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16008 results for: ‘苹果CMS首涂第30套可装修DIY主题模板免授权版✅项目合作 二开均可 TG:saolei44✅.ECSBgcuIHaE’

  • 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.

  • 29th October 2015 Sol 1148

    Posted by jbridges in Mars Science Laboratory Blog on October 29, 2015 We have completed another drill so that we now have the Big Sky and Greenhorn drill holes. As the team becomes more experienced we are getting quicker at producing drillholes and so we can get more analyses.

  • Thursday 29th November Sol 112

    Posted by jbridges in Mars Science Laboratory Blog on November 29, 2012 Our next major task is to select a suitable place for the first drilling operation using high resolution MastCam images that we have been taking.

  • 18th January 2015 Sol 872

    Posted by jbridges in Mars Science Laboratory Blog on January 18, 2015 Unlike Curiosity the Beagle2 lander never sent a signal back from Mars.  However, as a result of some new HiRISE images we now know where it is and what happened.

  • Publications

    Browse the publications published by and relating to the research undertaken by the Hopkinson Group in the School of Chemistry.

  • 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.

  • 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).

  • 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.

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