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7001 results for: ‘婚恋交友系统|红娘相亲小程序源码✅项目合作 二开均可 TG:saolei44✅.SQtBRyZPWugaPF’

  • 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...

  • 6th July 2016 Sol 1392

    Posted by jbridges in Mars Science Laboratory Blog on July 6, 2016 No current  photos because MSL has gone into safe mode for the last few days due to a software glitch. That means we wont get images or much data back for a few days.

  • 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.

  • 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.

  • 4th March 2017 Sol 1627

    Posted by jbridges in Mars Science Laboratory Blog on March 4, 2017 We are continuing the Bagnold Dunes campaign, with  stops 3 and 4. This NavCam view shows the Curiosity robotic arm for the team’s examination.

  • 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.

  • 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).

  • DOCK businesses targeted for university-business collaborations

    As part of a drive to encourage collaborations between local innovation businesses and the University, the Enterprise and Business Development Office (EBDO) held a successful event at DOCK recently (29 June).

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