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  • 5th August 2014 Sol 710

    Posted by jbridges in Mars Science Laboratory Blog on August 5, 2014 We are moving into a new sort of terrain as we enter Hidden Valley.  On this HiRISE image and the inset MAHLI image you can see the sand ripples that we are traversing.

  • 15th August 2014 Sol 720

    Posted by jbridges in Mars Science Laboratory Blog on August 15, 2014 We have retraced our tracks in Hidden Valley, going back to a site called Bonanza_King.

  • Sol 0 Monday 6th August

    Posted by jbridges in Mars Science Laboratory Blog on August 6, 2012 The next data relay via Mars Odyssey is at 12.30 am PDT (add 8 hours for BST). We will start the process of checking the instruments.

  • Monday 10th December Sol 123

    Posted by jbridges in Mars Science Laboratory Blog on December 10, 2012 Here is a Mastcam image of the new terrain we are exploring.  You can see layered deposits in the middle distance and a flat eroded surface in the near field.

  • 3rd May 2013 Sol 263

    Posted by jbridges in Mars Science Laboratory Blog on May 3, 2013 Our first image has come back after conjunction.  Here is the Chemcam remote microimager (RMI) of our titanium calibration target.

  • 1st August 2013 Sol 351

    Posted by jbridges in Mars Science Laboratory Blog on August 1, 2013 We have moved from southern summer into southern autumn (northern spring equinox).

  • 11th September 2014 Sol 746

    Posted by jbridges in Mars Science Laboratory Blog on September 11, 2014 We have now reached the first foothills in the Mt. Sharp part of the mission.  This area is called the Pahrump Hills.

  • 5th April 2017 Sol 1658

    Posted by jbridges in Mars Science Laboratory Blog on April 5, 2017 The second Bagnold Dunes campaign is now drawing to a close.

  • February 21st 2013 Sol 194

    Posted by jbridges in Mars Science Laboratory Blog on February 21, 2013 We are in the next stage of the drilling analysis process: the drilled sedimentary rock has been transferred to the scoop on the arm’s turret, prior to being taken into CHIMRA via the sieve, part of which...

  • 27th November 2015 Sol 1176

    Posted by jbridges in Mars Science Laboratory Blog on November 27, 2015 We have reached the Bagnold Dunes and are driving through a gap. The dark colour is due to the iron and magnesium-rich composition  of the sand grains (minerals like olivine and pyroxene).

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