We present the first scattered light image of the debris disk around HD 129590 , a \sim 1.3 M _ { \odot } G1V member of the Scorpius Centaurus association with age \sim 10-16 Myr .
The debris disk is imaged with the high contrast imaging instrument SPHERE at the Very Large Telescope , and is revealed by both the IRDIS and IFS subsytems , operating in the H and YJ bands respectively .
The disk has a high infrared luminosity of L _ { \textrm { IR } } / L _ { \textrm { star } } \sim 5 \times 10 ^ { -3 } , and has been resolved in other studies using ALMA .
We detect a nearly edge on ring , with evidence of an inner clearing .
We fit the debris disk using a model characterized by a single bright ring , with radius \sim 60-70 AU , in broad agreement with previous analysis of the target SED .
The disk is vertically thin , and has an inclination angle of \sim 75 ^ { \circ } .
Along with other previously imaged edge-on disks in the Sco-Cen association such as HD 110058 , HD 115600 , and HD 111520 , this disk image will allow of the structure and morphology of very young debris disks , shortly after the epoch of planet formation has ceased .