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  • 9th May 2016 Sol 1336

    Posted by jbridges in Mars Science Laboratory Blog on May 9, 2016 We have followed up the Lubango drillhole quickly with another one at a nearby Stimson aeolian sandstone outcrop (Okoruso).  The idea is to compare unaltered sandstone (Okoruso) to altered Lubango.

  • 15th February 2016 Sol 1254

    Posted by jbridges in Mars Science Laboratory Blog on February 15, 2016 We have now started driving away from the main Namib dunes, and onto the Naukluft Plateau.

  • How to Sell Success, Failure and Fanaticism? Understand the Customer!

    Posted by Georgios Patsiaouras in School of Business Blog on June 2, 2014 Georgios Patsiaouras, Lecturer in Marketing and Consumption at the School, draws sobering lessons from the popularity of the recent Hollywood Blockbuster, The Wolf of Wall Street.

  • Introducing SKYLARK

    Posted by Physics & Astronomy in Physics and Astronomy Blog on 26 October 2020 The SKYLARK rocket dominates our newly-revamped foyer in the School of Physics and Astronomy. This blog post provides some of the history of Leicester’s involvement in the SKYLARK project.

  • jbridges: Page 15

    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.

  • 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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