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Members of the MIMOS II Consortium are G. Klingelhöfer, B. Bernhardt P. A. de Souza Jr., J. Foh, R. Gellert, P. Gütlich, E. Kankeleit, R. V. Morris, F. Renz, D. S. Rodionov, C. Schröder, T. Wdowiak, and A. Yen
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Members of the MIMOS II Consortium are G. Klingelhöfer, B. Bernhardt P. A. de Souza Jr., J. Foh, R. Gellert, P. Gütlich, E. Kankeleit, R. V. Morris, F. Renz, D. S. Rodionov, C. Schröder, T. Wdowiak, and A. Yen.
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The term "martian soil" is used here to denote any loose unconsolidated materials that can be distinguished from rocks, bedrock, or strongly cohesive sediments. No implication of the presence or absence of organic materials or living matter is intended.
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6
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3843090469
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Velocity calibration was done using a spectrum of an absorber of metallic iron and hematite that was acquired in transmission geometry simultaneous with measurements on surface targets. As calculated from the error signal, the deviation of the actual velocity from the ideal waveform is <1% at the velocity extremes (±12 mm/s) and <0.2% at velocities between +6 and -6 mm/s.
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Names have been assigned to areographic features by the MER team for planning and operations purposes. The names are not formally recognized by the International Astronomical Union.
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Bertelsen, P.1
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3843087245
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A martian solar day has a mean period of 24 hours 39 min 35.244 s and is referred to as a sol to distinguish this from a roughly 3% shorter solar day on Earth. A martian sidereal day, as measured with respect to the fixed stars, is 24 hours 37 min 22.663 s, as compared with 23 hours 56 min 04.0905 s for Earth. See http:/www.giss.nasa.gov/tools/mars24/ for more information.
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Development and realization for MIMOS II was funded by the German Space Agency under contract 50QM 99022. The project has been supported by the Technical University of Darmstadt and the University of Mainz. P.A. des acknowledges support of Coordenação de Aperfeiçamento de Pessoal de Nívet Superior (CAPES) (contract PASJ 142/1999) and Companhia Vale do Rio Doce (CVRD) from Brazil R.V.M. and D.W.M. acknowledge support of the NASA Mars Exploration Rover Project and the NASA Johnson Space Center. The support of the Russian Space agency is acknowledged. We also acknowledge the unwavering support of Jet Propulsion Laboratory engineering and operations staff.
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