1. TRAVERSE ACROSS LOWER STRATA OF MERIDIANI PLANUM LAYERED DEPOSITS Alan D. Howard Department of Environmental Sciences University of Virginia Jeffrey M. Moore NASA Ames

2. General Concept We have explored only the top few meters of the >800 m thick stack of layered sediment in the Meridiani Planum region We have explored only the top few meters of the >800 m thick stack of layered sediment in the Meridiani Planum region These layered deposits have the greatest areal extent and the most informative regional context of all layered deposit sequences These layered deposits have the greatest areal extent and the most informative regional context of all layered deposit sequences We argue that these deposits accumulated as a sedimentary wedge at the edge of a large sea or ocean during the Noachian and are thus the most likely deposits to have incorporated organic compounds indicative of development of life We argue that these deposits accumulated as a sedimentary wedge at the edge of a large sea or ocean during the Noachian and are thus the most likely deposits to have incorporated organic compounds indicative of development of life

3. The Regional Context

4. A prominent topographic platform interrupts the northwestward slope of the gradual transition from highlands to lowlands It occurs at elevations from about 0 to -1600 m with a sharp drop off to about -2000 m We provisionally call this the Meridiani Bench

5. Arabia Lowlands Cratered Highlands M.B. The purple line encloses the Meridiani Bench and separates the Cratered Highlands from the Arabia Lowlands

6. MP The blue area is underlain by layered sediments of the Meridiani Planum portion of the Meridiani Bench. These layered sediments include the hematite-rich deposits being visited by the Opportunity Rover as well as sulfate-rich deposits. We suggest that the entire Meridiani Bench, including the Meridiani Planum deposits, are underlain by a sedimentary sequence of sediments eroded from the Cratered highlands extending into a former sea or ocean extending up to at least -1500 m

7. Prominent valley networks are shown in Cyan. They do not extend below about -1500 m White arrows show the ULM outflow channel system that formed subsequent to the landforms discussed here The possibility of a high-level ocean or sea in this region has also been suggested by Edgett and Parker [1997], Fairen et al. [2003], Fairen and Dohm [2004], and Clifford and Parker [2001]

8. A topographic barrier may have created semi- enclosed conditions that encouraged evaporite deposition as part of the Meridiani Planum sequence. Mawrth Valles may have been excavated by overflows/density flows over this barrier. Later outflow channel floods have breached this barrier.

9. We do not have the space or time here to develop the supporting evidence for our scenario, but a paper is in preparation We do not have the space or time here to develop the supporting evidence for our scenario, but a paper is in preparation Even if we are wrong, the presence of a thick sequence of layered deposits, hematite, hydrated minerals, and sufates warrants further exploration Even if we are wrong, the presence of a thick sequence of layered deposits, hematite, hydrated minerals, and sufates warrants further exploration Previous regional geologic investigations of the Meridiani region have been published by Hynek et al. [2002], Arvidson et al. [2003] and Edgett [2005]. Previous regional geologic investigations of the Meridiani region have been published by Hynek et al. [2002], Arvidson et al. [2003] and Edgett [2005]. Edgett compares the region to the terrestrial Colorado Plateau Edgett compares the region to the terrestrial Colorado Plateau

10. The Proposed Site The steep, 300-400 m scarp defining the northwestern edge of the Meridiani Planum/Meridiani Bench deposits exposes probably the most complete section of the lower portions of the sequence, complementing the examination of the higher beds by Opportunity The steep, 300-400 m scarp defining the northwestern edge of the Meridiani Planum/Meridiani Bench deposits exposes probably the most complete section of the lower portions of the sequence, complementing the examination of the higher beds by Opportunity We have suggested a site near 354°E and 8°N permitting a traverse across this scarp We have suggested a site near 354°E and 8°N permitting a traverse across this scarp

11. “X” marks the spot, the line is the NW scarp X

12. IR Mosaic of Landing Site Region & 3 proposed sites

13. The Geologic Context Hynek et al. [2001] and Edgett [2005] have provided geologic context Hynek et al. [2001] and Edgett [2005] have provided geologic context Two prominent units define the sedimentary sequence occurring here: Two prominent units define the sedimentary sequence occurring here: A lower set of beds which locally appears to incorporate fluvial channel deposits A lower set of beds which locally appears to incorporate fluvial channel deposits An upper sequence characterized by reticulate ridges of layered deposits An upper sequence characterized by reticulate ridges of layered deposits

14. (Edgett,2005) P=Plains-forming Unit R=Ridge-forming Unit S=Scarp Forming Unit L=Lower Unit X

15. (Hynek et al., 2002) Cs=Cratered, Subdued Cu=Cratered, Undivided IL=Interior Layered P1=Plains, Lower P2=Plains, Upper Ph=Plains, Middle P3=Etched X

16. Images of Region

17. 1 - E22004432 – E2200081

19. VIS mosaic showing locations of detailed MOC images

20. 1 R1601540 Scarp in lower layered unit – possibly traversable

21. 2 R1601540 In landing ellipse – somewhat scabby texture

22. 3 R1601540 Upper ridged unit – probably can be sampled at various levels

23. Landing site thermal intertias ~200, about the same as the Opportunity site

24. X Landing Site does not contain extensive exposures of hydrated minerals

25. A Possible Extended Mission Target The ~70 km crater about 20 km to the west of the landing site contains some of the best exposures of rhythmically-layered sediment on Mars The ~70 km crater about 20 km to the west of the landing site contains some of the best exposures of rhythmically-layered sediment on Mars The issue is feasibility of descending into the crater and traversing the rough floor The issue is feasibility of descending into the crater and traversing the rough floor

26. Landing Site Coordinates: L1: 354.029°E 7.900°N L2: 353.975°E 8.260°N L3: 354.545°E 8.408°N (listed in order of decreasing priority) Regional Polygon Vertices: 352.91°E 8.64°N 354.72°E 8.49°N 354.61°E 7.95°N 353.09°E 7.25°N E ‘E ‘ is the potential extended mission target

28. X Landing site is within mantled portion of Arabia, but detailed images show lots of rock exposures

29. Summary Why Revisit Meridiani Meridiani (whether at our proposed site or elsewhere) contains probably the largest and best exposed layered deposits of probable fluvial or lacustrine origin on Mars. Meridiani (whether at our proposed site or elsewhere) contains probably the largest and best exposed layered deposits of probable fluvial or lacustrine origin on Mars. The Meridiani site occurs on a gradual transition from highlands to lowlands and thus provides abundant geologic context for interpretation of age and depositional environment. The Meridiani site occurs on a gradual transition from highlands to lowlands and thus provides abundant geologic context for interpretation of age and depositional environment. A strong case can be made that the Meridiani deposits were deposited into a large regional sea or ocean, either open or ice-covered. A strong case can be made that the Meridiani deposits were deposited into a large regional sea or ocean, either open or ice-covered.

30. It is likely that a site can be found in the Meridiani Planum region that: It is likely that a site can be found in the Meridiani Planum region that: Provides an adequate landing environment Provides an adequate landing environment Provides close access to a thick sequence of the lower beds of the stratigraphic column Provides close access to a thick sequence of the lower beds of the stratigraphic column Contains accessible traverses Contains accessible traverses Contains low-energy fluvial or lacustrine depositional environments with abundant hydrated minerals and chemical precipitates Contains low-energy fluvial or lacustrine depositional environments with abundant hydrated minerals and chemical precipitates Affords dust-free exposures Affords dust-free exposures

31. Issues with Site Local steep slopes within the 20-km ellipses Local steep slopes within the 20-km ellipses Small-scale roughness on portions of the landing sites Small-scale roughness on portions of the landing sites Located in a partially mantled portion of Arabia Located in a partially mantled portion of Arabia May not be able to access rhythmically-bedded deposits within crater May not be able to access rhythmically-bedded deposits within crater No extensive exposures of hydrated minerals seen so far No extensive exposures of hydrated minerals seen so far

32. X Other potential landing site locations with thick exposed sequences of Meridiani layered deposits (arrows)

33. The next slide shows other potential traverse locations, shown on V037200003 (left) and V04881003 (right) The next slide shows other potential traverse locations, shown on V037200003 (left) and V04881003 (right)