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13913 results for: ‘museum studies’

  • 24th February 2017 – Sol 1620

    Posted by jbridges in Mars Science Laboratory Blog on February 24, 2017 We have been examining Ireson Hill and found this unusual 10-15 cm diameter rock- called Passagassawakakeag ! The shape is an almost perfect Dreikanter.

  • Saturday 5th August Landing Sequence

    Posted by jbridges in Mars Science Laboratory Blog on August 6, 2012 Nominal tones received from MSL. Target location estimated 230 m from centre of ellipse in current trajectory. 10.25 pm Atmospheric entry has occurred.  Now 7 minutes to go. Getting very quiet in the room.

  • Saturday 5th August Landing Sequence

    Posted by jbridges in Mars Science Laboratory Blog on August 6, 2012 10.15 pm. Cruise stage separation successful. Spin down of the aeroshell successful. Nominal ‘heartbeat’ tones from Curiosity. 5.4 km/s and speeding up 6 minutes from atmospheric entry.

  • 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.

  • 23rd February 2015 Sol 907

    Posted by jbridges in Mars Science Laboratory Blog on February 23, 2015 Our next drill target is Telegraph_Peak.

  • 11th May 2016 Sol 1337

    Posted by jbridges in Mars Science Laboratory Blog on May 11, 2016 Sol 1337 means that we have just reached our second martian year since landing in 2012,  Here is a birthday cake to the mission from the ChemCam team in Toulouse.

  • 19th July 2016 Sol 1405

    Posted by jbridges in Mars Science Laboratory Blog on July 19, 2016 MSL is back and working as normal. This MastCam picture shows that even at this early stage of the dust season (ls = 190 ie we haven’t reached perihelion of Mars orbit yet) the crater rim is becoming obscured.

  • 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.

  • 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).

  • 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...

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