  Using VLT/SPHERE near-infrared dual-band imaging and integral field
spectroscopy we discovered an edge-on debris disk around the 17\,Myr old A-type
member of the Scorpius-Centaurus OB association HD 110058. The edge-on disk can
be traced to about 0.6" or 65 AU projected separation. In its northern and
southern wings, the disk shows at all wavelengths two prominent, bright and
symmetrically placed knots at 0.3" or 32 AU from the star. We interpret these
knots as a ring of planetesimals whose collisions may produce most of the dust
observed in the disk. We find no evidence for a bow in the disk, but we
identify a pair of symmetric, hook-like features in both wings. Based on
similar features in the Beta Pictoris disk we propose that this wing-tilt
asymmetry traces either an outer planetesimal belt that is inclined with
respect to the disk midplane or radiation-pressure-driven dust blown out from a
yet unseen, inner belt which is inclined with respect to the disk midplane. The
misaligned inner or outer disk may be a result of interaction with a yet unseen
planet. Overall, the disk geometry resembles the nearby disk around Beta
Pictoris, albeit seen at smaller radial scales.
