Schwenzer, S. P.; Abramov, O. and Kring, D. A.
|Google Scholar:||Look up in Google Scholar|
Impact-generated hydrothermal systems on the Noachian surface of Mars are implicated by morphological and chemical evidence for (hot) water activity. The mechanics of their emplacement and evolution are well understood and thermochemical models (see our accompanying abstract) help constrain the formation conditions of sheet silicates and other alteration minerals. In this report we explore the paths of water through those systems over the periods (103 to >106 yrs) they were actively driving fluid flow through Mars’ crust.
|Item Type:||Conference Item|
|Copyright Holders:||2009 The Authors|
|Keywords:||impact generated hydrothermal systems; Mars; phyllosilicates; Noachian|
|Academic Unit/School:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Environment, Earth and Ecosystem Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Susanne Schwenzer|
|Date Deposited:||18 Nov 2010 11:28|
|Last Modified:||29 Nov 2016 17:11|
|Share this page:|