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  • Andrew Dunn: Page 15

    Academic Librarian.

  • 25th July 2013 Sol 344

    Posted by jbridges in Mars Science Laboratory Blog on July 25, 2013 This HiRISE image shows Curiosity at work at the Shaler outcrop in Yellowknife Bay. The tracks from Bradbury landing are also clearly visible.

  • 2nd October 2013 Sol 411

    Posted by jbridges in Mars Science Laboratory Blog on October 2, 2013 Mars Science Laboratory is having a team meeting at the California Institute of Technology (Caltech) in Pasadena, California.

  • 4th October 2016 Sol 1480

    Posted by jbridges in Mars Science Laboratory Blog on October 4, 2016 This MAHLI mosaic view of Curiosity and Murray Butte no. 12 is where we have just been drilling Quela – the 14th drillhole on Mars.

  • 17th July 2015 Sol 1047

    Posted by jbridges in Mars Science Laboratory Blog on July 17, 2015 The science team is considering the next drill target. ChemCam and APXS results suggest that the sediment compositions are changing within the Murray Formation, with more altered compositions.

  • 13th November 2015 Sol 1164

    Posted by jbridges in Mars Science Laboratory Blog on November 13, 2015 We are nearing the next major phase of the mission – the Bagnold Dunes campaign.

  • 23rd September 2013 Sol 402

    Posted by jbridges in Mars Science Laboratory Blog on September 23, 2013 This image shows the arm deployed over the conglomerate and veins as we gather more MAHLI data.  The shadow from the arm shows how we are operating at near noon, local time at Gale Crater.

  • 28th December 2015 Sol 1206

    Posted by jbridges in Mars Science Laboratory Blog on December 28, 2015 The MSL team is taking a break from operations for a few days.  We have dumped the Greenhorn drill tailings and are progressing on the Bagnold Dunes campaign.

  • 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).

  • 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).

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