HD 177830

HD 177830
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Lyra
Right ascension 19h 05m 20.7732s
Declination +25° 55 14.373
Apparent magnitude (V) 7.175
Characteristics
A
Evolutionary stage subgiant or giant
Spectral type K2IV
B
Evolutionary stage main sequence
Spectral type M4V
Astrometry
Radial velocity (Rv)−71.86±0.06 km/s
Proper motion (μ) RA: −41.248(12) mas/yr
Dec.: −52.580(17) mas/yr
Parallax (π)16.0063±0.0165 mas
Distance203.8 ± 0.2 ly
(62.48 ± 0.06 pc)
Absolute magnitude (MV)+3.33
Orbit
Period (P)~800 yr
Semi-major axis (a)97 au
Details
A
Mass1.48 M
Radius3.6 R
Luminosity6.3 L
Surface gravity (log g)3.43 cgs
Temperature4,824 K
Metallicity [Fe/H]0.31 dex
Rotational velocity (v sin i)2.54 km/s
Age4.4±2.2 Gyr
B
Mass0.23 M
Other designations
BD+25°3719, Gliese 743.2, HIP 93746, GSC 02126-01196, SAO 86791
Database references
SIMBADdata

HD 177830 is a 7th magnitude binary star system located approximately 205 light-years away in the constellation of Lyra. The primary star is slightly more massive than the Sun, but cooler being a type K star. It has evolved away from the main sequence and expanded to 3.6 times the radius of the Sun. In visual light it is over six times brighter than the Sun, but because of its distance, about 204 light years, it is not visible to the unaided eye. With binoculars it is be easily visible.

The primary star is known to have two extrasolar planets orbiting around it.