Experimental phase functions of mm-sized cosmic dust grains

Abstract

We present experimental phase functions of three types of millimeter-sized dust grains consisting of enstatite, quartz and volcanic material from Mount Etna, respectively. The three grains present similar sizes but different absorbing properties. The measurements are performed at 527 nm covering the scattering angle range from 3 to 170 degrees. The measured phase functions show two well defined regions i) soft forward peaks and ii) a continuous increase with the scattering angle at side- and back-scattering regions. This behavior at side- and back-scattering regions are in agreement with the observed phase functions for the Fomalhaut and HR 4796A dust rings. Further computations and measurements (including polarization) for millimeter sized-grains are needed to draw some conclusions about the fluffy or compact structure of the dust grains.

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• Models of Rosetta/OSIRIS 67P dust coma phase function
• HD 117214 debris disk: scattered-light images and constraints on the presence of planets
• The high-albedo, low polarization disk around HD 114082 harbouring a Jupiter-sized transiting planet
• Characterization of debris disks observed with SPHERE