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Thermo-chemical Evolution and Global Contraction of Mercury

Grott, M. and Breuer, D. and Laneuville, M. (2011) Thermo-chemical Evolution and Global Contraction of Mercury. Earth and Planetary Science Letters, 307 (1-2), pp. 135-146. Elsevier. DOI: 10.1016/j.epsl.2011.04.040

Full text not available from this repository.

Official URL: http://www.sciencedirect.com/science/article/pii/S0012821X11002676

Abstract

The very limited amount of global contraction observed on Mercury's surface poses severe constraints on models of the planet's thermo-chemical evolution and current models rely on a very refractory, Thorium rich composition to slow planetary cooling. However, a refractory composition appears to be incompatible with evidence for pyroclastic eruptions, which require a substantial amount of volatiles to be present in the planetary interior. Furthermore, volcanic activity appears to have been ongoing for a considerable part of the planet's history, while current models predict an early cessation of crustal production. To address these inconsistencies we have reinvestigated the thermo-chemical evolution of Mercury using a non-refractory compositional model, taking the presence of a thermally insulating regolith layer into account. We find that models with a stiff mantle rheology satisfy the observational constraints if the regolith layer is at least 2 km thick. In these models, inefficient mantle convection and thermal insulation significantly slow planetary cooling and prolong the phase of crustal production to 2.5 Gyr after core formation, allowing the volume increase associated with mantle differentiation to offset some of the radial contraction caused by planetary cooling. Models furthermore predict substantial core sulfur contents above 6 wt.%, average crustal thicknesses between 10 and 40 km, and secular cooling rates of 30 K/Gyr.

Item URL in elib:https://elib.dlr.de/71497/
Document Type:Article
Title:Thermo-chemical Evolution and Global Contraction of Mercury
Authors:
AuthorsInstitution or Email of AuthorsAuthors ORCID iD
Grott, M.matthias.grott (at) dlr.deUNSPECIFIED
Breuer, D.doris.breuer (at) dlr.deUNSPECIFIED
Laneuville, M.Institut de Physique du Globe de Paris, Saint Maur des Fossés, FranceUNSPECIFIED
Date:2011
Journal or Publication Title:Earth and Planetary Science Letters
Refereed publication:Yes
Open Access:No
Gold Open Access:No
In SCOPUS:Yes
In ISI Web of Science:Yes
Volume:307
DOI :10.1016/j.epsl.2011.04.040
Page Range:pp. 135-146
Publisher:Elsevier
Status:Published
Keywords:Mercury; Mercury interior; thermal histories; Geophysics
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: Noack, Lena
Deposited On:08 Nov 2011 10:52
Last Modified:10 Jan 2019 15:47

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