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10.1098/rsta.2015.0391 http://scihub22266oqcxt.onion/10.1098/rsta.2015.0391 C5394255!5394255!28416727     free     free     free Deprecated: Implicit conversion from float 211.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 211.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 211.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534       Philos+Trans+A+Math+Phys+Eng+Sci 2017 ; 375 (2094): ä Nephropedia Template TP {{tp|p=28416727|t=2017. Remotely distinguishing and mapping endogenic water on the Moon |pdf=|usr=}}{{28416727}} gab.com Text Remotely distinguishing and mapping endogenic water on the Moon JO: Philos Trans A Math Phys Eng Sci http://www.kidney.de/pget.php?&tw=1&pmid=28416727 #FOAvip Water and/or hydroxyl detected remotely on the lunar surface originates from several sources: (i) comets and other exogenous debris; (ii) solar-wind implantation; (iii) the lunar interior. While each of these sources is interesting in its own right, distinguishing among them is critical for testing hypotheses for the origin and evolution of the Moon and our Solar System. Existing spacecraft observations are not of high enough spectral resolution to uniquely characterize the bonding energies of the hydroxyl molecules that have been detected. Nevertheless, the spatial distribution and associations of H, OH? or H2O with specific lunar lithologies provide some insight into the origin of lunar hydrous materials. The global distribution of OH?/H2O as detected using infrared spectroscopic measurements from orbit is here examined, with particular focus on regional geological features that exhibit OH?/H2O absorption band strengths that differ from their immediate surroundings.This article is part of the themed issue ?The origin, history and role of water in the evolution of the inner Solar System?. Twit Text FOAVip Remotely distinguishing and mapping endogenic water on the Moon ????Philos Trans A Math Phys Eng Sci http://www.kidney.de/pget.php?&tw=1&pmid=28416727 #FOAvip Twit Text # Free Paper on # # # # # LINK http://www.kidney.de/pget.php?&tw=1&pmid=28416727 #FOAvip English Wikipedia <ref>{{Cite pmid|28416727}}</ref> Remotely distinguishing and mapping endogenic water on the Moon #MMPMID28416727 Klima RL; Petro NE Philos Trans A Math Phys Eng Sci 2017[May]; 375 (2094): ä PMID28416727show ga Water and/or hydroxyl detected remotely on the lunar surface originates from several sources: (i) comets and other exogenous debris; (ii) solar-wind implantation; (iii) the lunar interior. While each of these sources is interesting in its own right, distinguishing among them is critical for testing hypotheses for the origin and evolution of the Moon and our Solar System. Existing spacecraft observations are not of high enough spectral resolution to uniquely characterize the bonding energies of the hydroxyl molecules that have been detected. Nevertheless, the spatial distribution and associations of H, OH? or H2O with specific lunar lithologies provide some insight into the origin of lunar hydrous materials. The global distribution of OH?/H2O as detected using infrared spectroscopic measurements from orbit is here examined, with particular focus on regional geological features that exhibit OH?/H2O absorption band strengths that differ from their immediate surroundings.This article is part of the themed issue ?The origin, history and role of water in the evolution of the inner Solar System?. äRemotely distinguishing and mapping endogenic water on the Moon (epmc).pdf DeepDyve Pubget Overpricing