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Future Mars geophysical observatories for understanding its internal structure, rotation, and evolution

Dehant, V. and Banerdt, B. and Lognonné, P. and Grott, M. and Asmar, S. and Biele, J. and Breuer, D. and Forget, F. and Jaumann, R. and Johnson, C. L. and Knapmeyer, M. and Langlais, B. and Le Feuvre, M. and Mimoun, D. and Mocquet, A. and Read, P. and Rivoldini, A. and Romberg, O. and Schubert, G. and Smrekar, S.E. and Spohn, T. and Tortora, P. and Ulamec, S. and Vennerstrøm, S. (2012) Future Mars geophysical observatories for understanding its internal structure, rotation, and evolution. Planetary and Space Science, 68 (1), pp. 123-145. Elsevier Inc.. DOI: doi:10.1016/j.pss.2011.10.016.

Full text not available from this repository.

Official URL: http://www.sciencedirect.com/science/article/pii/S0032063311003278

Abstract

Our fundamental understanding of the interior of the Earth comes from seismology, geodesy, geochemistry, geomagnetism, geothermal studies, and petrology. For the Earth, measurements in those disciplines of geophysics have revealed the basic internal layering of the Earth, its dynamical regime, its thermal structure, its gross compositional stratification, as well as significant lateral variations in these quantities. Planetary interiors not only record evidence of conditions of planetary accretion and differentiation, they exert significant control on surface environments. We present recent advances in possible in-situ investigations of the interior of Mars, experiments and strategies that can provide unique and critical information about the fundamental processes of terrestrial planet formation and evolution. Such investigations applied on Mars have been ranked as a high priority in virtually every set of European, US and international high-level planetary science recommendations for the past 30 years. New seismological methods and approaches based on the cross-correlation of seismic noise by two seismic stations/landers on the surface of Mars and on joint seismic/orbiter detection of meteorite impacts, as well as the improvement of the performance of Very Broad-Band (VBB) seismometers have made it possible to secure a rich scientific return with only two simultaneously recording stations. In parallel, use of interferometric methods based on two Earth-Mars radio links simultaneously from landers tracked from Earth has increased the precision of radio science experiments by one order of magnitude. Magnetometer and heat flow measurements will complement seismic and geodetic data in order to obtain the best information on the interior of Mars. In addition to studying the present structure and dynamics of Mars, these measurements will provide important constraints for the astrobiology of Mars by helping to understand why Mars failed to sustain a magnetic field, by helping to understand the planet’s climate evolution, and by providing a limit for the energy available to the chemoautotrophic biosphere through a measurement of the surface heat flow. The landers of the mission will also provide meteorological stations to monitor the climate and obtain new measurements in the atmospheric boundary layer.

Document Type:Article
Title:Future Mars geophysical observatories for understanding its internal structure, rotation, and evolution
Authors:
AuthorsInstitution or Email of Authors
Dehant, V.Royal Observatory of Belgium, Brussels, Belgium
Banerdt, B.Jet Propulsion Laboratory, USA
Lognonné, P.IGPG Paris, France
Grott, M.matthias.grott@dlr.de
Asmar, S.Jet Propulsion Laboratory, USA
Biele, J.jens.biele@dlr.de
Breuer, D.doris.breuer@dlr.de
Forget, F.Laboratoire de Météorologie Dynamique, Paris, France
Jaumann, R. ralf.jaumann@dlr.de
Johnson, C. L.Planetary Science Institute, Tucson, AZ, USA
Knapmeyer, M.Martin.Knapmeyer@dlr.de
Langlais, B.Laboratoire de Planétologie et Géodynamique, UMR 6112, Université de Nantes, Nantes Atlantique Universités, CNRS, France
Le Feuvre, M.Laboratoire de Planétologie et Géodynamique, UMR 6112, Université de Nantes, Nantes Atlantique Universités, CNRS, France
Mimoun, D.Laboratoire de Planétologie et Géodynamique, UMR 6112, Université de Nantes, Nantes Atlantique Universités, CNRS, France
Mocquet, A.Laboratoire de Planétologie et Géodynamique, UMR 6112, Université de Nantes, Nantes Atlantique Universités, CNRS, France
Read, P.Atmospheric Oceanic and Planetary Physics, Oxford Physics, UK
Rivoldini, A.Royal Observatory of Belgium And Université catholique de Louvain, Earth and Life Institute (ELI), Georges Lemaître Centre for Earth and Climate Research (TECLIM), Belgium
Romberg, O.Institute of Space Systems (DLR), Bremen, Germany
Schubert, G.University of California, Los Angeles, California
Smrekar, S.E.Jet Propulsion Laboratory, California Institute of Technology, Pasa-dena
Spohn, T.Tilman.Spohn@dlr.de
Tortora, P.University of Bologna, Italy
Ulamec, S.stephan.ulamec@dlr.de
Vennerstrøm, S.National Space Institute, Technical University of Denmark, Denmark
Date:2012
Journal or Publication Title:Planetary and Space Science
Refereed publication:Yes
In Open Access:No
In SCOPUS:Yes
In ISI Web of Science:Yes
Volume:68
DOI:doi:10.1016/j.pss.2011.10.016
Page Range:pp. 123-145
Publisher:Elsevier Inc.
Status:Published
Keywords:Interior Structure; Rotation; Magnetic Field; Heat Flow; Seismology; Mars; Atmosphere; Habitability
HGF - Research field:Aeronautics, Space and Transport (old)
HGF - Program:Space (old)
HGF - Program Themes:W EW - Erforschung des Weltraums
DLR - Research area:Space
DLR - Program:W EW - Erforschung des Weltraums
DLR - Research theme (Project):W - Vorhaben Exploration des Sonnensystems (old)
Location: Köln-Porz , Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Planetary Physics
Space Operations and Astronaut Training > User center for space experiments (MUSC)
Institute of Planetary Research
Deposited By: Lena Noack
Deposited On:21 Dec 2011 11:30
Last Modified:26 Mar 2013 13:35

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