25th September 2013 Sol 404

We have now left Waypoint Point 1 and started out for Waypoint 2, at about 1 km distance. 

At Leicester University and the Open University (Dr Susanne Schwenzer) we are busy preparing a paper which uses a variety of ChemCam, CheMin, APXS data to work out the processes and conditions (T, fluid composition, pH etc.) that the alteration minerals at Yellowknife Bay experienced.  Its a big challenge but fascinating.  By knowing the thermodynamic properties of the minerals we can backtrack though modelling and terrestrial analogues to what went on with water in Gale Crater about 4 Gyr.  The calculated fluids can then be used to understand other secondary assemblages that we encounter on the way to, and at, Mt. Sharp.

The image shows an example of  the minerals that would precipitate from a likely alteration fluid at a variety of water to rock ratios (W/R).  They are similar to the minerals identified in the Sheepbed mudstone of Yellowknife Bay.

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jbridges

About jbridges

This blog is a record of my experiences and work during the Mars Science Laboratory mission, from the preparation, landing on August 5th 2012 Pacific Time, and onwards... I will also post updates about our other Mars work on meteorites, ExoMars and new missions. You can also follow the planetary science activities with @LeicsPlanets Professor John Bridges, School of Physics and Astronomy

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