First results from the cosmic dust aggregation experiment CODAG

被引:16
作者
Blum, J
Wurm, G
Poppe, T
Kempf, S
Kozasa, T
机构
[1] Inst Astrophys, D-07745 Jena, Germany
[2] Univ Observ, D-07745 Jena, Germany
[3] Univ Colorado, Atmospher & Space Phys Lab, Boulder, CO 80309 USA
[4] Max Planck Inst Nucl Phys, D-69117 Heidelberg, Germany
[5] Hokkaido Univ, Grad Sch Sci, Div Earth & Planetary Sci, Sapporo, Hokkaido 0600810, Japan
来源
IMPACT OF THE GRAVITY LEVEL ON MATERIALS PROCESSING AND FLUID DYNAMICS | 2002年 / 29卷 / 04期
关键词
D O I
10.1016/S0273-1177(01)00647-0
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The Cosmic Dust Aggregation Experiment (CODAG), an experimental simulation of the onset of planet formation, was successfully flown on STS-95 (October/November 1998) and on Maser 8 (May 1999). The main objective of the CODAG experiment was a direct observation of the Brownian motion-induced coagulation process of micron-sized dust particles. To overcome rapid sedimentation of the dust grains in the rarefied gas atmosphere, experiments were conducted in a long-duration microgravity environment. In the experiment, we observed that within several minutes the initially deagglomerated dust grains formed fractal dust aggregates due to their thermal motion and subsequent mutual collisions. The results from this experiment are the first experimental proof that the concept of pre-planetary dust coagulation is correct. (C) 2002 COSPAR. Published by Elsevier Science Ltd. All rights reserved.
引用
收藏
页码:497 / 503
页数:7
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