  We present the first scattered light image of the debris disk around HD
129590, a ~1.3 M$_\odot$ G1V member of the Scorpius Centaurus association with
age ~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
$L_{\textrm{IR}}/L_{\textrm{star}}$~5$\times$10$^{-3}$, and has been resolved
in other studies using ALMA. We detect a nearly edge on ring, with evidence of
an inner clearing. We fit the debris disk using a model characterized by a
single bright ring, with radius ~60-70 AU, in broad agreement with previous
analysis of the target SED. The disk is vertically thin, and has an inclination
angle of ~75$^\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.
