Magnetism of Shergottites
نویسندگان
چکیده
Introduction: New discoveries in cold (Antarctica) and hot desert areas have significantly increased the number of Martian meteorites (SNC) to more than 50 (unpaired) [1,2]. Martian meteorites are classified in four main groups in terms of their pe-trology and mineralogy, namely Orthopyroxenite (1 published member), Chassignites (dunite, 2), Nakhlites (clinopyroxenite, 7) and Shergottites (42) which are additionally subdivided in basal-tic, olivine-phyric, olivine-opx phyric, lherzolitic and one wehrlite [1]. Magnetism of shergottites: Recently, geochemical studies revealed that independently from the " old " scheme shergottites can be divided into 3 different subgroups based on their trace element and isotopic signature (enriched, depleted, and intermediate suite) [3]. This is interpreted as additionally reflecting the heterogeneity of the magma reservoirs [4]. The petrology and mineralogy of the lherzolitic shergottites is quite homogeneous (neglecting secondary processes) [5,6]. Their magnetic signature was found to follow specific trends, mainly depending on shock degree and terrestrial alteration effects, the latter in turn strongly depending on size/weight (TKW) of the individual Martian meteorites [7-9]. However, the magnetic signature of the members of the other shergottite groups appears quite scattered and was not found to follow distinct trends so far. In this study, we tried to (re-) compile published and original data, specifically addressing and incorporating new shergottite finds, concerning their magnetic signature in order to evaluate likely trends or groupings (such as for lherzolites). Additionally, the effects of secondary processes such as terrestrial alteration on the magnetic characteristics of the SNC were studied using the NWA 2975 (basaltic), SaU 005/008 and NWA 1068 (oliv.-phyric) and DaG 476 (oliv.-opx phyric) clans representing large sets of sample sizes and weights (TKW). The main result of our investigations is that only sufficiantly large sample sets and the respective databases allow to get insight and to eventually control these secondary processes in a satisfying manner.
منابع مشابه
The Magmatism of Mars Inferred from Chemical Composition of Shergottites
Introduction: It is well known that shergottites have a large variation of rare earth elements (REEs) abundance patterns and isotopic compositions. Jones [1] and Borg and Draper [2] suggest that light REEs (LREEs)-enriched shergottites resulted from mixing of a LREEs-enriched component with their parental magma. The LREEsenriched component is thought to be either Martian crust [1] or a KREEP-li...
متن کاملComparison of Redox States between Geochemically-intermediate and Enriched Lherzolitic Shergottites
Introduction: Lherzolitic shergottites show similar mineralogy and ages [e.g., 1,2], and are widely believed to have originated from the geochemically-intermediate reservoir having distinct trace element and isotopic compositions [e.g., 3,4]. RBT04262 and NWA4468 are recently discovered new shergottites that contain py-roxene oikocrysts enclosing olivine and chromite, and petrographically simil...
متن کاملSHOCK METAMORPHISM ON BADDELEYITE: IMPLICATION FOR U-Pb ISOTOPIC SYSTEMATICS OF SHERGOTTITES
Introduction: The age significance of isotope chronometers in basaltic shergottites is not agreed yet [1-3]. Bouvier et al. [3] argued that crystallization ages of shergottites were old (~4.1 Ga), and suggested that young ages of shergottites (i.e., ~180 Ma) represent reset by shock metamorphism. Baddeleyite (ZrO 2) is an important mineral for U-Pb dating of basaltic shergottites. By compressio...
متن کاملShergottite Lead Isotope Signature in Chassigny and the Nakhlites
Introduction: The nakhlites/chassignites and the shergottites represent two differing suites of basaltic martian meteorites. The shergottites have ages ≤ 0.6 Ga and a large range of initial Sr/Sr and e(Nd) ratios. Conversely, the nakhlites and chassignites cluster at 1.3-1.4 Ga and have a limited range of initial Sr/Sr and e(Nd) [1]. More importantly, the shergottites have e(W) < 1, whereas the...
متن کاملControls on Highly Siderophile Element Concentrations in Martian Basalt: Sulfide Saturation and Under-saturation
Introduction: Highly siderophile elements (HSE; Re, Au and the platinum group elements) in shergottites exhibit a wide range from very high, similar to the terrestrial mantle, to very low, similar to sulfide saturated mid ocean ridge basalt (e.g., [1]). This large range has been difficult to explain without good constraints on sulfide saturation or under-saturation [2]. A new model for predicti...
متن کامل