Aqueous Sedimentary Depositional Environments, Meridiani Planum, Mars
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1 Aqueous Sedimentary Depositional Environments, Meridiani Planum, Mars John Grotzinger on behalf of MER Athena Science Team
2
3 The Team
4 The PI
5 The Rovers 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
6 Opportunity at Meridiani Planum Meridiani Gusev
7 Hematite: Mineralogic Beacon
8 Meridiani Landing Site
9 Spirit: View from Lander 5 metres Opportunity: View from Lander 5 metres
10 Geological Traverse
11 Geological Map
12 El Capitan
13
14 Bromine vs. Chlorine
15 APXS Results: High S in Rocks 40 Fe 2 O35 3 (wt.%) HEMATITE-RICH Spherulerich Soil Dust Spherule-rich Fract fill/vein Basalts Soil Bright Soil Soil on Rock Nat Rk surface Rk w/soil Rk nat surf Rk RAT'd Basalt END MEMBERS (SCHEMATIC) RAT'd Rocks SULFATES SO 3 (wt.%, total S as SO 3 ) B. Jolliff
16 APXS Results: Crud Extraction 12 Al 2 O 3 (wt.%) Spherulerich Soil Soil Bright Soil Soil on Rock Nat Rk surfa ce RAT'd Rocks Soil Dust Spherule-rich Fract fill/vein Rk w/soil Rk nat surf Rk RAT'd Basalt If subtract 60% of dust or basalt component from average RAT d rock composition, Al 2 O 3 and Cr 2 O 3 go to zero at ~50% SO SO 3 (wt.%, total S as SO 3 ) B. Jolliff
17 N. Tosca
18 Rio Tinto, Spain
19 Mini-TES: Hematite Distribution
20 Soil Granules (Spherules)
21 Pancam on Stone Mountain
22 Microimager: Spherules in Outcrop
23 Concretions
24 Spherules Not Concentrated Along Bedding
25 Distribution of Concretions
26 W. Watters, D. Fike
27 Doublets Triplet
28 The Berry Bowl
29 Mössbauer on the Berry Bowl
30 N. Tosca
31 Concretions: Two Types?
32
33 Vugs
34 Sulfate Minerals: Gypsum?
35 Evaporite-Filled Crystal Molds on Earth
36 The Rocks are Sandstones Laminae Defined by Variable Grain Size 0.3 mm Medium Grain size Well Rounded 0.8 mm
37 Bedforms in Flowing Water Southard and Bouchwal, 1990
38 Current Ripples in Water 6 hours of ripple migration Image is 60x40 cm Flume experiments by Dave Rubin and Jon Nelson, USGS
39 Current Ripples in Cross Section Simulation by Dave Rubin, USGS
40 Ripple Cross-Bedding on Mars
41 Ripple Cross-Bedding
42 Festoon Cross-Bedding on Earth
43 Modern Mars Analog: Umm a Samin Braid Plain Modern Playa Dunes 100 km
44 Network of Interdune Depressions
45 Interdune Depression
46 Modern Interdune Depression: Namib Desert
47
48 Endurance Chemostratigraphy
49 A Trail of 11 RAT Holes
50 Ratio to surface rock average Depth in crater A. Haldemann
51 Changes Down Section: Texture Ontario Diamond Jenness
52 Diagenetic Model S. McLennan, N. Tosca
53 S. McLennan, N. Tosca
54 S. McLennan, N. Tosca
55 Other Evidence for Liquid Water on Mars Modern Ancient
56 What about (astro)biology? Rover reveals Mars was once wet enough for life (MsNBC) Red planet may have been hospitable to life (CNN) Mars could once support life, scientists now say, but did it? (NY Times)
57 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
58 Could Life Begin in Acidic Waters? Several key reactions do not proceed at acidic ph: e.g. Strecker synthesis (generates amino acids) Proteins and DNA both readily hydrolyzed in acidic waters Experimental growth of nucleotides yields triple helix in acidic waters The oxidizing surface of Mars would make things worse. We need to understand when Meridiani-like conditions were established on Mars. Was there ever a surface environment that was more conducive to prebiotic chemistry?
59 The Good News 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. All this favors Meridiani Planum as a target for sample return.
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