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10.1038/srep43177 http://scihub22266oqcxt.onion/10.1038/srep43177 C5324095!5324095!28233797     free     free     free Deprecated: Implicit conversion from float 231.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 231.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 231.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534       Sci+Rep 2017 ; 7 (ä): ä Nephropedia Template TP {{tp|p=28233797|t=2017. A record of igneous evolution in Elysium, a major martian volcanic province |pdf=|usr=}}{{28233797}} gab.com Text A record of igneous evolution in Elysium, a major martian volcanic province JO: Sci Rep http://www.kidney.de/pget.php?&tw=1&pmid=28233797 #FOAvip A major knowledge gap exists on how eruptive compositions of a single martian volcanic province change over time. Here we seek to fill that gap by assessing the compositional evolution of Elysium, a major martian volcanic province. A unique geochemical signature overlaps with the southeastern flows of this volcano, which provides the context for this study of variability of martian magmatism. The southeastern lava fields of Elysium Planitia show distinct chemistry in the shallow subsurface (down to several decimeters) relative to the rest of the martian mid-to-low latitudes (average crust) and flows in northwest Elysium. By impact crater counting chronology we estimated the age of the southeastern province to be 0.85?±?0.08?Ga younger than the northwestern fields. This study of the geochemical and temporal differences between the NW and SE Elysium lava fields is the first to demonstrate compositional variation within a single volcanic province on Mars. We interpret the geochemical and temporal differences between the SE and NW lava fields to be consistent with primary magmatic processes, such as mantle heterogeneity or change in depth of melt formation within the martian mantle due to crustal loading. Twit Text FOAVip A record of igneous evolution in Elysium, a major martian volcanic province ????Sci Rep http://www.kidney.de/pget.php?&tw=1&pmid=28233797 #FOAvip Twit Text # Free Paper on # # # # # LINK http://www.kidney.de/pget.php?&tw=1&pmid=28233797 #FOAvip English Wikipedia <ref>{{Cite pmid|28233797}}</ref> A record of igneous evolution in Elysium, a major martian volcanic province #MMPMID28233797 Susko D; Karunatillake S; Kodikara G; Skok JR; Wray J; Heldmann J; Cousin A; Judice T Sci Rep 2017[]; 7 (ä): ä PMID28233797show ga A major knowledge gap exists on how eruptive compositions of a single martian volcanic province change over time. Here we seek to fill that gap by assessing the compositional evolution of Elysium, a major martian volcanic province. A unique geochemical signature overlaps with the southeastern flows of this volcano, which provides the context for this study of variability of martian magmatism. The southeastern lava fields of Elysium Planitia show distinct chemistry in the shallow subsurface (down to several decimeters) relative to the rest of the martian mid-to-low latitudes (average crust) and flows in northwest Elysium. By impact crater counting chronology we estimated the age of the southeastern province to be 0.85?±?0.08?Ga younger than the northwestern fields. This study of the geochemical and temporal differences between the NW and SE Elysium lava fields is the first to demonstrate compositional variation within a single volcanic province on Mars. We interpret the geochemical and temporal differences between the SE and NW lava fields to be consistent with primary magmatic processes, such as mantle heterogeneity or change in depth of melt formation within the martian mantle due to crustal loading. äA record of igneous evolution in Elysium, a major martian volcanic pro(epmc).pdf DeepDyve Pubget Overpricing