Interior structure of terrestrial planets: Modeling Mars' mantle and its electromagnetic, geodetic, and seismic properties
Identifieur interne : 001C08 ( Istex/Corpus ); précédent : 001C07; suivant : 001C09Interior structure of terrestrial planets: Modeling Mars' mantle and its electromagnetic, geodetic, and seismic properties
Auteurs : O. Verhoeven ; A. Rivoldini ; P. Vacher ; A. Mocquet ; G. Choblet ; M. Menvielle ; V. Dehant ; T. Van Hoolst ; J. Sleewaegen ; J. Barriot ; P. LognonnéSource :
- Journal of Geophysical Research: Planets [ 0148-0227 ] ; 2005-04.
Abstract
We present a new procedure to describe the one‐dimensional thermodynamical state and mineralogy of any Earth‐like planetary mantle, with Mars as an example. The model parameters are directly related to expected results from a geophysical network mission, in this case electromagnetic, geodetic, and seismological processed observations supplemented with laboratory measurements. We describe the internal structure of the planet in terms of a one‐dimensional model depending on a set of eight parameters: for the crust, the thickness and the mean density, for the mantle, the bulk volume fraction of iron, the olivine volume fraction, the pressure gradient, and the temperature profile, and for the core, its mass and radius. Currently, available geophysical and geochemical knowledge constrains the range of the parameter values. In the present paper, we develop the forward problem and present the governing equations from which synthetic data are computed using a set of parameter values. Among all Martian models fitting the currently available knowledge, we select eight candidate models for which we compute synthetic network science data sets. The synergy between the three geophysical experiments of electromagnetic sounding, geodesy, and seismology is emphasized. The stochastic inversion of the synthetic data sets will be presented in a companion paper.
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DOI: 10.1029/2004JE002271
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<front><div type="abstract">We present a new procedure to describe the one‐dimensional thermodynamical state and mineralogy of any Earth‐like planetary mantle, with Mars as an example. The model parameters are directly related to expected results from a geophysical network mission, in this case electromagnetic, geodetic, and seismological processed observations supplemented with laboratory measurements. We describe the internal structure of the planet in terms of a one‐dimensional model depending on a set of eight parameters: for the crust, the thickness and the mean density, for the mantle, the bulk volume fraction of iron, the olivine volume fraction, the pressure gradient, and the temperature profile, and for the core, its mass and radius. Currently, available geophysical and geochemical knowledge constrains the range of the parameter values. In the present paper, we develop the forward problem and present the governing equations from which synthetic data are computed using a set of parameter values. Among all Martian models fitting the currently available knowledge, we select eight candidate models for which we compute synthetic network science data sets. The synergy between the three geophysical experiments of electromagnetic sounding, geodesy, and seismology is emphasized. The stochastic inversion of the synthetic data sets will be presented in a companion paper.</div>
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<title>Interior structure of terrestrial planets: Modeling Mars' mantle and its electromagnetic, geodetic, and seismic properties</title>
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<affiliation>Royal Observatory of Belgium, Brussels, Belgium</affiliation>
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<author xml:id="author-2"><persName><forename type="first">A.</forename>
<surname>Rivoldini</surname>
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<affiliation>Royal Observatory of Belgium, Brussels, Belgium</affiliation>
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<author xml:id="author-3"><persName><forename type="first">P.</forename>
<surname>Vacher</surname>
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</author>
<author xml:id="author-4"><persName><forename type="first">A.</forename>
<surname>Mocquet</surname>
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<affiliation>Laboratoire de Planétologie et Géodynamique, UMR‐CNRS 6112, Université de Nantes, Nantes, France</affiliation>
</author>
<author xml:id="author-5"><persName><forename type="first">G.</forename>
<surname>Choblet</surname>
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<affiliation>Laboratoire de Planétologie et Géodynamique, UMR‐CNRS 6112, Université de Nantes, Nantes, France</affiliation>
</author>
<author xml:id="author-6"><persName><forename type="first">M.</forename>
<surname>Menvielle</surname>
</persName>
<affiliation>CETP/IPSL, UMR CNRS/UBSQ 8639, Observatoire de Saint‐Maur, Saint Maur des Fossés, France</affiliation>
<affiliation>Université Paris‐Sud, Paris, France</affiliation>
</author>
<author xml:id="author-7"><persName><forename type="first">V.</forename>
<surname>Dehant</surname>
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<affiliation>Royal Observatory of Belgium, Brussels, Belgium</affiliation>
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<author xml:id="author-8"><persName><forename type="first">T.</forename>
<surname>Van Hoolst</surname>
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<affiliation>Royal Observatory of Belgium, Brussels, Belgium</affiliation>
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<author xml:id="author-9"><persName><forename type="first">J.</forename>
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<author xml:id="author-10"><persName><forename type="first">J.‐P.</forename>
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<author xml:id="author-11"><persName><forename type="first">P.</forename>
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<abstract><p>We present a new procedure to describe the one‐dimensional thermodynamical state and mineralogy of any Earth‐like planetary mantle, with Mars as an example. The model parameters are directly related to expected results from a geophysical network mission, in this case electromagnetic, geodetic, and seismological processed observations supplemented with laboratory measurements. We describe the internal structure of the planet in terms of a one‐dimensional model depending on a set of eight parameters: for the crust, the thickness and the mean density, for the mantle, the bulk volume fraction of iron, the olivine volume fraction, the pressure gradient, and the temperature profile, and for the core, its mass and radius. Currently, available geophysical and geochemical knowledge constrains the range of the parameter values. In the present paper, we develop the forward problem and present the governing equations from which synthetic data are computed using a set of parameter values. Among all Martian models fitting the currently available knowledge, we select eight candidate models for which we compute synthetic network science data sets. The synergy between the three geophysical experiments of electromagnetic sounding, geodesy, and seismology is emphasized. The stochastic inversion of the synthetic data sets will be presented in a companion paper.</p>
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<abstractGroup><abstract type="main"><p xml:id="jgre1866-para-0001" label="1">We present a new procedure to describe the one‐dimensional thermodynamical state and mineralogy of any Earth‐like planetary mantle, with Mars as an example. The model parameters are directly related to expected results from a geophysical network mission, in this case electromagnetic, geodetic, and seismological processed observations supplemented with laboratory measurements. We describe the internal structure of the planet in terms of a one‐dimensional model depending on a set of eight parameters: for the crust, the thickness and the mean density, for the mantle, the bulk volume fraction of iron, the olivine volume fraction, the pressure gradient, and the temperature profile, and for the core, its mass and radius. Currently, available geophysical and geochemical knowledge constrains the range of the parameter values. In the present paper, we develop the forward problem and present the governing equations from which synthetic data are computed using a set of parameter values. Among all Martian models fitting the currently available knowledge, we select eight candidate models for which we compute synthetic network science data sets. The synergy between the three geophysical experiments of electromagnetic sounding, geodesy, and seismology is emphasized. The stochastic inversion of the synthetic data sets will be presented in a companion paper.</p>
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<abstract>We present a new procedure to describe the one‐dimensional thermodynamical state and mineralogy of any Earth‐like planetary mantle, with Mars as an example. The model parameters are directly related to expected results from a geophysical network mission, in this case electromagnetic, geodetic, and seismological processed observations supplemented with laboratory measurements. We describe the internal structure of the planet in terms of a one‐dimensional model depending on a set of eight parameters: for the crust, the thickness and the mean density, for the mantle, the bulk volume fraction of iron, the olivine volume fraction, the pressure gradient, and the temperature profile, and for the core, its mass and radius. Currently, available geophysical and geochemical knowledge constrains the range of the parameter values. In the present paper, we develop the forward problem and present the governing equations from which synthetic data are computed using a set of parameter values. Among all Martian models fitting the currently available knowledge, we select eight candidate models for which we compute synthetic network science data sets. The synergy between the three geophysical experiments of electromagnetic sounding, geodesy, and seismology is emphasized. The stochastic inversion of the synthetic data sets will be presented in a companion paper.</abstract>
<note type="additional physical form">Tab‐delimited Table 1.Tab‐delimited Table 2.Tab‐delimited Table 3.Tab‐delimited Table 4.Tab‐delimited Table 5.</note>
<subject><genre>keywords</genre>
<topic>internal structure</topic>
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<topic authorityURI="http://psi.agu.org/taxonomy5/3600">MINERALOGY AND PETROLOGY</topic>
<topic authorityURI="http://psi.agu.org/taxonomy5/3672">Planetary mineralogy and petrology</topic>
<topic authorityURI="http://psi.agu.org/taxonomy5/5400">PLANETARY SCIENCES: SOLID SURFACE PLANETS</topic>
<topic authorityURI="http://psi.agu.org/taxonomy5/5430">Interiors</topic>
<topic authorityURI="http://psi.agu.org/taxonomy5/5410">Composition</topic>
<topic authorityURI="http://psi.agu.org/taxonomy5/6200">PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS</topic>
<topic authorityURI="http://psi.agu.org/taxonomy5/6225">Mars</topic>
<topic authorityURI="http://psi.agu.org/taxonomy5/8100">TECTONOPHYSICS</topic>
<topic authorityURI="http://psi.agu.org/taxonomy5/8147">Planetary interiors</topic>
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<identifier type="ISSN">0148-0227</identifier>
<identifier type="eISSN">2156-2202</identifier>
<identifier type="DOI">10.1002/(ISSN)2156-2202e</identifier>
<identifier type="CODEN">JGREA2</identifier>
<identifier type="PublisherID">JGRE</identifier>
<part><date>2005</date>
<detail type="volume"><caption>vol.</caption>
<number>110</number>
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