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10404 results for: ‘蓝色通用机械类企业站织梦模板✅项目合作 二开均可 TG:saolei44✅.yXMqrBYgqRaznzm’

  • 29th April 2013 Sol 260

    Posted by jbridges in Mars Science Laboratory Blog on April 29, 2013 Mars is not out of conjunction yet, so, we are only getting short, small data volumes of communication from Curiosity.

  • 13th November 2013 Sol 453

    Posted by jbridges in Mars Science Laboratory Blog on November 13, 2013 We have restarted science operations again after the software upload taking longer than expected.

  • 15th May 2014 Sol 630

    Posted by jbridges in Mars Science Laboratory Blog on May 15, 2014 As you can see from this NavCam image we are now driving away from Mt Remarkable.

  • 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.

  • 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.

  • Doug Gregg

    The academic profile of Doug Gregg, PhD Researcher at University of Leicester

  • Wednesday 14th Nov 2012 Sol 98

    Posted by jbridges in Mars Science Laboratory Blog on November 14, 2012 With its APXS (Alpha Particle X-ray Spectrometer) instrument on the robotic arm of Curiosity is measuring the composition of rocks and soil at Rocknest.

  • Daqi Liu

    The academic profile of Dr Daqi Liu, Lecturer at University of Leicester

  • 14th July 2014 Sol 688

    Posted by jbridges in Mars Science Laboratory Blog on July 14, 2014 In addition to driving towards the Murray Buttes gap in the dunes, and our path onto Mt. Sharp, we stop sometimes to do contact science.  The image gives an example of what this entails.

  • 14th October 2013 Sol 424

    Posted by jbridges in Mars Science Laboratory Blog on October 14, 2013 The noon to pre-dawn temperature variation at Gale Crater can be up to 90 degrees centigrade.   This MastCam image shows the effects of this extreme temperature variation.

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