Smrekar, Suzanne E.
[Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA]
Lognonné, Philippe
[Institut de Physique du Globe de Paris, Univ Paris Diderot-Sorbonne Paris Cité, 35 rue Hélène Brion – Case 7071, Lamarck A, 75205 Paris Cedex 13, France]
Spohn, Tilman
[German Aerospace Center (DLR), Rutherfordstrasse 2, 12489 Berlin, Germany]
Banerdt, W. Bruce
[Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA]
Breuer, Doris
[German Aerospace Center (DLR), Rutherfordstrasse 2, 12489 Berlin, Germany]
Dehant, Véronique
[UCL]
The Interior exploration using Seismic Investigations, Geodesy, and Heat Transport (InSight) Mission will focus on Mars’ interior structure and evolution. The basic structure of crust, mantle, and core form soon after accretion. Understanding the early differentiation process on Mars and how it relates to bulk composition is key to improving our understanding of this process on rocky bodies in our solar system, as well as in other solar
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