  The recent discoveries of nearby star clusters and associations within a few
hundred pc of the Sun, as well as the order of magnitude difference in the
formation rates of the embedded and open cluster populations, suggests that
additional poor stellar groups are likely to be found at surprisingly close
distances to the Sun. Here I describe a new nearby stellar aggregate found by
virtue of the parallel proper motions, similar trigonometric parallaxes, and
consistent color-magnitude distribution of its early-type members. The 120
Myr-old group lies in Ophiuchus at $d$ $\simeq$ 170 pc, with its most massive
member being the 4th-magnitude post-MS B8II-III star $\mu$ Oph. The group may
have escaped previous notice due to its non-negligible extinction ($A_V$
$\simeq$ 0.9 mag). If the group was born with a normal initial mass function,
and the nine B- and A-type systems represent a complete system of
intermediate-mass stars, then the original population was probably of order
$\sim$200 systems. The age and space motion of the new cluster are very similar
to those of the Pleiades, $\alpha$ Per cluster, and AB Dor Moving Group,
suggesting that these aggregates may have formed in the same star-forming
complex some $\sim10^8$ yr ago.
