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  • Leicester scientists develop new imaging system for worlds largest gamma ray observatory

    Richard White (MPIK), Duncan Ross (UoL), Jon Lapington (UoL) Image credit Richard White, Max Planck Institute for Nuclear Physics in Heidelberg (MPIK) Scientists from the University's Space Research Centre have returned from the inauguration of the Gamma-ray Cherenkov...

  • 4th September 2015 Sol 1094

    Posted by jbridges in Mars Science Laboratory Blog on September 4, 2015 This NavCam mosaic shows the Williams outcrop in front of us, which is part of the Stimson unit.

  • 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.

  • 27th October 2014 Sol 791

    Posted by jbridges in Mars Science Laboratory Blog on October 27, 2014 You can see from the inset on this map that we have started driving again, south towards the higher ground, though in small distances compared to some of the long ~100 m drives we did earlier in the mission.

  • 1st April 2014 Sol 587

    Posted by jbridges in Mars Science Laboratory Blog on April 1, 2014 We have continued with contact science at the Square Top outcrop, with its characteristic striated upper surface, before we drive up to the Kimberley location.

  • 1st December 2014 Sol 825

    Posted by jbridges in Mars Science Laboratory Blog on December 1, 2014 This NavCam image shows a dusty view of Mt Sharp and its layers.  It is a sign that we are very close to summer solstice again.

  • 13th June 2016 Sol 1370

    Posted by jbridges in Mars Science Laboratory Blog on June 13, 2016 Here is the Oudam drillhole and the nearby dump piles for material that has been analysed by CheMin.

  • 29th November 2016 Sol 1534

    Posted by jbridges in Mars Science Laboratory Blog on November 29, 2016 We have started our 19th drill or scoop.  Curiosity now aims to drill at regular elevation intervals (25 m) as we progress up through the Murray formation.

  • Tuesday 25th September Sol 49

    Posted by jbridges in Mars Science Laboratory Blog on September 25, 2012 We are now getting a combination of the high resolution MAHLI images, APXS and ChemCam compositional data and the other camera images.

  • 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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