1st October 2015 Sol 1121

Our latest drillhole has gone successfully, at Big Sky.  We will compare the compositional and X-ray diffraction data mineral data to that of the Buckskin drillhole  to try and understand the unusual silica enrichments. Are we looking at compositions not unlike terrestrial sandstones formed by erosion of a differentiated crust, or is the composition dominated by the alteration of basaltic composition sediments – which releases silica?Identifying the different types of silica (SiO2) minerals that form at characteristic temperatures will help resolve this when combined with all the Curiosity imagery.

This week at the European Planetary Science Congress in Nantes, France, we are discussing many of the Curiosity results including alteration of the Gale sediments by groundwaters.

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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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