Northwest Africa 16788: The Largest Known Individual Martian Meteorite—A New Olivine Microgabbroic Shergottite and Its Implications for Martian Magmatism
Xhonatan Shehaj, Giovanni Pratesi, Cristian Carli, Riccardo Avanzinelli, Alice Stephant, Annarita Franza, Eleonora Ammannito
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Abstract
We present a comprehensive study of a new Martian meteorite, Northwest Africa (NWA) 16788, found in the Sahara Desert in July 2023. This specimen constitutes the largest known individual meteorite of Martian origin, with a total weight of ⁓25 kg. A detailed mineralogical and geochemical investigation identifies NWA 16788 as an enriched olivine microgabbroic shergottite. Petrographic analysis reveals a millimeter-sized cumulate texture, which is intermediate between poikilitic and gabbroic shergottites, primarily composed of pyroxene (⁓61 vol.%), maskelynite (shocked plagioclase, ⁓21 vol.%), and olivine (⁓15 vol.%). Pyroxene grains exhibit a distinctive zoning pattern, placing NWA 16788 within a small group of Martian meteorites and lunar samples that record unique cooling histories, suggesting that similar samples may be more prevalent within the Martian igneous rocks than previously recognized. High-precision analyses of bulk 143Nd/144Nd and 87Sr/86Sr isotopic composition, combined with trace element abundance, indicate that NWA 16788 originated from the partial melting of an enriched Martian mantle source. Electron backscatter diffraction analysis reveals a unimodal distribution of olivine grain misorientation, averaging ⁓4.6°, consistent with a high-energy single-impact event. Moreover, visible and near-infrared spectroscopy data acquired on NWA 16788 could aid in identifying potential locations of analogous igneous rocks on the Martian surface. Finally, this study proposes refinements to the current classification scheme of Martian meteorites, aiming to reduce taxonomic ambiguity and improve the alignment between Martian meteorites and Martian igneous rocks, based on data from Mars rovers.
期刊介绍:
The Journal of Geophysical Research Planets is dedicated to the publication of new and original research in the broad field of planetary science. Manuscripts concerning planetary geology, geophysics, geochemistry, atmospheres, and dynamics are appropriate for the journal when they increase knowledge about the processes that affect Solar System objects. Manuscripts concerning other planetary systems, exoplanets or Earth are welcome when presented in a comparative planetology perspective. Studies in the field of astrobiology will be considered when they have immediate consequences for the interpretation of planetary data. JGR: Planets does not publish manuscripts that deal with future missions and instrumentation, nor those that are primarily of an engineering interest. Instrument, calibration or data processing papers may be appropriate for the journal, but only when accompanied by scientific analysis and interpretation that increases understanding of the studied object. A manuscript that describes a new method or technique would be acceptable for JGR: Planets if it contained new and relevant scientific results obtained using the method. Review articles are generally not appropriate for JGR: Planets, but they may be considered if they form an integral part of a special issue.