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The influence of pressure-dependent viscosity on the thermal evolution of super-Earths

Stamenkovic, V. and Noack, L. and Breuer, D. and Spohn, T. (2012) The influence of pressure-dependent viscosity on the thermal evolution of super-Earths. The Astrophysical Journal, 748 (1/41), pp. 1-22. The American Astronomical Society. DOI: doi:10.1088/0004-637X/748/1/41. ISSN 0004-637X.

Full text not available from this repository.

Official URL: http://iopscience.iop.org/0004-637X/748/1/41/

Abstract

We study the thermal evolution of super-Earths with a one-dimensional (1D) parameterized convection model that has been adopted to account for a strong pressure dependence of the viscosity. A comparison with a 2D spherical convection model shows that the derived parameterization satisfactorily represents the main characteristics of the thermal evolution of massive rocky planets. We find that the pressure dependence of the viscosity strongly influences the thermal evolution of super-Earths—resulting in a highly sluggish convection regime in the lower mantles of those planets. Depending on the effective activation volume and for cooler initial conditions, we observe with growing planetary mass even the formation of a conductive lid above the core-mantle boundary (CMB), a so-called CMB-lid. For initially molten planets our results suggest no CMB-lids but instead a hot lower mantle and core as well as sluggish lower mantle convection. This implies that the initial interior temperatures, especially in the lower mantle, become crucial for the thermal evolution—the thermostat effect suggested to regulate the interior temperatures in terrestrial planets does not work for massive planets if the viscosity is strongly pressure dependent. The sluggish convection and the potential formation of the CMB-lid reduce the convective vigor throughout the mantle, thereby affecting convective stresses, lithospheric thicknesses, and heat fluxes. The pressure dependence of the viscosity may therefore also strongly affect the propensity of plate tectonics, volcanic activity, and the generation of a magnetic field of super-Earths.

Document Type:Article
Title:The influence of pressure-dependent viscosity on the thermal evolution of super-Earths
Authors:
AuthorsInstitution or Email of Authors
Stamenkovic, V.vlada.stamenkovic@dlr.de
Noack, L.lena.noack@dlr.de
Breuer, D.doris.breuer@dlr.de
Spohn, T.Tilman.Spohn@dlr.de
Date:2012
Journal or Publication Title:The Astrophysical Journal
Refereed publication:Yes
In SCOPUS:Yes
In ISI Web of Science:Yes
Volume:748
DOI:doi:10.1088/0004-637X/748/1/41
Page Range:pp. 1-22
Publisher:The American Astronomical Society
ISSN:0004-637X
Status:Published
Keywords:convection; Earth; planets and satellites: general; planets and satellites: interiors; planets and satellites: physical evolution; planets and satellites: tectonics
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: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Planetary Physics
Institute of Planetary Research
Deposited By: Lena Noack
Deposited On:27 Jun 2012 14:42
Last Modified:26 Mar 2013 13:39

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