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WET MARS SIGNED

Hydrological processes on late Mars: water under the telescope and under the microscope

Total Cost €

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EC-Contrib. €

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Partnership

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 WET MARS project word cloud

Explore the words cloud of the WET MARS project. It provides you a very rough idea of what is the project "WET MARS" about.

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Project "WET MARS" data sheet

The following table provides information about the project.

Coordinator
UNIVERSITEIT UTRECHT 

Organization address
address: HEIDELBERGLAAN 8
city: UTRECHT
postcode: 3584 CS
website: www.uu.nl

contact info
title: n.a.
name: n.a.
surname: n.a.
function: n.a.
email: n.a.
telephone: n.a.
fax: n.a.

 Coordinator Country Netherlands [NL]
 Total cost 165˙598 €
 EC max contribution 165˙598 € (100%)
 Programme 1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
 Code Call H2020-MSCA-IF-2017
 Funding Scheme MSCA-IF-EF-ST
 Starting year 2018
 Duration (year-month-day) from 2018-06-01   to  2020-05-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    UNIVERSITEIT UTRECHT NL (UTRECHT) coordinator 165˙598.00

Map

 Project objective

Mars displays clear evidence of water, having regions where water flowed at several times in its 4 billion years history.

The aim of this fellowship is to reconstruct paleo-hydrological conditions on late Mars (from 3Ga to date) and to recreate the hydrogeological cycle that created the complex channel systems found on Mars’ surface. The stream tables, the Earth Simulation Lab and numerical modelling at the UU will allow for the first time: 1) to simulate frozen Martian subsoil characteristic and conditions; 2) to seek out signature of melting ice as sources up front of Martian river systems; 3) to investigate together the role of thermal and mechanical erosion.

I will determine the lithological and fluid characteristics and their possible related deposits, water source triggering mechanisms, and will explain if it is by impact or spin axis / obliquity changes. High-resolution digital elevation modelling will be used to constrain hydrogeological parameters (under the telescope). Laboratory experiments and numerical modelling using a streamtable and an Earth Simulation Laboratory will support the core task (under the microscope). This research is urgently needed as it addresses key questions about past Martian habitability and its implications in subsurface degassing, potential landing site of future robotic/human missions and climate. The inter-disciplinary perspective adopted in this study, close integration of surface geology, analog modelling, and numerical modelling studies, will provide important new knowledge on the late Mars environment.

The Experienced Researcher (ER) will work in the world-leading “River and delta morphodynamics group” group in the Department of Physical Geography at Utrecht University. The ER is already proving himself as a future leader: he has published five peer-reviewed papers, and led international teams on fluvio-lacustrine features and climate conditions and erosion rates on early Mars.

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The information about "WET MARS" are provided by the European Opendata Portal: CORDIS opendata.

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