The ChemCam instrument suite on the Mars science laboratory (MSL) rover: Science objectives and mast unit description
Creators
- Maurice, S.1
- Gasnault, O.1
- Forni, O.1
- Baratoux, D.1
- Berger, G.1
- Cousin, A.1
- Cros, A.1
- Dupieux, M.1
- D'Uston, L.1
- Gharsa, T.1
- Lasue, J.1
- Meslin, P.Y.1
- Orttner, G.1
- Pares, L.1
- Parot, Y.1
- Pinet, P.1
- Salle, B.1
- Seran, H.1
- Thocaven, J.J.1
- Toplis, M.J.1
- Wiens, R.C.2
- Barraclough, B.2
- Bender, S.2
- Bernardin, J.2
- Clegg, S.2
- Dingler, B.2
- Lasue, J.2
- Stiglich, R.2
- Vaniman, D.2
- Saccoccio, M.3
- Faure, B.3
- Gaboriaud, A.3
- Michel, Y.3
- Paillet, A.3
- Perez, R.3
- Mangold, N.4
- Le Mouelic, S.4
- Sotin, C.4
- Berthe, M.5
- Langevin, Y.5
- Berthe, M.6
- Langevin, Y.6
- Bridges, N.7
- Blaney, D.8
- DeFlores, L.8
- Kan, E.8
- Limonadi, D.8
- Miller, E.8
- Sotin, C.8
- Simmonds, J.J.8
- Bouye, M.9
- Dubois, B.9
- Kouach, D.9
- Striebig, N.9
- Cais, P.10
- Quertier, B.10
- Clark, B.11
- Cremers, D.12
- Derycke, C.13
- Durand, E.13
- Dromart, G.14
- Fabre, C.15
- Herkenhoff, K.16
- Kirkland, L.17
- Lacour, J.L.18
- Mauchien, P.18
- Salle, B.18
- Sirven, J.B.18
- Lewin, E.19
- Lewin, E.20
- Manhes, G.21
- McKay, C.22
- Newsom, H.E.23
- Lescure, M.24
- Sautter, V.25
- Vaniman, D.26
- 1. Univ Toulouse 3, CNRS, Inst Rech Astrophys et Planetol, Observ Midi Pyrenees, F-31062 Toulouse, (France)
- 2. Los Alamos Natl Lab, Los Alamos, NM (United States)
- 3. Ctr Natl Etud Spatiales, F-31055 Toulouse, (France)
- 4. Univ Nantes, CNRS, Lab Planetol et Geodynam, Nantes, (France)
- 5. Univ Paris 11, Inst Astrophys Spatiale, Orsay, (France)
- 6. CNRS, F-91405 Orsay, (France)
- 7. Johns Hopkins Univ, Appl Phys Lab, Laurel, MD (United States)
- 8. CALTECH, Jet Prop Lab, Pasadena, CA (United States)
- 9. Observ Midi Pyrenees, Grp Instrumentat Sci, F-31400 Toulouse, (France)
- 10. Univ Bordeaux, CNRS, Lab Astrophys Bordeaux, Floirac, (France)
- 11. Space Sci Inst, Boulder, CO (United States)
- 12. Appl Res Associates, Albuquerque, NM (United States)
- 13. Thales Optron Sa, Elancourt, (France)
- 14. Univ Lyon, Lab Geol Lyon, ENS Lyon, Lyon, (France)
- 15. Univ Lorraine, CNRS, Vandoeuvre Les Nancy, (France)
- 16. US Geol Survey, Astrogeol Sci Ctr, Flagstaff, AZ 86001 (United States)
- 17. Lunar and Planetary Inst, Houston, TX 77058 (United States)
- 18. CEA, DEN, Dept Phys Chem, Gif Sur Yvette, (France)
- 19. Univ Grenoble 1, Inst Sci Terre, Grenoble, (France)
- 20. CNRS, Grenoble, (France)
- 21. Inst Phys Globe, Paris, (France)
- 22. NASA, Ames Res Ctr, Mountain View, CA (United States)
- 23. Univ New Mexico, Albuquerque, NM 87131 (United States)
- 24. CNRS, Lab Anal et Architecture Syst, Toulouse, (France)
- 25. Museum Natl Hist Nat, CNRS, Lab Mineral et Cosmochim, Paris, (France)
- 26. Planetary Sci Inst, Tucson, AZ (United States)
Description
ChemCam is a remote sensing instrument suite on board the 'Curiosity' rover (NASA) that uses Laser-Induced Breakdown Spectroscopy (LIBS) to provide the elemental composition of soils and rocks at the surface of Mars from a distance of 1.3 to 7 m, and a telescopic imager to return high resolution context and micro-images at distances greater than 1.16 m. We describe five analytical capabilities: rock classification, quantitative composition, depth profiling, context imaging, and passive spectroscopy. They serve as a toolbox to address most of the science questions at Gale crater. ChemCam consists of a Mast-Unit (laser, telescope, camera, and electronics) and a Body-Unit (spectrometers, digital processing unit, and optical de-multiplexer), which are connected by an optical fiber and an electrical interface. We then report on the development, integration, and testing of the Mast-Unit, and summarize some key characteristics of ChemCam. This confirmed that nominal or better than nominal performances were achieved for critical parameters, in particular power density (≥ 1 GW/cm2). The analysis spot diameter varies from 350 μm at 2 m to 550 μm at 7 m distance. For remote imaging, the camera field of view is 20 mrad for 1024*1024 pixels. Field tests demonstrated that the resolution (∼ 90 μrad) made it possible to identify laser shots on a wide variety of images. This is sufficient for visualizing laser shot pits and textures of rocks and soils. An auto-exposure capability optimizes the dynamical range of the images. Dedicated hardware and software focus the telescope, with precision that is appropriate for the LIBS and imaging depths-of-field. The light emitted by the plasma is collected and sent to the Body-Unit via a 6 m optical fiber. The companion to this paper (Wiens et al. this issue) reports on the development of the Body-Unit, on the analysis of the emitted light, and on the good match between instrument performance and science specifications. (authors)
Availability note (English)
Available from doi: http://dx.doi.org/10.1007/s11214-012-9912-2Additional details
Identifiers
Publishing Information
- Journal Title
- Space Science Reviews
- Journal Volume
- 170
- Journal Issue
- no.1-4
- Series
- Country input: France
- Journal Page Range
- p. 95-166
- ISSN
- 0038-6308
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- France
- INIS RN
- 45086508
- Subject category
- S37: INORGANIC, ORGANIC, PHYSICAL AND ANALYTICAL CHEMISTRY;
- Descriptors DEI
- CHEMICAL COMPOSITION; MARS PLANET; POWER DENSITY; QUANTITATIVE CHEMICAL ANALYSIS; REMOTE SENSING; ROCKS; SOILS; SURFACES; TELESCOPES; TEXTURE
- Descriptors DEC
- CHEMICAL ANALYSIS; PLANETS
Optional Information
- Notes
- 74 refs.