PRIMA far-infrared observations could detect water ice disks (44 µm feature) within 60 pc and water vapor disks within 20 pc for masses above ~10^20 g, based on synthetic spectra.
Doppler imaging of the planetary debris disc at the white dwarf SDSS J122859.93+104032.9,
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Detecting water ice and vapor disks originating from icy planetary bodies around white dwarfs with future PRIMA observations
PRIMA far-infrared observations could detect water ice disks (44 µm feature) within 60 pc and water vapor disks within 20 pc for masses above ~10^20 g, based on synthetic spectra.