       lacaille 9352 (lac 9352) is a 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 even under excellent seeing conditions. parallax measurements place it at a distance of about  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 from lacaille 9352. ==distance==          ==properties== this star has the fourth highest known proper motion, (which was first noticed by benjamin gould in 1881) moving a total of 6.9 arcseconds per year. however, this is still a very small movement overall, as there are 3,600 arcseconds in a degree of arc. the space velocity components of this star are {{nowrap
Durchmusterung_objects Gliese_and_GJ_objects Henry_Draper_Catalogue_objects High-proper-motion_stars Hipparcos_objects M-type_main-sequence_stars Objects_within_100_ly_of_Earth Piscis_Austrinus