Pi Virginis

Pi Virginis (π Vir, π Virginis) is a binary star in the zodiac constellation of Virgo. It is visible to the naked eye with an apparent visual magnitude of 4.64. The distance to this star, based upon parallax measurements, is roughly 380 light years.

π Virginis
Location of π Virginis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Virgo
Right ascension 12h 00m 52.39042s
Declination +06° 36 51.5571
Apparent magnitude (V) 4.64
Characteristics
Spectral type A5 V
U−B color index +0.12
B−V color index +0.12
Astrometry
Radial velocity (Rv)−10.4 km/s
Proper motion (μ) RA: +0.26 mas/yr
Dec.: −30.10 mas/yr
Parallax (π)8.49 ± 0.39 mas
Distance380 ± 20 ly
(118 ± 5 pc)
Absolute magnitude (MV)−0.70
Orbit
Primaryπ Virginis A
Companionπ Virginis B
Period (P)282.69 days
Semi-major axis (a)3.55 mas
Eccentricity (e)0.265
Inclination (i)62.71°
Longitude of the node (Ω)149.34°
Periastron epoch (T)2448281.3906
Argument of periastron (ω)
(secondary)
312°
Semi-amplitude (K1)
(primary)
26.20 km/s
Details
π Vir A
Mass2.2 M
Radius1.5 R
Surface gravity (log g)3.51 cgs
Temperature8,000 K
Rotational velocity (v sin i)71 km/s
Other designations
BD+07°2502, FK5 1311, HD 104321, HIP 58590, HR 4589, SAO 119164
Database references
SIMBADdata

This is a spectroscopic binary system with a stellar classification of A5V. They have an orbital period of 283 days with an eccentricity of 0.27. The mass ratio of the two stars is about 0.47, with the primary having an estimated mass of around 2.2 times that of the Sun. The primary is a cool metallic-lined Am star.

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