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10.1002/2014JE004757 http://scihub22266oqcxt.onion/10.1002/2014JE004757 C4508961!4508961!26213668     free     free     free Warning: file_get_contents(https://eutils.ncbi.nlm.nih.gov/entrez/eutils/elink.fcgi?dbfrom=pubmed&id=26213668&cmd=llinks): Failed to open stream: HTTP request failed! HTTP/1.1 429 Too Many Requests in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 215 Deprecated: Implicit conversion from float 211.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534       J+Geophys+Res+Planets 2015 ; 120 (1): 1-19 Nephropedia Template TP {{tp|p=26213668|t=2015. Diagenesis and clay mineral formation at Gale Crater, Mars |pdf=|usr=}}{{26213668}} gab.com Text Diagenesis and clay mineral formation at Gale Crater, Mars JO: J Geophys Res Planets http://www.kidney.de/pget.php?&tw=1&pmid=26213668 #FOAvip The Mars Science Laboratory rover Curiosity found host rocks of basaltic composition and alteration assemblages containing clay minerals at Yellowknife Bay, Gale Crater. On the basis of the observed host rock and alteration minerals, we present results of equilibrium thermochemical modeling of the Sheepbed mudstones of Yellowknife Bay in order to constrain the formation conditions of its secondary mineral assemblage. Building on conclusions from sedimentary observations by the Mars Science Laboratory team, we assume diagenetic, in situ alteration. The modeling shows that the mineral assemblage formed by the reaction of a CO2-poor and oxidizing, dilute aqueous solution (Gale Portage Water) in an open system with the Fe-rich basaltic-composition sedimentary rocks at 10?50°C and water/rock ratio (mass of rock reacted with the starting fluid) of 100?1000, pH of ?7.5?12. Model alteration assemblages predominantly contain phyllosilicates (Fe-smectite, chlorite), the bulk composition of a mixture of which is close to that of saponite inferred from Chemistry and Mineralogy data and to that of saponite observed in the nakhlite Martian meteorites and terrestrial analogues. To match the observed clay mineral chemistry, inhomogeneous dissolution dominated by the amorphous phase and olivine is required. We therefore deduce a dissolving composition of approximately 70% amorphous material, with 20% olivine, and 10% whole rock component. Twit Text FOAVip Diagenesis and clay mineral formation at Gale Crater, Mars ????J Geophys Res Planets http://www.kidney.de/pget.php?&tw=1&pmid=26213668 #FOAvip Twit Text # Free Paper on # # # # # LINK http://www.kidney.de/pget.php?&tw=1&pmid=26213668 #FOAvip English Wikipedia <ref>{{Cite pmid|26213668}}</ref> Diagenesis and clay mineral formation at Gale Crater, Mars #MMPMID26213668 Bridges JC; Schwenzer SP; Leveille R; Westall F; Wiens RC; Mangold N; Bristow T; Edwards P; Berger G J Geophys Res Planets 2015[Jan]; 120 (1): 1-19 PMID26213668show ga The Mars Science Laboratory rover Curiosity found host rocks of basaltic composition and alteration assemblages containing clay minerals at Yellowknife Bay, Gale Crater. On the basis of the observed host rock and alteration minerals, we present results of equilibrium thermochemical modeling of the Sheepbed mudstones of Yellowknife Bay in order to constrain the formation conditions of its secondary mineral assemblage. Building on conclusions from sedimentary observations by the Mars Science Laboratory team, we assume diagenetic, in situ alteration. The modeling shows that the mineral assemblage formed by the reaction of a CO2-poor and oxidizing, dilute aqueous solution (Gale Portage Water) in an open system with the Fe-rich basaltic-composition sedimentary rocks at 10?50°C and water/rock ratio (mass of rock reacted with the starting fluid) of 100?1000, pH of ?7.5?12. Model alteration assemblages predominantly contain phyllosilicates (Fe-smectite, chlorite), the bulk composition of a mixture of which is close to that of saponite inferred from Chemistry and Mineralogy data and to that of saponite observed in the nakhlite Martian meteorites and terrestrial analogues. To match the observed clay mineral chemistry, inhomogeneous dissolution dominated by the amorphous phase and olivine is required. We therefore deduce a dissolving composition of approximately 70% amorphous material, with 20% olivine, and 10% whole rock component. äDiagenesis and clay mineral formation at Gale Crater, Mars (epmc).pdf DeepDyve Pubget Overpricing