34 Boötis

34 Boötis

File:WBooLightCurve.png The visual band light curve of W Boötes, adapted from Percy et al. (1997)
Observation data Epoch J2000      Equinox J2000
Constellation	Boötes
Right ascension	Template:RA
Declination	Template:DEC
Apparent magnitude (V)	4.80 (4.49 - 5.40)
Characteristics
Spectral type	M3− III
B−V Template:Engvar
Variable type	Semi-regular
Astrometry
Radial velocity (Rv)	km/s
Proper motion (μ)	RA: –13.57 mas/yr Dec.: −16.08 mas/yr
Parallax (π)	4.63±0.28 mas
Distance	Template:Rnd ± Template:Rnd ly (Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)	−1.86
Details
Mass	Template:Solar mass
Radius	Template:Solar radius
Luminosity	Template:Solar luminosity
Surface gravity (log g)	1.24 cgs
Temperature	K
Age	Gyr
Metallicity [Fe/H]	{{{metal_fe2}}} dex
Other designations
Template:Odlist
Database references
SIMBAD	data

34 Boötis is a single variable star in the northern constellation Boötes, located around 700 light years away from the Sun. At that distance, the visual magnitude of the star is diminished by an extinction of due to interstellar dust. It has the variable star designation W Boötis; 34 Boötis is the Flamsteed designation. This object is visible to the naked eye as a faint, red-hued star with a baseline apparent visual magnitude of 4.80. It is moving away from the Earth with a heliocentric radial velocity of +5.6 km/s.

This is an aging red giant star with a stellar classification of M3− III, which indicates it has exhausted the supply of hydrogen at its core and evolved off the main sequence branch. It is classified as a semiregular variable with a brightness that varies from magnitude +4.49 down to +5.4 with a period of 25 days, with some evidence of longer term variation and mode switching. The star is around a billion years old with 2.2 times the mass of the Sun and has expanded to 129 times the size of the Sun. It is radiating 2,802 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 3,691 K.

The parallax calculated in the new Hipparcos reduction is , and in Gaia Data Release 2 the parallax is given as . Each has a margin of error of about 5%, but they differ from each other by far more than 5%.