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Experiments on the photophoretic motion of chondrules and dust aggregates—Indications for the transport of matter in protoplanetary disks
Authors:Gerhard Wurm  Jens Teiser  Henning Haack
Affiliation:a Faculty of Physics, University Duisburg-Essen, Lotharstr. 1, 47057 Duisburg, Germany
b Institut für Planetologie, Wilhelm-Klemm-Str. 10, 48149 Münster, Germany
c Centre for Star and Planet Formation, Natural History Museum of Denmark, University of Copenhagen, Øster Voldgade 5-7, DK-1350 Copenhagen K, Denmark
Abstract:In a set of 16 drop tower experiments the motion of sub-millimeter to millimeter-sized particles under microgravity was observed. Illumination by a halogen lamp induced acceleration of the particles due to photophoresis. Photophoresis on dust-free chondrules, on chondrules, glass spheres and metal spheres covered with SiC dust and on pure SiC dust aggregates was studied. This is the first time that photophoretic motion of millimeter-sized particles has been studied experimentally. The absolute values for the photophoretic force are consistent with theoretical expectations for spherical particles. The strength of the photophoretic force varies for chondrules, dust covered particles and pure dust from low to strong, respectively. The measurements support the idea that photophoresis in the early Solar System can be efficient to transport solid particles outward.
Keywords:Disks   Experimental techniques   Origin, Solar System   Meteorites   Solar nebula
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