Magnetic Properties Experiments on the Mars Exploration Rover mission

被引:52
作者
Madsen, MB
Bertelsen, P
Goetz, W
Binau, CS
Olsen, M
Folkmann, F
Gunnlaugsson, HP
Kinch, KM
Knudsen, JM
Merrison, J
Nornberg, P
Squyres, SW
Yen, AS
Rademacher, JD
Gorevan, S
Myrick, T
Bartlett, P
机构
[1] Univ Copenhagen, Niels Bohr Inst Astron Phys & Geophys, Ctr Planetary Sci, DK-2100 Copenhagen, Denmark
[2] Aarhus Univ, Dept Phys & Astron, Aarhus, Denmark
[3] Aarhus Univ, Dept Earth Sci, Aarhus, Denmark
[4] Cornell Univ, Ctr Radiophys & Space Res, Dept Astron, Ithaca, NY 14853 USA
[5] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[6] Honeybee Robot, New York, NY 10012 USA
关键词
Martian dust and soil; magnetic properties; permanent magnet instruments; magnetic dust; Mossbauer spectroscopy; ultrafine particle physics; IRON-OXIDES; MOSSBAUER; DUST; NANOPHASE; SOIL; METEORITES; HEMATITE; SPECTRA; ANALOG;
D O I
10.1029/2002JE002029
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 Mars Exploration Rovers each carry a set of Magnetic Properties Experiments designed with the following objectives in mind: (1) to identify the magnetic mineral(s) in the dust, soil and rocks on Mars, (2) to establish if the magnetic material is present in the form of nanosized (d < 10 nm) superparamagnetic crystallites embedded in the micrometer sized airborne dust particles, and (3) to establish if the magnets are culling a subset of strongly magnetic particles or if essentially all particles of the airborne dust are sufficiently magnetic to be attracted by the magnets. To accomplish these goals, the Mars Exploration Rovers each carry a set of permanent magnets of several different strengths and sizes. Each magnet has its own specific objective. The dust collected from the atmosphere by the Capture magnet and the Filter magnet (placed on the front of each rover) will be studied by the Mossbauer spectrometer and the Alpha Particle X-ray Spectrometer, both of which are instruments located on the rover's Instrument Deployment Device. The captured dust particles will also be imaged by the Pancam and Microscopic Imager. The Sweep magnet will be imaged by Pancam and is placed near the Pancam calibration target. The four magnets in the Rock Abrasion Tool (RAT) are designed to capture magnetic particles originating from the grinding of Martian surface rocks. The magnetic particles captured by the RAT magnets will be imaged by Pancam.
引用
收藏
页数:19
相关论文
共 47 条
[11]   MAGNETIC STUDIES ON SHERGOTTY AND OTHER SNC METEORITES [J].
CISOWSKI, SM .
GEOCHIMICA ET COSMOCHIMICA ACTA, 1986, 50 (06) :1043-1048
[12]   TITANOMAGHEMITE IN MAGNETIC SOILS ON EARTH AND MARS [J].
COEY, JMD ;
MORUP, S ;
MADSEN, MB ;
KNUDSEN, JM .
JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH AND PLANETS, 1990, 95 (B9) :14423-14425
[13]   Magnetic properties of Martian meteorites: Implications for an ancient Martian magnetic field [J].
Collinson, DW .
METEORITICS & PLANETARY SCIENCE, 1997, 32 (06) :803-811
[14]  
Fanale F.P., 1992, Mars, P1135
[15]   AN ASSESSMENT OF THE METEORITIC CONTRIBUTION TO THE MARTIAN SOIL [J].
FLYNN, GJ ;
MCKAY, DS .
JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH AND PLANETS, 1990, 95 (B9) :14497-14509
[16]   Rock Abrasion Tool: Mars exploration Rover mission [J].
Gorevan, SP ;
Myrick, T ;
Davis, K ;
Chau, JJ ;
Bartlett, P ;
Mukherjee, S ;
Anderson, R ;
Squyres, SW ;
Arvidson, RE ;
Madsen, MB ;
Bertelsen, P ;
Goetz, W ;
Binau, CS ;
Richter, L .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 2003, 108 (E12)
[17]  
Greenwood T.C., 1971, MOSSBAUER SPECTROSCO, DOI DOI 10.1007/978-94-009-5921-7
[18]   Analysis of the magnetic properties experiment data on Mars: results from Mars Pathfinder [J].
Gunnlaugsson, HP .
PLANETARY AND SPACE SCIENCE, 2000, 48 (15) :1491-1504
[19]   VIKING MAGNETIC-PROPERTIES EXPERIMENT - EXTENDED MISSION RESULTS [J].
HARGRAVES, RB ;
COLLINSON, DW ;
ARVIDSON, RE ;
CATES, PM .
JOURNAL OF GEOPHYSICAL RESEARCH, 1979, 84 :8379-8384
[20]   Magnetic enhancement on the surface of Mars? [J].
Hargraves, RB ;
Knudsen, JM ;
Bertelsen, P ;
Goetz, W ;
Gunnlaugsson, HP ;
Hviid, SF ;
Madsen, MB ;
Olsen, M .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 2000, 105 (E1) :1819-1827