Boötis is a single[8] star located 166.5 light years away from the Sun in the northern constellation of Boötes. It is visible to the naked eye as a dim, yellow-white hued star with an apparent visual magnitude of 5.64.[2] The star is moving away from the Earth with a heliocentric radial velocity of +12 km/s.[5]

Right ascension14h 59m 36.94745s[1]
Declination+39° 15 55.1994[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
40 Boötis
Observation data
Epoch J2000      Equinox J2000
Constellation Boötes
Right ascension 14h 59m 36.94745s[1]
Declination +39° 15 55.1994[1]
Apparent magnitude (V) 5.64[2]
Characteristics
Evolutionary stage giant[3]
Spectral type F1 III–IV[4]
B−V color index 0.336±0.004[2]
Astrometry
Radial velocity (Rv)+12.3±0.7[5] km/s
Proper motion (μ) RA: −32.109[1] mas/yr
Dec.: 41.246[1] mas/yr
Parallax (π)19.5911±0.0702 mas[1]
Distance166.5 ± 0.6 ly
(51.0 ± 0.2 pc)
Absolute magnitude (MV)2.08[2]
Details
Mass1.47[6] M
Radius2.35+0.34
−0.13
[1] R
Luminosity11.585±0.054[1] L
Surface gravity (log g)3.88[6] cgs
Temperature7,070±240[6] K
Metallicity [Fe/H]−0.29[5] dex
Rotational velocity (v sin i)72.5[3] km/s
Age1.166[6] Gyr
Other designations
40 Boo, BD+39°2820, FK5 3182, HD 132772, HIP 73369, HR 5588, SAO 64449[7]
Database references
SIMBADdata
Close

The Hipparcos catalogue (1997) lists a stellar classification of F1 III–IV,[9] matching the luminosity class of an aging star that is evolving into a giant.[3] Earlier, Cowley and Bidelman (1979) listed a class of F2 III,[10] while Sato and Kuji (1990) found a main sequence class of F0V.[11] It is around 1.2[6] billion years old with a relatively high rotation rate, showing a projected rotational velocity of 72.5 km/s.[3] The star has 1.5[6] times the mass of the Sun and 2.4[1] times the Sun's radius. It is radiating 11.6[1] times the luminosity of the Sun from its photosphere at an effective temperature of 7,070 K.[6]

References

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