The Open UniversitySkip to content
 

Impact-generated hydrothermal systems on Noachian Mars: the path of water

Schwenzer, S. P.; Abramov, O. and Kring, D. A. (2009). Impact-generated hydrothermal systems on Noachian Mars: the path of water. In: 40th Lunar and Planetary Science Conference, 23-27 Mar 2009, Houston, TX, USA.

URL: http://www.lpi.usra.edu/meetings/lpsc2009/pdf/2328...
Google Scholar: Look up in Google Scholar

Abstract

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/Department: Science > Physical Sciences
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
Item ID: 24294
Depositing User: Susanne Schwenzer
Date Deposited: 18 Nov 2010 11:28
Last Modified: 16 Nov 2012 12:27
URI: http://oro.open.ac.uk/id/eprint/24294
Share this page:

Actions (login may be required)

View Item
Report issue / request change

Policies | Disclaimer

© The Open University   + 44 (0)870 333 4340   general-enquiries@open.ac.uk