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  • 13th April 2015 Sol 955

    Posted by jbridges in Mars Science Laboratory Blog on April 13, 2015 We have left Garden City and are commencing a week of driving.  This also marks 10 km on the odometer, at up to 100 m a day we can travel quite quickly.

  • February 16th 2013 Sol 189

    Posted by jbridges in Mars Science Laboratory Blog on February 16, 2013 This image shows the row of 10 laser spots shot by ChemCam in the drill tailings.   This is one of our first analyses prior to the analysis of material by CheMin and SAM.

  • 6th November 2013 Sol 445

    Posted by jbridges in Mars Science Laboratory Blog on November 6, 2013 Curiosity is having a software upgrade this week, so no science operations. We are still at Cooperstown and thinking about the close up images of the outcrop layers.

  • 9th September 2016 Sol 1455

    Posted by jbridges in Mars Science Laboratory Blog on September 9, 2016 We are heading toward a new drill site at the base of one the the buttes.  These are the landforms that dominate the landscape at this point in the traverse – The Murray Buttes.

  • 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.

  • 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.

  • 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).

  • 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.

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