MIRI/JWST images of HD 106906's debris disk, modeled with radiative transfer, imply a 70 au disk with a filled inner region, micron-sized grains, and a dust mass of about 0.003 Earth masses for the mid-IR-emitting grains (0.1-0.16 Earth masses when extrapolated to centimeter sizes).
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MIRI-JWST mid-infrared direct imaging of the debris disk of HD106906
MIRI/JWST images of HD 106906's debris disk, modeled with radiative transfer, imply a 70 au disk with a filled inner region, micron-sized grains, and a dust mass of about 0.003 Earth masses for the mid-IR-emitting grains (0.1-0.16 Earth masses when extrapolated to centimeter sizes).