Search

16061 results for: ‘金秋十月美图v1.0织梦dede图片站模板整站源码 数据✅项目合作 二开均可 TG:saolei44✅.urNRlGmLxgKS’

  • Tuesday 20th Nov. Sol 104

    Posted by jbridges in Mars Science Laboratory Blog on November 20, 2012 We have moved from Rocknest where our analyses of soil, rocks and atmosphere are complete.  We have a lot of data to examine.

  • Friday 31st August Sol 25

    Posted by jbridges in Mars Science Laboratory Blog on August 31, 2012 We now have a weather report for Gale Crater courtesy of the REM instrument.

  • Research Methods in Cell Biology

    Module code: MB7002 When a gene is found to be mutated in a cancer we first need to understand how its protein product functions and then how the protein produced by the mutant gene alters the behaviour of cancer cells.

  • Research Methods in Cell Biology

    Module code: BS4002 When a gene is found to be mutated in a cancer we first need to understand how its protein product functions and then how the protein produced by the mutant gene alters the behaviour of cancer cells.

  • Sunday August 19th Sol 14

    Posted by jbridges in Mars Science Laboratory Blog on August 20, 2012 Excellent ChemCam  LIBS (Laser Induced Breakdown Spectroscopy Results) on our first rock.  This means that in addition to imaging data from MastCam we are now getting compositional data.

  • 22nd March 2018 Sol 2000

    MSL

  • 25th April 2014 Sol 611

    Posted by jbridges in Mars Science Laboratory Blog on April 25, 2014 Here is the chosen drill site – Windjana (named after a famous set of rocks in W. Australia which show ancient paintings).

  • Every breath you take...

    Professor Paul Monks explores air pollution and its impact on human health and the climate.

  • Thursday 4th October Sol 58

    Posted by jbridges in Mars Science Laboratory Blog on October 5, 2012   Previous missions suggest that the ‘soil’ on Mars is roughly basaltic in composition.  However, on Earth sand is mainly composed of quartz (silica).

  • Thursday 6th September Sol 30

    Posted by jbridges in Mars Science Laboratory Blog on September 6, 2012 Telescopes on Earth need to measure ‘flat’ and ‘dark’ frames with every set of observations in order to correct for distortions on the telescope mirror and any false detections on the light detector.

Back to top
MENU