Extent of thermal ablation suffered by model organic microparticles during aerogel capture at hypervelocities

被引:26
作者
Burchell, M. J. [1 ]
Foster, N. J. [1 ]
Ormond-Prout, J. [2 ]
Dupin, D. [2 ]
Armes, S. P. [2 ]
机构
[1] Univ Kent, Sch Phys Sci, Canterbury CT2 7NH, Kent, England
[2] Univ Sheffield, Dept Chem, Sheffield S3 7HF, S Yorkshire, England
基金
英国科学技术设施理事会;
关键词
ENHANCED RAMAN-SCATTERING; COMET; 81P/WILD-2; SURFACE CHARACTERIZATION; LATEX-PARTICLES; POLYPYRROLE; IMPACTS; COLLECTION; DUST; IDENTIFICATION; PROJECTILES;
D O I
10.1111/j.1945-5100.2009.tb01182.x
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
New model organic microparticles are used to assess the thermal ablation that occurs during aerogel capture at speeds from 1 to 6 km s(-1). Commercial polystyrene particles (20 mu m diameter) were coated with all ultrathin 20 nm overlayer of an organic conducting polymer, polypyrrole. This overlayer comprises only 0.8% by mass of the projectile but has a very strong Raman signature, hence its survival or destruction is a sensitive measure of the extent of chemical degradation suffered. After aerogel capture, microparticles were located via optical microscopy and their composition was analyzed in situ using Raman microscopy. The ultrathin polypyrrole overlayer survived essentially intact for impacts at similar to 1 km s(-1), but significant surface carbonization was found at 2 km s(-1), and major particle mass loss at >= 3 km s(-1). Particles impacting at similar to 6.1 km s(-1) (the speed at which cometary dust was collected in the NASA Stardust mission) were reduced to approximately half their original diameter during aerogel capture (i.e., a mass loss of 84%). Thus significant thermal ablation occurs at speeds above a few km s(-1). This suggests that during the Stardust mission the thermal history of the terminal dust grains during capture in aerogel may be sufficient to cause significant processing or loss of organic materials. Further, while Raman D and G hands of carbon can be obtained from captured grains, they may well reflect the thermal processing during capture rather than the pre-impact particle's thermal history.
引用
收藏
页码:1407 / 1420
页数:14
相关论文
共 48 条
  • [1] Surface of young Jupiter family comet 81 P/Wild 2: View from the Stardust spacecraft
    Brownlee, DE
    Horz, F
    Newburn, RL
    Zolensky, M
    Duxbury, TC
    Sandford, S
    Sekanina, Z
    Tsou, P
    Hanner, MS
    Clark, BC
    Green, SF
    Kissel, J
    [J]. SCIENCE, 2004, 304 (5678) : 1764 - 1769
  • [2] BROWNLEE DE, 1994, 25 LUN PLAN SCI C 1, P183
  • [3] Comet 81P/Wild 2 under a microscope
    Brownlee, Don
    Tsou, Peter
    Aleon, Jerome
    Alexander, Conel M. O'D.
    Araki, Tohru
    Bajt, Sasa
    Baratta, Giuseppe A.
    Bastien, Ron
    Bland, Phil
    Bleuet, Pierre
    Borg, Janet
    Bradley, John P.
    Brearley, Adrian
    Brenker, F.
    Brennan, Sean
    Bridges, John C.
    Browning, Nigel D.
    Brucato, John R.
    Bullock, E.
    Burchell, Mark J.
    Busemann, Henner
    Butterworth, Anna
    Chaussidon, Marc
    Cheuvront, Allan
    Chi, Miaofang
    Cintala, Mark J.
    Clark, B. C.
    Clemett, Simon J.
    Cody, George
    Colangeli, Luigi
    Cooper, George
    Cordier, Patrick
    Daghlian, C.
    Dai, Zurong
    D'Hendecourt, Louis
    Djouadi, Zahia
    Dominguez, Gerardo
    Duxbury, Tom
    Dworkin, Jason P.
    Ebel, Denton S.
    Economou, Thanasis E.
    Fakra, Sirine
    Fairey, Sam A. J.
    Fallon, Stewart
    Ferrini, Gianluca
    Ferroir, T.
    Fleckenstein, Holger
    Floss, Christine
    Flynn, George
    Franchi, Ian A.
    [J]. SCIENCE, 2006, 314 (5806) : 1711 - 1716
  • [4] ARE SOME CHONDRULE RIMS FORMED BY IMPACT PROCESSES - OBSERVATIONS AND EXPERIMENTS
    BUNCH, TE
    SCHULTZ, P
    CASSEN, P
    BROWNLEE, D
    PODOLAK, M
    LISSAUER, J
    REYNOLDS, R
    CHANG, S
    [J]. ICARUS, 1991, 91 (01) : 76 - 92
  • [5] Short-period Jupiter family comets after Stardust
    Burchell, M. J.
    Kearsley, A. T.
    [J]. PLANETARY AND SPACE SCIENCE, 2009, 57 (10) : 1146 - 1161
  • [6] Hypervelocity capture of particles in aerogel: Dependence on aerogel properties
    Burchell, M. J.
    Fairey, S. A. J.
    Foster, N. J.
    Cole, M. J.
    [J]. PLANETARY AND SPACE SCIENCE, 2009, 57 (01) : 58 - 70
  • [7] Cosmic dust collection in aerogel
    Burchell, Mark J.
    Graham, Giles
    Kearsley, Anton
    [J]. ANNUAL REVIEW OF EARTH AND PLANETARY SCIENCES, 2006, 34 : 385 - 418
  • [8] Identification of minerals and meteoritic materials via Raman techniques after capture in hypervelocity impacts on aerogel
    Burchell, MJ
    Mann, J
    Creighton, JA
    Kearsley, AT
    Graham, G
    Franchi, IA
    [J]. METEORITICS & PLANETARY SCIENCE, 2006, 41 (02) : 217 - 232
  • [9] Identification of organic particles via Raman techniques after capture in hypervelocity impacts on aerogel
    Burchell, MJ
    Creighton, JA
    Kearsley, AT
    [J]. JOURNAL OF RAMAN SPECTROSCOPY, 2004, 35 (03) : 249 - 253
  • [10] Impact ionization experiments with low density conducting polymer-based micro-projectiles as analogues of solar system dusts
    Burchell, MJ
    Willis, MJ
    Armes, SP
    Khan, MA
    Percy, MJ
    Perruchot, C
    [J]. PLANETARY AND SPACE SCIENCE, 2002, 50 (10-11) : 1025 - 1035