Wednesday 3rd October Sol 57

 

The
hazard cameras onboard Curiosity can give a valuable low angle view of the ground surface
in front of the rover.  Here we see the small
ridge of dust and sand that we will scoop for our imminent experiments.  Dust can be useful as well as a
nuisance.  Because it is fine grained it
has been blown over wide regions and thus homogenised its composition.  So when we analyse dusty soil we are getting an average crustal composition and set of minerals. That will  be a valuable addition to our knowledge of Mars and a good way of comparing to other planetary crusts, revealing any fluid processes that may have altered the martian crust over time.

 

We will also be analyzing the rocks surrounding the dust sampling area to determine their origin.

Share this page:

Share this page:

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

View more posts by jbridges

Subscribe to jbridges's posts

Leave a Reply

Network-wide options by YD - Freelance Wordpress Developer