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The X-ray regime is a largely underused resource for constraininginterstellar dust grain models and improving our understanding of the physicalprocesses that dictate how grains evolve over their lifetimes. This is mostlydue to current detectors' relatively low sensitivity and high background,limiting the targets to the brightest sources. The improved sensitivity of thenext generation of X-ray detectors will allow studies of much fainter sources,at much higher angular resolution, expanding our sampled sightlines in bothquality and quantity.

Astro2020 Science White Paper: Probing the Structure of Interstellar Dust from Micron to Kpc Scales with X-ray Imaging