61 Virginis

61 Virginis (abbreviated 61 Vir) is the Flamsteed designation of a G-type main-sequence star (G7V) slightly less massive than the Sun (which has a hotter G2V spectral type), located 27.8 light-years (8.5 parsecs) away in the constellation of Virgo. The composition of this star is nearly identical to the Sun.

61 Virginis

61 Vir as seen with a 12.5" telescope with a field of view of 45.1 arcminutes
Observation data
Epoch J2000      Equinox J2000
Constellation Virgo
Right ascension 13h 18m 24.31399s
Declination −18° 18 40.2977
Apparent magnitude (V) 4.74
Characteristics
Spectral type G7V
Apparent magnitude (B) 5.45
Apparent magnitude (J) 3.334
Apparent magnitude (H) 2.974
Apparent magnitude (K) 2.956
U−B color index 0.26
B−V color index 0.71
V−R color index 0.37
R−I color index 0.33
Astrometry
Radial velocity (Rv)−7.86±0.13 km/s
Proper motion (μ) RA: −1,070.202 mas/yr
Dec.: −1,063.849 mas/yr
Parallax (π)117.1726 ± 0.1456 mas
Distance27.84 ± 0.03 ly
(8.53 ± 0.01 pc)
Absolute magnitude (MV)5.07
Details
Mass0.93 M
Radius0.9867±0.0048 R
Luminosity0.8222±0.0033 L
Surface gravity (log g)4.5 cgs
Temperature5538±13 K
Metallicity [Fe/H]−0.02 dex
Rotation29 days
Rotational velocity (v sin i)3.9 ± 0.9 km/s
Age6.1–6.6 Gyr
Other designations
BD-17°3813, FK5 1345, GCTP 3039.00, GJ 506, HD 115617, HIP 64924, HR 5019, LHS 349, LTT 5111, SAO 157844.
Database references
SIMBADdata
Exoplanet Archivedata
ARICNSdata

61 Virginis (G7V) is the first well-established main-sequence star very similar to the Sun with a potential super-Earth, though it was preceded by CoRoT-7 (a borderline orange dwarf).

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