  We report superluminal jet motion with an apparent speed of
$\beta_\mathrm{app}=1.65\pm0.57$ in the radio-quiet (RQ) low ionisation nuclear
emission line region (LINER) galaxy, KISSR872. This result comes from two epoch
phase-referenced very long baseline interferometry (VLBI) observations at 5
GHz. The detection of bulk relativistic motion in the jet of this extremely
radio faint AGN, with a total 1.4 GHz flux density of 5 mJy in the 5.4 arcsec
resolution Very Large Array (VLA) FIRST survey image and 1.5 mJy in the $\sim5$
milli-arcsec resolution Very Long Baseline Array (VLBA) image, is the first of
its kind in a RQ LINER galaxy. The presence of relativistic jets in lower
accretion rate objects like KISSR872, with an Eddington ratio of 0.04, reveals
that even RQ AGN can harbor relativistic jets, and evidentiates their
universality over a wide range of accretion powers.
