Cosmic dust collection in aerogel

被引:107
作者
Burchell, Mark J. [1 ]
Graham, Giles
Kearsley, Anton
机构
[1] Univ Kent, Sch Phys Sci, Ctr Astrophys & Planetary Sci, Canterbury CT2 7NR, Kent, England
[2] Lawrence Livermore Natl Lab, Inst Geophys & Planetary Phys, Livermore, CA 94551 USA
[3] Nat Hist Museum, Dept Mineral, London SW7 2AZ, England
关键词
hypervelocity; impact; comet; asteroid;
D O I
10.1146/annurev.earth.34.031405.124939
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Aerogel is an ultra-low-density material that can be used to capture small particles incident upon it at speeds in excess of 1 km s(-1). This permits capture of cosmic dust in space where the high speeds usually result in destructive impact events. The performance of aerogel in laboratory impact tests is described. Completely intact capture is rare; most studies show that between 10% to 100% of the incident particle's mass is captured. However, in all cases unaltered domains were found in the particles captured in the laboratory at speeds up to 6 or 7 km s(-1). Several analytic techniques can be applied in situ to particles captured in aerogel, yielding data on the preimpact composition of the particle. Extraction techniques for removing small particles from aerogel are described, and after extraction, handling and analysis in the laboratory can proceed as for any small-sized particle. Coupled with the survival of intact regions in the captured particles, this allows detailed identification of the composition of the dust. Examples are given of current space missions using aerogel dust collectors: Data on these will soon be supplemented by cometary dust particles captured in aerogel on the NASA Stardust spacecraft.
引用
收藏
页码:385 / 418
页数:34
相关论文
共 78 条
[1]   STUDY OF A THRESHOLD CHERENKOV COUNTER BASED ON SILICA AEROGELS WITH LOW REFRACTIVE-INDEXES [J].
ADACHI, I ;
SUMIYOSHI, T ;
HAYASHI, K ;
IIDA, N ;
ENOMOTO, R ;
TSUKADA, K ;
SUDA, R ;
MATSUMOTO, S ;
NATORI, K ;
YOKOYAMA, M ;
YOKOGAWA, H .
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 1995, 355 (2-3) :390-398
[2]   PHYSICS OF INTERPLANETARY DUST CAPTURE VIA IMPACT INTO ORGANIC POLYMER FOAMS [J].
ANDERSON, WW ;
AHRENS, TJ .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 1994, 99 (E1) :2063-2071
[3]   Impact ionization from silica aerogel [J].
Auer, S .
INTERNATIONAL JOURNAL OF IMPACT ENGINEERING, 1998, 21 (1-2) :89-95
[4]  
Auer S., 2001, INSTRUMENTATION, P385
[5]  
BARRETT RA, 1992, P LUNAR PLANET SCI, V22, P203
[6]   PYROXENE WHISKERS AND PLATELETS IN INTERPLANETARY DUST - EVIDENCE OF VAPOR-PHASE GROWTH [J].
BRADLEY, JP ;
BROWNLEE, DE ;
VEBLEN, DR .
NATURE, 1983, 301 (5900) :473-477
[7]   COSMIC DUST - COLLECTION AND RESEARCH [J].
BROWNLEE, DE .
ANNUAL REVIEW OF EARTH AND PLANETARY SCIENCES, 1985, 13 :147-173
[8]   Stardust:: Comet and interstellar dust sample return mission -: art. no. 8111 [J].
Brownlee, DE ;
Tsou, P ;
Anderson, JD ;
Hanner, MS ;
Newburn, RL ;
Sekanina, Z ;
Clark, BC ;
Hörz, F ;
Zolensky, ME ;
Kissel, J ;
McDonnell, JAM ;
Sandford, SA ;
Tuzzolino, AJ .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 2003, 108 (E10)
[9]  
BROWNLEE DE, 1994, LUNAR PLANET SCI, V25, P183
[10]   ARE SOME CHONDRULE RIMS FORMED BY IMPACT PROCESSES - OBSERVATIONS AND EXPERIMENTS [J].
BUNCH, TE ;
SCHULTZ, P ;
CASSEN, P ;
BROWNLEE, D ;
PODOLAK, M ;
LISSAUER, J ;
REYNOLDS, R ;
CHANG, S .
ICARUS, 1991, 91 (01) :76-92