Journal
ICARUS
Volume 215, Issue 2, Pages 596-598Publisher
ACADEMIC PRESS INC ELSEVIER SCIENCE
DOI: 10.1016/j.icarus.2011.07.036
Keywords
Planetesimals; Planetary formation; Origin, Solar System; Solar Nebula
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Funding
- Deutsche Forschungsgemeinschaft [FOR 759]
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We have examined the influence of impact angle in collisions between small dust aggregates and larger dust targets through laboratory experiments. Targets consisted of mu m-sized quartz dust and had a porosity of about 67%; the projectiles, between 1 and 5 mm in diameter, were slightly more compact (64% porosity). The collision velocity was centered at 20 m/s and impact angles range from 0 degrees to 45 degrees. At a given impact angle, the target gained mass for projectiles smaller than a threshold size, which decreases with increasing angle from about 3 mm to 1 mm. The fact that growth is possible up to the largest angles studied supports the idea of planetesimal formation by sweep-up of small dust aggregates. (C) 2011 Elsevier Inc. All rights reserved.
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