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Influence of a variable thermal conductivity on the thermo-chemical evolution of Mars

Schumacher, S. and Breuer, D (2005) Influence of a variable thermal conductivity on the thermo-chemical evolution of Mars. Journal of Geophysical Research, 111 (E2), E02006. DOI: doi:10.1029/2005JE002429. ISSN 0148-0227.

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Abstract

The influences of variations in thermal conductivity due to composition, temperature, and pressure in mantle and crust on the thermochemical evolution of Mars have been examined with parameterized convection models. We use a temperature- and pressure-dependent thermal conductivity in the mantle and column-averaged values between 1.5 and 4 Wm<sup>-1</sup>K<sup>-1</sup> for the crust (with 2 Wm<sup>-1</sup>K<sup>-1</sup> as the representative value for a basaltic crust). The major characteristic of the models is a slower cooling of the upper mantle with a long-existing global partial melt zone and a stronger crustal production late in the evolution compared to earlier models which assume a constant thermal conductivity of 4 Wm<sup>-1</sup>K<sup>-1</sup>. To explain the observed crustal thickness and the early crustal formation on Mars, the formation of an enriched primordial crust is required. Recent volcanism can be explained by lateral temperature variations that are caused by thickness variations of the low conducting crust. These melt zones which occur underneath thicker than average crust may be the source region for the observed longstanding volcanism in Tharsis and Elysium instead of plumes rising from the core-mantle boundary. The evolution of the elastic lithosphere is characterized by a transition at which the elastic strength is first provided by the crust and later also by the upper mantle. This finding may explain the estimated elastic lithosphere thickness of less than 16 km in the Noachian and more than 100 km in the Hesperian and Amazonian.

Document Type:Article
Title:Influence of a variable thermal conductivity on the thermo-chemical evolution of Mars
Authors:
AuthorsInstitution or Email of Authors
Schumacher, S.Institute for Planetology, University of Münster
Breuer, DUNSPECIFIED
Date:2005
Journal or Publication Title:Journal of Geophysical Research
Refereed publication:Yes
In ISI Web of Science:Yes
Volume:111
DOI:doi:10.1029/2005JE002429
Page Range:E02006
ISSN:0148-0227
Status:Published
Keywords:Mars, planetary interior, thermal conductivity, thermal evolution.
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 Vergleichende Planetologie (old)
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Planetary Physics
Deposited By: Nils Müller
Deposited On:01 Mar 2006
Last Modified:14 Jan 2010 20:23

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