Mars Express Science Presentation - ESA M. MCCaughrean (PDF)

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Spectroscopy reveals the mineral SCIENCE AND ROBOTIC EXPLORATION composition Mars Science Laboratory landing event ESOC, Darmstadt, August 6, 2012 Debris aprons surrounding craters in southern highlands contain hydrated minerals formed at high temperatures (~100–300°C) in deep (few km) subsurface MEX OMEGA mapping in Tyrrhena Terra over Mars Odyssey IR images / Loizeau et al. 2012, Icarus / ESA, NASA 34
So, why Gale crater today? SCIENCE AND ROBOTIC EXPLORATION Mars Science Laboratory landing event ESOC, Darmstadt, August 6, 2012 Combined MEX HRSC, MRO Context Camera, and Viking data / NASA, ESA, DLR, FU Berlin (G. Neukum) 35
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Page 9 and 10: Mars exploration family portrait SC
Page 11 and 12: Mars Express spacecraft SCIENCE AND
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Page 17 and 18: The enigmatic martian moons SCIENCE
Page 27 and 28: 2 km Olympia Undae Probing below th
Page 29 and 30: 11 7 < 3 A short-lived polar ocean?
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Mars Express Science Presentation - ESA M. MCCaughrean (PDF)

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