Nu Virginis

ν Virginis, Latinized as Nu Virginis, is a single star in the zodiac constellation of Virgo, located at the western tip of the classic constellation and nearly due south of the prominent star Denebola. It is a red-hued star with an apparent visual magnitude of 4.04 and can be seen with the naked eye. Because the star lies near the ecliptic it is subject to occultations by the Moon. Parallax measurements provide an estimated distance of around 294 light years from the Sun, and it is drifting further away with a radial velocity of +50 km/s.

ν Virginis
Location of ν Virginis (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Virgo
Right ascension 11h 45m 51.55957s
Declination +06° 31 45.7413
Apparent magnitude (V) 4.04
Characteristics
Evolutionary stage asymptotic giant branch
Spectral type M1 III
U−B color index +1.80
B−V color index +1.52
Astrometry
Radial velocity (Rv)50.19±0.30 km/s
Proper motion (μ) RA: −18.96 mas/yr
Dec.: −181.56 mas/yr
Parallax (π)11.10 ± 0.18 mas
Distance294 ± 5 ly
(90 ± 1 pc)
Absolute magnitude (MV)−0.87
Details
Mass1.6 M
Radius54 R
Luminosity631 L
Surface gravity (log g)1.0 cgs
Temperature4,009 K
Metallicity [Fe/H]0.06 dex
Rotational velocity (v sin i)3.8 km/s
Other designations
ν Vir, 3 Virginis, BD+07°2479, FK5 1302, HD 102212, HIP 57380, HR 4517, SAO 119035
Database references
SIMBADdata

This object is an M-type red giant, currently on the asymptotic giant branch, with a stellar classification of M1 III. It is an SRB-type semiregular variable star with its brightness varying by 0.0125 in magnitude. These variations have four periods lasting 11.1, 12.3, 16.8, and 23.7 days. This star has about 1.6 times the mass of the sun, but it has expanded to 54 times the Sun's radius and shines 631 times as brightly as the Sun. The effective temperature of its outer atmosphere is 4,009 K.

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.