45 Boötis

Single star in the constellation Boötes From Wikipedia, the free encyclopedia

45 Boötis is a single[6][7] star located 63 light years away from the Sun in the northern constellation of Boötes. It has the Bayer designation c Boötis; 45 Boötis is the Flamsteed designation. This body is visible to the naked eye as a faint, yellow-white hued star with an apparent visual magnitude of 4.93.[2] It has a relatively high proper motion, traversing the celestial sphere at the rate of 0.247 per year.[8] The star is moving closer to the Earth with a heliocentric radial velocity of −11 km/s,[2] and is a stream member of the Ursa Major Moving Group.[9]

Quick Facts Observation data Epoch J2000 Equinox J2000, Constellation ...
45 Boötis
Observation data
Epoch J2000      Equinox J2000
Constellation Boötes
Right ascension 15h 07m 18.06587s[1]
Declination +24° 52 09.0952[1]
Apparent magnitude (V) 4.93[2]
Characteristics
Spectral type F5 V[3]
B−V color index +0.43[3]
Astrometry
Radial velocity (Rv)−11.2[2] km/s
Proper motion (μ) RA: +184.767[1] mas/yr
Dec.: −164.012[1] mas/yr
Parallax (π)51.6674 ± 0.1882 mas[1]
Distance63.1 ± 0.2 ly
(19.35 ± 0.07 pc)
Absolute magnitude (MV)3.96[4]
Details[2]
Mass1.21±0.16 M
Radius1.461±0.027 R
Luminosity3.30+0.25
−0.22
 L
Surface gravity (log g)4.19 cgs
Temperature6,435 K
Metallicity [Fe/H]−0.02 dex
Rotational velocity (v sin i)39.8 km/s
Age1.6+0.8
−0.6
 Gyr
Other designations
c Boo, 45 Boo, NSV 6945, BD+25°2873, FK5 1396, GJ 578, HD 134083, HIP 73996, HR 5634, SAO 83671, WDS J15073+2452[5]
Database references
SIMBADdata
Close

This is an F-type main-sequence star with a stellar classification of F5 V.[3] It is around 1.6 billion years old and is spinning with a projected rotational velocity of 40 km/s. The star has 1.2 times the mass of the Sun and 1.46 times the Sun's radius. It is radiating 3.3 times the luminosity of the Sun from its photosphere at an effective temperature of 6,435 K.[2] 45 Boötis is a source of X-ray emission.[10]

There is a magnitude 11.53 visual companion at an angular separation of 103.50 along a position angle (PA) of 40°, as of 2012. A magnitude 10.23 star can be found at a separation of 247.90″ with a PA of 358°, as of 2015.[11]

References

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