1. The 2004 Mars Exploration Rover Mission Evidence for Water and Prospects for Life Produced by and for the Hot Science – Cool Talks Outreach Lecture Series of the Environmental Science Institute. We request that the use of any of these materials include an acknowledgement of Dr. John Grotzinger, and the Hot Science – Cool Talks Outreach Lecture Series of the Environmental Science Institute of the University of Texas at Austin. We hope you find these materials educational and enjoyable. Dr. John Grotzinger Hot Science - Cool Talks Volume 38

2. The 2004 Mars Exploration Rover Mission: Evidence for Water and Prospects for Life John Grotzinger on behalf of MER Athena Science Team

3. Mars Science Strategy Common Thread Mars Science Strategy: Follow the Water! LIFE CLIMATE GEOLOGY HUMAN

4. The Athena Science Payload Remote Sensing Package Pancam Mast Assembly (PMA) Pancam Mini-TES In-Situ Package Instrument Deployment Device (IDD) Microscopic Imager Alpha Particle X-Ray Spectrometer Mössbauer Spectrometer Rock Abrasion Tool Magnetic Properties Experiment

5. The Team

6. Mars Pathfinder

7. The MER Rover

8. Wrap it up and cram it in… Wrap it up and cram it in……

9. The Three Challenging Mission Phases The Three Challenging Mission Phases Launch & Cruise Entry, Descent & Landing Egress & Surface Operations

10. Video by Dan Mass

11. Opportunity at Meridiani Planum Meridiani Gusev 2000 km

12. Hematite: Mineralogic Beacon Hematite Distribution Map from Tes Data 5oN5oN 6oS6oS 10 o W 0 02oE2oE 15% hematite0% (Figure based on Christensen et al., (2001) JGR, v. 106(E10), Plate 2, p.23,877.)

13. Meridiani Landing Site

14. Hole in One Eagle Crater

15. Backshell and Parachute

16. You are here

17. A Martian Eclipse

18. Short-Timescale Temperature Excursions Red = hot Purple = cold Red to purple is 2 K (degrees Kelvin) Largest temperature variations confined to lowest 100 meters or so Appears that temperature perturbations propagate upward Minutes past 1000 hours (sol 12) 212223252726242928 0 0.6 0.4 0.2 1 0.8 Height Above Surface (km)

19. Dust Devils

20. Opportunity: View from Lander Spirit: View from Lander 5 metres

21. The first rock investigated by Opportunity

22. Schematic representation of the Mössbauer Spectrometer

23. Mössbauer Spectrum of El Capitan Mössbauer Spectrum of El Capitan: Meridiani Planum Jarosite: (K, Na, X +1 )Fe 3 (SO 4 ) (OH) 6

24. Rio Tinto, Spain Andy Knoll

25. Spherules 5 mm

26. The “Berry Bowl”

27. Mössbauer on the Berry Bowl

28. Sediment Bedforms Sediment Bedforms ( e.g. Ripples )

29. Ancient Terrestrial Ripples Ancient Terrestrial Ripples: 1.4 Billion Years Old

30. Ripple Cross-Bedding in 3-D Ripple Cross-Bedding in 3D

31. Bedforms in Flowing Water Southard and Bouchwal,1990 Antidunes Upper Plane Beds Dunes No Sediment Movement Ripples V. Fine SandV. Coarse Sand Lower Plane Beds Median grain diameter (mm) Mean flow velocity (m sec -1 ) 0.1 0.51.02.0 0.2 2.0 1.0 0.6

32. Current Ripples in Water Flume experiments by Dave Rubin and Jon Nelson, USGS 6 hours of ripple migration Image is 60x40 cm

33. Current Ripples in Cross Section Simulation by Dave Rubin, USGS

34. Festoon Cross-Bedding on Earth

35. Festoon Cross-Bedding on Mars

36. Burns formation 2.0 m Burns formation (Endurance crater)

37. Burns Stratigraphy m 6 5 4 3 2 1 7 Lower Unit Interdune/Playa Festoon Cross-lamination Wavy Bedding Translatent Strata Whatanga Contact Zone of Recrystallization Capillary Fringe of Water Table? Eolian Sand Sheet Translatent Strata Low-Angle Strata Wellington Contact Deflation Surface Water Table Controlled? Eolian Dune Field Cross-Bedded Sandstone

38. Modern Sand Dunes on Mars ~ 50 cm

39. Interdu ne Surfac e Interdune Surface

40. Interdune Deflation Surface

41. Modern Mars Analog Modern Mars Analog: Um Asamin

42. Formation of evaporite salts

43. Modern Interdune Depression

44. Endurance Chemostratigraphy ~ 50 cm

45. Ratio to surface rock average Depth in crater

46. Changes Down Section: Texture OntarioDiamond Jenness

47. Meridiani environment appears to have been acidic, hypersaline, and only intermittently wet. Life exists at such extremes on Earth. But Meridiani data suggest potential challenges to origin as well as persistence of life. Rio Tinto Extremophiles Andy Knoll

48. Evidence of any life that might have existed might well be preserved in chemical sediments and concretions. Chemical and textural details of Meridiani salts and iron oxides likely to reveal much about environmental history. The Good News All this favors Meridiani Planum as a target for sample return. Andy Knoll

49. Summary Rovers have: –Operated for over 1200 days –Returned over 100,000 images –Analyzed dozens of rocks and soils

50. Summary Evidence for water: –Mössbauer detection of jarosite –Crystal molds, concretions, diagenesis –Festoon ripple cross-bedding –Stratigraphic succession of environments

51. Summary Prospects for Life: –Preservation potential is good –But did life originate under such extreme conditions?

52. Dr. John Grotzinger Fletcher Jones Professor of Geology California Institute of Technology John Grotzinger is a field geologist interested in the co-evolution of surficial environments and life on Earth and Mars. His research addresses the chemical development of the early oceans and atmosphere, and the environmental context of early evolution. Field mapping studies are the starting point for more topical laboratory-based studies involving geochemical, paleontological, and geochronological techniques. Currently, his research is focused on the reconstruction of environmental conditions associated with the Cambrian radiation of animals in Oman, Namibia and Siberia. In 2004, he served as a member of both the Geology and Long Term Planning Groups for the Mars Exploration Rover mission.