*** Welcome to piglix ***

11 Leonis Minoris

11 Leonis Minoris A/B
Observation data
Epoch J2000      Equinox J2000
Constellation Leo Minor
Right ascension 09h 35m 39.50337s
Declination +35° 48′ 36.4874″
Apparent magnitude (V) 4.80/12.50
Characteristics
Spectral type G8V + M5V
U−B color index 0.44/—
B−V color index 0.77/—
Variable type RS CVn
Astrometry
Radial velocity (Rv) +14.40 km/s
Proper motion (μ) RA: -728.71 mas/yr
Dec.: -259.81 mas/yr
Parallax (π) 87.96 ± 0.32mas
Distance 37.1 ± 0.1 ly
(11.37 ± 0.04 pc)
Absolute magnitude (MV) 5.25±0.008
Orbit
Companion 11 LMi B
Period (P) 201 yr
Semi-major axis (a) 3.84″
Eccentricity (e) 0.88
Inclination (i) 117°
Details
11 LMi A
Mass 0.964 M
Radius 1.0029 ± 0.0158 R
Luminosity 0.7550 ± 0.0055 L
Temperature 5376 ± 43 K
Metallicity [Fe/H] +0.33 dex
Rotation 18.0 days
Age 7.9 Gyr
11 LMi B
Mass 0.23 M
Other designations
11 Leonis Minoris, GJ 356, HD 82885, HIP 47080, HR 3815, SAO 61586, WDS 09357+3549

11 Leonis Minoris (11 LMi) is a star system located 37 light years away from Earth, in the northern constellation of Leo Minor. The primary component is a G-type main sequence star of spectral type G8V, which is slightly more massive but slightly dimmer than Sol. This is an RS Canum Venaticorum variable star with its luminosity varying by 0.033 magnitudes over a period of 18 days. Compared to the Sun, it has more than double the abundance of elements more massive than helium—what astronomers term the star's metallicity.

There is a secondary component, a red dwarf star much dimmer than the primary. It has a highly eccentric orbit ranging from roughly 4 AU to 63 AU from the primary.

John J. Lumpkin used the star system in his novel Through Struggle, the Stars.



...
Wikipedia

...