elib
DLR-Header
DLR-Logo -> http://www.dlr.de
DLR Portal Home | Impressum | Kontakt | English
Schriftgröße: [-] Text [+]

Implications of Large Elastic Thicknesses for the Composition and Current Thermal State of Mars

Grott, M. und Breuer, D. (2008) Implications of Large Elastic Thicknesses for the Composition and Current Thermal State of Mars. In: Eos Trans. AGU, Fall Meet. Suppl., 89 (53), . AGU Fall meeting, 2008-12-14 - 2008-12-19, San Francisco, California (USA).

Dieses Archiv kann nicht den gesamten Text zur Verfügung stellen.

Kurzfassung

The elastic lithosphere thickness at the Martian north polar cap has recently been constrained using radar sounding data obtained by SHARAD, the shallow radar onboard the Mars Reconnaissance Orbiter. Analysis of the SHARAD radargrams showed that the amount of deflection caused by ice loading at the polar caps is negligible - less than 100 m. Quantitative analysis yielded a lower bound on the elastic lithosphere thickness T<sub>e</sub> of 300 km, a value twice as large as previous estimates from theoretical considerations and flexure studies. Such large elastic thicknesses are only compatible with the planet's thermal evolution if the planetary interior is relatively cold and this could have direct bearing on the admissible amount of radioactive elements in the Martian interior. On the other hand, if the concentration of heat producing elements in the Martian interior is indeed reduced, the resulting low interior temperatures could possibly inhibit partial mantle melting and magmatism. However, geological evidence suggests that Mars has been volcanically active in the recent past. We have investigated the Martian thermal evolution and identified models which are consistent with a present day elastic thickness in excess of 300 km. We find that a wet mantle rheology is best compatible with the observed elastic thicknesses, but in this case the bulk concentration of heat producing elements in the silicate fraction cannot exceed 50 % of the chondritic concentration if 50 % of the radioacitve elements are concentrated in the crust. Furthermore, due to the efficient cooling of the planet for a wet mantle rheology, recent volcanism can only be explained by hydrous mantle melting. This requires the mantle water content to exceed 1500 ppm and although this is within the range reported for the shergottite parent magmas, it is certainly on the boundary of the plausible parameter range. If a dry mantle rheology is assumed, bulk Mars does not need to be sub-chondritic, but at least 70 % of the radiogenic elements need to be concentrated in the crust to be consistent with the large elastic thicknesses. For a dry mantle, recent volcanism could be driven by decompression melting in the heads of strong mantle plumes which are present in numerical simulations of mantle convection if the viscosity is strongly pressure dependent or endothermic phase transitions are present near the core-mantle boundary.

Dokumentart:Konferenzbeitrag (Poster)
Titel:Implications of Large Elastic Thicknesses for the Composition and Current Thermal State of Mars
Autoren:
AutorenInstitution oder E-Mail-Adresse der Autoren
Grott, M.NICHT SPEZIFIZIERT
Breuer, D.NICHT SPEZIFIZIERT
Datum:Dezember 2008
Erschienen in:Eos Trans. AGU, Fall Meet. Suppl.
Referierte Publikation:Nein
In SCOPUS:Nein
In ISI Web of Science:Nein
Band:89
Seitenbereich:
Status:veröffentlicht
Stichwörter:Interiors, Volcanism, Mars, Planetary Sciences, SHARAD, Mars Reconnaissance Orbiter, MRO
Veranstaltungstitel:AGU Fall meeting
Veranstaltungsort:San Francisco, California (USA)
Veranstaltungsart:internationale Konferenz
Veranstaltungsdatum:2008-12-14 - 2008-12-19
HGF - Forschungsbereich:Verkehr und Weltraum (alt)
HGF - Programm:Weltraum (alt)
HGF - Programmthema:W EW - Erforschung des Weltraums
DLR - Schwerpunkt:Weltraum
DLR - Forschungsgebiet:W EW - Erforschung des Weltraums
DLR - Teilgebiet (Projekt, Vorhaben):W - Vorhaben Vergleichende Planetologie (alt)
Standort: Berlin-Adlershof
Institute & Einrichtungen:Institut für Planetenforschung > Planetenphysik
Hinterlegt von: Stefanie Hempel
Hinterlegt am:05 Jan 2009
Letzte Änderung:27 Apr 2009 15:39

Nur für Mitarbeiter des Archivs: Kontrollseite des Eintrags

Blättern
Suchen
Hilfe & Kontakt
Informationen
electronic library verwendet EPrints 3.3.12
Copyright © 2008-2013 Deutsches Zentrum für Luft- und Raumfahrt (DLR). Alle Rechte vorbehalten.