Lacaille 9352

Lacaille 9352 (Lac 9352) is a red dwarf star in the southern constellation of Piscis Austrinus. With an apparent visual magnitude of 7.34, this star is too faint to be viewed with the naked eye except possibly under excellent seeing conditions. Parallax measurements place it at a distance of about 10.74 light-years (3.29 parsecs) from Earth. It is the eleventh closest star system to the Solar System and is the closest star in the constellation Piscis Austrinus. The ChView simulation shows that its closest neighbour is the EZ Aquarii triple star system at about 4.1 ly away.

Lacaille 9352

the neighborhood of the solar system which also includes Lacaille 9352
Observation data
Epoch J2000      Equinox J2000
Constellation Piscis Austrinus
Right ascension 23h 05m 52.03604s
Declination −35° 51 11.0475
Apparent magnitude (V) 7.34
Characteristics
Spectral type M0.5V
U−B color index +1.18
B−V color index +1.50
Variable type Suspected
Astrometry
Radial velocity (Rv)+9.7 km/s
Proper motion (μ) RA: +6,765.995 mas/yr
Dec.: +1,330.388 mas/yr
Parallax (π)304.1354 ± 0.0200 mas
Distance10.7241 ± 0.0007 ly
(3.2880 ± 0.0002 pc)
Absolute magnitude (MV)9.8
Details
Mass0.479+0.011
−0.010
 M
Radius0.474±0.008 R
Luminosity0.0368±0.0006 L
Surface gravity (log g)4.78 cgs
Temperature3,672+36
−34
 K
Metallicity [Fe/H]−0.22±0.09 dex
Rotational velocity (v sin i)1 km/s
Age4.57 Gyr
Other designations
HD 217987, CD-36°15693, GCTP 5584, GJ 887, LHS 70, SAO 214301, LTT 9348, LFT 1758, Cordoba 31353, NSV 14420, HIP 114046, UGPMF 591
Database references
SIMBADdata
ARICNSdata
Lacaille 9352
Location of Lacaille 9352 in the constellation Piscis Austrinus

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