Phyllosilicate controls on magnesium isotopic fractionation during weathering of granites: Implications for continental weathering and riverine system
نویسندگان
چکیده
Continental weathering is a fundamental process in releasing magnesium (Mg) from crystalline rocks to the hydrosphere and biosphere. Mg isotopes can be substantially mobilized, re-distributed, fractionated during weathering, therefore used as powerful tool trace biogeochemical cycle of Mg. Causes significant isotopic fractionation behaviors silicate are still not well understood, hindering further application probe different geological processes. In this study, we demonstrate that dissolution formation phyllosilicates main control sub-tropical granite. Furthermore, mechanisms for same mineral phase could also cause variations magnitude directionality fractionation. incipient supergene form mainly through topotactic transformation. Vermiculitization parental chlorite tends release 24Mg causes 26Mg enrichment saprock. an advanced stage compositions more influenced by interaction with soil solutions. Minerals formed dissolution-precipitation mechanism neoformed dominantly sourced contemporary would firstly incorporated into phyllosilicates, such vermiculite, interstratified biotite/vermiculite chlorite/vermiculite. Therefore, solutions became enriched depth pedolith, which relatively 24Mg-rich form. However, saprolite, precipitation illite may have preferentially scavenged 24Mg, enriching 26Mg. Varying relative abundances phyllosilicate minerals along profile large regolith. Our study shows composition slightly weathered materials significantly heavy. Hence, entrainment 26Mg-rich but alternative explain high ?26Mg recorded some sedimentary rocks, especially aeolian source. Whereas low widely archived groundwater river water alternatively explained saprock scavenging transformation, instead severe depletion due intense vast secondary minerals, previously suggested. Comprehensive characterization processes resultant products essential interpret observed
منابع مشابه
The Mg isotopic systematics of granitoids in continental arcs and implications for the role of chemical weathering in crust formation.
Continental crust is too Si-rich and Mg-poor to derive directly from mantle melting, which generates basaltic rather than felsic magmas. Converting basalt to more felsic compositions requires a second step involving Mg loss, which is thought to be dominated by internal igneous differentiation. However, igneous differentiation alone may not be able to generate granites, the most silicic endmembe...
متن کاملMineralogical Controls on Cold Desert Weathering
Copyright and Moral Rights for the articles on this site are retained by the individual authors and/or other copyright owners. For more information on Open Research Online's data policy on reuse of materials please consult the policies page.
متن کاملSerpentinite Weathering and Implications for Mars
Introduction: In the search for life on Mars nearsurface soil environments may be important habitats for life accessible to future missions. Serpentinite rocks have been documented on Mars [1], as well as other clay minerals including smectite and kaolinites [2, 3]. Previous studies of soils formed on serpentinites on Earth have documented the formation of extensive clays, including smectite [4...
متن کاملGeochemistry of the Paleocene Sediments from SW Ahar: Implications for Provenance, Tectonics and Source Rock Weathering
The mineralogy and geochemistry of Paleocene shales and interbedded siltstones in the southwestern of Ahar town (NW Iran) were studied by optical microscopy, XRD, SEM, XRF, and ICP-MS techniques. The mineralogical composition, mainly characterized by calcite, quartz, feldspar, dolomite, muscovite, magnesiohornblende, chlorite, illite, montmorionite, palygorskite, and koninckite, suggests relati...
متن کاملChemical Weathering Trends from Tir Spectral Models: Implications for Deriving Weathering Trends from Martian Spectral Data
Introduction: Chemical weathering and petrologic trends of the martian surface have been estimated from thermal infrared (TIR) spectral models from the Thermal Emission Spectrometer (TES) and Mini-TES on the Spirit and Opportunity rovers [1,2]. Interpretations of chemical data from APXS on the MER rovers and TIR data from TES and the Thermal Emission Imaging System (THEMIS) suggest planet-wide ...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Earth and Planetary Science Letters
سال: 2021
ISSN: ['1385-013X', '0012-821X']
DOI: https://doi.org/10.1016/j.epsl.2020.116613