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10.1098/rsta.2013.0240 http://scihub22266oqcxt.onion/10.1098/rsta.2013.0240 C4128263!4128263!25114310     free     free     free Deprecated: Implicit conversion from float 213.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 213.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 213.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534       Philos+Trans+A+Math+Phys+Eng+Sci 2014 ; 372 (2024): ä Nephropedia Template TP {{tp|p=25114310|t=2014. Contraction or expansion of the Moon s crust during magma ocean freezing?|pdf=|usr=}}{{25114310}} gab.com Text Contraction or expansion of the Moon s crust during magma ocean freezing JO: Philos Trans A Math Phys Eng Sci http://www.kidney.de/pget.php?&tw=1&pmid=25114310 #FOAvip The lack of contraction features on the Moon has been used to argue that the Moon underwent limited secular cooling, and thus had a relatively cool initial state. A cool early state in turn limits the depth of the lunar magma ocean. Recent GRAIL gravity measurements, however, suggest that dikes were emplaced in the lower crust, requiring global lunar expansion. Starting from the magma ocean state, we show that solidification of the lunar magma ocean would most likely result in expansion of the young lunar crust, and that viscous relaxation of the crust would prevent early tectonic features of contraction or expansion from being recorded permanently. The most likely process for creating the expansion recorded by the dikes is melting during cumulate overturn of the newly solidified lunar mantle. Twit Text FOAVip Contraction or expansion of the Moon s crust during magma ocean freezing ????Philos Trans A Math Phys Eng Sci http://www.kidney.de/pget.php?&tw=1&pmid=25114310 #FOAvip Twit Text # Free Paper on # # # # # LINK http://www.kidney.de/pget.php?&tw=1&pmid=25114310 #FOAvip English Wikipedia <ref>{{Cite pmid|25114310}}</ref> Contraction or expansion of the Moon s crust during magma ocean freezing? #MMPMID25114310 Elkins-Tanton LT; Bercovici D Philos Trans A Math Phys Eng Sci 2014[Sep]; 372 (2024): ä PMID25114310show ga The lack of contraction features on the Moon has been used to argue that the Moon underwent limited secular cooling, and thus had a relatively cool initial state. A cool early state in turn limits the depth of the lunar magma ocean. Recent GRAIL gravity measurements, however, suggest that dikes were emplaced in the lower crust, requiring global lunar expansion. Starting from the magma ocean state, we show that solidification of the lunar magma ocean would most likely result in expansion of the young lunar crust, and that viscous relaxation of the crust would prevent early tectonic features of contraction or expansion from being recorded permanently. The most likely process for creating the expansion recorded by the dikes is melting during cumulate overturn of the newly solidified lunar mantle. äContraction or expansion of the Moon s crust during magma ocean freezi(epmc).pdf DeepDyve Pubget Overpricing