Cometary and Interstellar Dust Analyzer for comet Wild 2 -: art. no. 8114

被引:51
作者
Kissel, J
Glasmachers, A
Grün, E
Henkel, H
Höfner, H
Haerendel, G
von Hoerner, H
Hornung, K
Jessberger, EK
Krueger, FR
Möhlmann, D
Greenberg, JM
Langevin, Y
Silén, J
Brownlee, D
Clark, BC
Hanner, MS
Hoerz, F
Sandford, S
Sekanina, Z
Tsou, P
Utterback, NG
Zolensky, ME
Heiss, C
机构
[1] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
[2] Univ Wuppertal, Fachbereich Elektrotech & Informat Tech, D-42119 Wuppertal, Germany
[3] Max Planck Inst Kernphys, D-69117 Heidelberg, Germany
[4] Von Hoerner & Sulgar GmbH, D-68723 Schwetzingen, Germany
[5] Int Univ Bremen, D-28725 Bremen, Germany
[6] Univ Neubiberg, D-85577 Neubiberg, Germany
[7] Univ Munster, Inst Planetol, D-48149 Munster, Germany
[8] Ingenieurbuero Krueger, D-64291 Darmstadt, Germany
[9] DLR Inst Weltraumsensorik, D-12489 Berlin, Germany
[10] Fac Sci Orsay, Inst Astrophys, F-91405 Orsay, France
[11] Finnish Meteorol Inst, Dept Geophys, SF-00101 Helsinki, Finland
[12] Univ Washington, Dept Astron, Seattle, WA 98105 USA
[13] Lockheed Martin Aerosp, Denver, CO 80201 USA
[14] Jet Prop Lab, Pasadena, CA 91103 USA
[15] NASA, Lyndon B Johnson Space Ctr, Houston, TX 77058 USA
[16] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[17] Merck AG, Darmstadt, Germany
关键词
dust mass spectrometer; interstellar and cometary dust; composition; positive and negative ions; instrument description;
D O I
10.1029/2003JE002091
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
[1] The Cometary and Interstellar Dust Analyzer (CIDA) instrument analyzes the composition of individual grains in the cometary coma. As each particle impacts a silver plate, the high-impact energy due to the relative velocity of the spacecraft as it flies through the coma causes the elements and molecular compounds in the particle to become ionized. Using a fast time-of-flight mass spectrometer, a complete set of ions are detected for each impact, from a mass range of 1 ( atomic hydrogen) up to a few thousand atomic mass units, encompassing all elements in the periodic table and many molecules, such as organic compounds. This experimental technique has already been applied with excellent success at Halley's comet, and the CIDA derivative instrument is flying on the Stardust mission, which will encounter comet Wild 2 in January of 2004. The data returned will give clues to the elemental and chemical composition of the dust component of this comet.
引用
收藏
页数:8
相关论文
共 22 条
[1]  
CLARK BC, 1987, ASTRON ASTROPHYS, V187, P779
[2]   HEOS 2 AND HELIOS MICROMETEOROID EXPERIMENTS [J].
DIETZEL, H ;
EICHHORN, G ;
FECHTIG, H ;
GRUN, E ;
HOFFMANN, HJ ;
KISSEL, J .
JOURNAL OF PHYSICS E-SCIENTIFIC INSTRUMENTS, 1973, 6 (03) :209-217
[3]  
FRIICHTENICHT JF, 1963, 6 S HYP IMP CLEV OH
[4]  
GRUN E, 1977, J GEOPHYS-Z GEOPHYS, V42, P717
[5]  
JESSBERGER EK, 1991, ASTROPHYS SPACE SC L, V167, P1075, DOI 10.1017/S0252921100012823
[6]  
Jessberger EK, 2001, ASTR AST LI, P253
[7]   THE ORGANIC-COMPONENT IN DUST FROM COMET HALLEY AS MEASURED BY THE PUMA MASS-SPECTROMETER ON BOARD VEGA-1 [J].
KISSEL, J ;
KRUEGER, FR .
NATURE, 1987, 326 (6115) :755-760
[8]   COMPOSITION OF COMET HALLEY DUST PARTICLES FROM VEGA OBSERVATIONS [J].
KISSEL, J ;
SAGDEEV, RZ ;
BERTAUX, JL ;
ANGAROV, VN ;
AUDOUZE, J ;
BLAMONT, JE ;
BUCHLER, K ;
EVLANOV, EN ;
FECHTIG, H ;
FOMENKOVA, MN ;
VONHOERNER, H ;
INOGAMOV, NA ;
KHROMOV, VN ;
KNABE, W ;
KRUEGER, FR ;
LANGEVIN, Y ;
LEONAS, VB ;
LEVASSEURREGOURD, AC ;
MANAGADZE, GG ;
PODKOLZIN, SN ;
SHAPIRO, VD ;
TABALDYEV, SR ;
ZUBKOV, BV .
NATURE, 1986, 321 (6067) :280-282
[9]   Time-of-flight mass spectrometric analysis of ion formation in hypervelocity impact of organic polymer microspheres:: comparison with secondary ion mass spectrometry, 252Cf mass spectrometry and laser mass spectrometry [J].
Kissel, J ;
Krueger, FR .
RAPID COMMUNICATIONS IN MASS SPECTROMETRY, 2001, 15 (18) :1713-1718
[10]   ION FORMATION BY IMPACT OF FAST DUST PARTICLES AND COMPARISON WITH RELATED TECHNIQUES [J].
KISSEL, J ;
KRUEGER, FR .
APPLIED PHYSICS A-MATERIALS SCIENCE & PROCESSING, 1987, 42 (01) :69-85