38 Boötis

38 Boötis
Observation data
Epoch J2000      Equinox J2000
Constellation Boötes
Right ascension 14h 49m 18.67062s
Declination +46° 06 58.3369
Apparent magnitude (V) 5.76
Characteristics
Evolutionary stage subgiant
Spectral type F6 IVs
B−V color index 0.482±0.002
Astrometry
Radial velocity (Rv)−4.5±0.2 km/s
Proper motion (μ) RA: –6.404 mas/yr
Dec.: −78.073 mas/yr
Parallax (π)20.7166±0.0638 mas
Distance157.4 ± 0.5 ly
(48.3 ± 0.1 pc)
Absolute magnitude (MV)2.31
Details
Mass1.60±0.04 M
Radius2.51+0.04
−0.08
 R
Luminosity9.511±0.039 L
Surface gravity (log g)3.92±0.02 cgs
Temperature6,591±63 K
Metallicity [Fe/H]0.11±0.05 dex
Rotational velocity (v sin i)9.8 km/s
Age1.74+0.19
−0.10
 Gyr
Other designations
Merga, Marrha, El Mara el Musalsela, Falx Italica, h Boötis, 38 Boo, BD+46°1993, FK5 1383, GC 19959, HD 130945, HIP 72487, HR 5533, SAO 45226
Database references
SIMBADdata

38 Boötis is a single star in the northern constellation of Boötes, located approximately 157 light years from the Sun. It has the traditional name Merga /ˈmɜːrɡə/ and the Bayer designation h Boötis; 38 Boötis is the star's Flamsteed designation. This object is visible to the naked eye as a dim, yellow-white hued star with an apparent visual magnitude of 5.76. It is moving closer to the Earth with a heliocentric radial velocity of −4.5 km/s.

This is a sharp-lined ('s') subgiant star with a stellar classification of F6 IVs, which indicates it has consumed the hydrogen at its core and is evolving off the main sequence. It is about 1.7 billion years old and is spinning with a relatively low projected rotational velocity of 10 km/s, as indicated by the sharp lines. The star has 1.6 times the mass of the Sun and 2.5 times the Sun's radius. It is radiating 9.5 times the luminosity of the Sun from its photosphere at an effective temperature of 6,591 K.