  We present the first results of the eXtreme UV Environments (XUE) James Webb
Space Telescope (JWST) program, that focuses on the characterization of planet
forming disks in massive star forming regions. These regions are likely
representative of the environment in which most planetary systems formed.
Understanding the impact of environment on planet formation is critical in
order to gain insights into the diversity of the observed exoplanet
populations. XUE targets 15 disks in three areas of NGC 6357, which hosts
numerous massive OB stars, among which some of the most massive stars in our
Galaxy. Thanks to JWST we can, for the first time, study the effect of external
irradiation on the inner ($< 10$ au), terrestrial-planet forming regions of
proto-planetary disks. In this study, we report on the detection of abundant
water, CO, CO$_2$, HCN and C$_2$H$_2$ in the inner few au of XUE 1, a highly
irradiated disk in NGC 6357. In addition, small, partially crystalline silicate
dust is present at the disk surface. The derived column densities, the
oxygen-dominated gas-phase chemistry, and the presence of silicate dust are
surprisingly similar to those found in inner disks located in nearby,
relatively isolated low-mass star-forming regions. Our findings imply that the
inner regions of highly irradiated disks can retain similar physical and
chemical conditions as disks in low-mass star-forming regions, thus broadening
the range of environments with similar conditions for inner disk rocky planet
formation to the most extreme star-forming regions in our Galaxy.
