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Dynamical modeling of Mars deep interior Sylvaine Ferrachat Institut für Planetologie Westfälische Wilhelms-Universität Münster

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Page 1: Dynamical modeling of Mars deep interior Sylvaine Ferrachat Institut für Planetologie Westfälische Wilhelms-Universität Münster

Dynamical modeling of Mars deep interior

Sylvaine Ferrachat

Institut für PlanetologieWestfälische Wilhelms-Universität Münster

Page 2: Dynamical modeling of Mars deep interior Sylvaine Ferrachat Institut für Planetologie Westfälische Wilhelms-Universität Münster

Main projects / Interests

Earth mantle dynamics– Convection pattern– Relationships

convection/plate tectonics– Mixing properties of 2D, 3D

conv. Syst.– Secular chemical evolution– Relationships convection

basalt / geochemistry

Mars mantle dynamics– Early history and chemical

distribution– Magnetic field– Gravity field– Magmatism

Page 3: Dynamical modeling of Mars deep interior Sylvaine Ferrachat Institut für Planetologie Westfälische Wilhelms-Universität Münster

Main projects / Interests

Earth mantle dynamics– Convection pattern– Relationships

convection/plate tectonics– Mixing properties of 2D, 3D

conv. Syst.– Secular chemical evolution– Relationships convection

basalt / geochemistry

Mars mantle dynamics– Early history and chemical

distribution– Magnetic field– Gravity field– Magmatism

Curriculum– 2000, PhD thesis, ENS

Lyon, adv. Y. Ricard

– 2000 - 2002, Post-doc, UC Davis

– 2002 - 2003, teaching assistant, IUFM Lyon

– 2003 - 2004 consultancy for UC Davis

– 2004, post-doc, IfP Münster

Page 4: Dynamical modeling of Mars deep interior Sylvaine Ferrachat Institut für Planetologie Westfälische Wilhelms-Universität Münster

Main projects / Interests

Earth mantle dynamics– Convection pattern– Relationships

convection/plate tectonics– Mixing properties of 2D, 3D

conv. Syst.– Secular chemical evolution– Relationships convection

basalt / geochemistry

Mars mantle dynamics– Early history and chemical

distribution– Magnetic field– Gravity field– Magmatism

Curriculum– 2000, PhD thesis, ENS

Lyon, adv. Y. Ricard

– 2000 - 2002, Post-doc, UC Davis

– 2002 - 2003, teaching assistant, IUFM Lyon

– 2003 - 2004 consultancy for UC Davis

– 2004, post-doc, IfP Münster

Page 5: Dynamical modeling of Mars deep interior Sylvaine Ferrachat Institut für Planetologie Westfälische Wilhelms-Universität Münster

Main projects / Interests

Earth mantle dynamics– Convection pattern– Relationships

convection/plate tectonics– Mixing properties of 2D, 3D

conv. Syst.– Secular chemical evolution– Relationships convection

basalt / geochemistry

Mars mantle dynamics– Early history and chemical

distribution– Magnetic field– Gravity field– Magmatism

Curriculum– 2000, PhD thesis, ENS

Lyon, adv. Y. Ricard

– 2000 - 2002, Post-doc, UC Davis

– 2002 - 2003, teaching assistant, IUFM Lyon

– 2003 - 2004 consultancy for UC Davis

– 2004, post-doc, IfP Münster

Page 6: Dynamical modeling of Mars deep interior Sylvaine Ferrachat Institut für Planetologie Westfälische Wilhelms-Universität Münster

Earth mantle efficient convection

Vs

Distinct geochemical signatures in basalt

PhD thesisMixing in the mantle & geochemical heterogeneities

Page 7: Dynamical modeling of Mars deep interior Sylvaine Ferrachat Institut für Planetologie Westfälische Wilhelms-Universität Münster

Features:•Partial melting based on adiabatic equilibrium•Latent heat consumption and feedback on local temperature

Intentions:•Evolution of the distribution of chemical species and isotope ratios (U, Pb, He,…) in the whole system

F in each cell of the partial melting zone

Concentration of any incompatible

species

Low

High

Heterogeneous residu

Homogeneous

Basaltic liquid

Fractionation law

Scientific project in UC DavisThermochemical convection & dynamical partial melting

Page 8: Dynamical modeling of Mars deep interior Sylvaine Ferrachat Institut für Planetologie Westfälische Wilhelms-Universität Münster

Current MAGE project:Mars early history & mantle dynamics

Would chemical stratif. due to fractional crystallization of a deep magma ocean be able to start a dynamo and reproduce the Martian magnetic history?

This work investigates this idea with convective models…

…sudden cooling of the CMB?After L. Elkins-Tanton et al, 2003

Page 9: Dynamical modeling of Mars deep interior Sylvaine Ferrachat Institut für Planetologie Westfälische Wilhelms-Universität Münster

Current MAGE project

Page 10: Dynamical modeling of Mars deep interior Sylvaine Ferrachat Institut für Planetologie Westfälische Wilhelms-Universität Münster

Current MAGE project

Page 11: Dynamical modeling of Mars deep interior Sylvaine Ferrachat Institut für Planetologie Westfälische Wilhelms-Universität Münster

Current MAGE projectFuture directions

An improved model will take into account:

– Phase transitions

– Viscosity variations

– Partial melting

This model will be tested against its effects on:

– Magnetic field history

– Volcanism

– Gravity signal

Page 12: Dynamical modeling of Mars deep interior Sylvaine Ferrachat Institut für Planetologie Westfälische Wilhelms-Universität Münster

Current MAGE projectFuture directions

An improved model will take into account:

– Phase transitions

– Viscosity variations

– Partial melting

This model will be tested against its effects on:

– Magnetic field history

– Volcanism

– Gravity signal

Collab. with other teams within the MAGE Network

Page 13: Dynamical modeling of Mars deep interior Sylvaine Ferrachat Institut für Planetologie Westfälische Wilhelms-Universität Münster

Current Experience in the Network

A few general points:

– Late arrival in the Network (as most postdocs here!)

Only a brief experience…

– Really nice welcome in the group

– Good scientific exchanges and discussions within the group

A big advantage of being part of the MAGE network:Switch from solid Earth dynamics community

to planetology community

Opportunity to:– Enlarge my field– Enter the planetology community