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NASA’s Exploration Plan: “Follow the Water” GEOLOGY LIFE CLIMATE Prepare for Human Exploration When Where Form Amount WATER NASA’s Strategy for Mars Exploration.

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Presentation on theme: "NASA’s Exploration Plan: “Follow the Water” GEOLOGY LIFE CLIMATE Prepare for Human Exploration When Where Form Amount WATER NASA’s Strategy for Mars Exploration."— Presentation transcript:

1 NASA’s Exploration Plan: “Follow the Water” GEOLOGY LIFE CLIMATE Prepare for Human Exploration When Where Form Amount WATER NASA’s Strategy for Mars Exploration

2 Mars Global Surveyor (1997-2006) Global topography (elevation) discovery of recent water-carved gullies First orbiter around Mars since Viking (mid- 1970’s) Recently lost after 10 years of successful operations.

3 Science Package

4 1997 Mars Global Surveyor (MGS) Mars Orbiter Laser Altimeter (MOLA) –Global 500 m resolution grid with < 1 m vertical resolution Mars Orbiter Camera (MOC) –Few-meter resolution camera –more than 120,000 released images Thermal Emission Spectrometer –Near-Infrared broadband spectrometer rock, ice, and atmosphere compositions thermal structure of the Martian surface

5 Pre-MGS Global Topography

6 MGS Topography

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8 2011 Mars Science Laboratory

9 2011 MSL Key Goals Characterize a site that: –was a habitable environment. What does this mean? –is likely to have preserved biosignatures. –can be related to the “Big Picture”.

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11 Let’s watch it now!

12 2009 Mars Science Laboratory

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14 Keeping in Mind the Key MSL Goals… Characterize a site that: –was a habitable environment. What does this mean? –is likely to have preserved biosignatures. –can be related to the “Big Picture”.

15 VL1 MPF MER-B VL2 MER-A 2007 Phoenix Where would you land a $2.3B spacecraft?

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19 But how can we assess the engineering and safety of the landing sites??

20 GIS to the rescue!

21 Four Finalist Candidate Landing Sites Eberswalde Crater (24°S, 327°E, -1.5 km) contains a clay-bearing delta formed when an ancient river deposited sediment, possibly into a lake. Gale Crater (4.5°S, 137°E, -4.5 km) contains a 5-km sequence of layers that vary from clay-rich materials near the bottom to sulfates at higher elevation. Mawrth Vallis (24°N, 341°E, -2.2 km) exposes layers within Mars’ surface with differing mineralogy, including at least two kinds of clays. Holden Crater (26°S, 325°E, -1.9 km) has alluvial fans, flood deposits, possible lake beds, and clay- rich sediment.

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