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The importance of lake breach floods for valley incision on early Mars. Nature 2021; 597:645-649. [PMID: 34588670 DOI: 10.1038/s41586-021-03860-1] [Citation(s) in RCA: 9] [Impact Index Per Article: 3.0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/23/2020] [Accepted: 07/27/2021] [Indexed: 02/08/2023]
Abstract
The surface environment of early Mars had an active hydrologic cycle, including flowing liquid water that carved river valleys1-3 and filled lake basins4-6. Over 200 of these lake basins filled with sufficient water to breach the confining topography4,6, causing catastrophic flooding and incision of outlet canyons7-10. Much past work has recognized the local importance of lake breach floods on Mars for rapidly incising large valleys7-12; however, on a global scale, valley systems have often been interpreted as recording more persistent fluvial erosion linked to a distributed Martian hydrologic cycle1-3,13-16. Here, we demonstrate the global importance of lake breach flooding, and find that it was responsible for eroding at least 24% of the volume of incised valleys on early Mars, despite representing only approximately 3% of total valley length. We conclude that lake breach floods were a major geomorphic process responsible for valley incision on early Mars, which in turn influenced the topographic form of many Martian valley systems and the broader landscape evolution of the cratered highlands. Our results indicate that the importance of lake breach floods should be considered when reconstructing the formative conditions for Martian valley systems.
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2
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Shen J, Wyness AJ, Claire MW, Zerkle AL. Spatial Variability of Microbial Communities and Salt Distributions Across a Latitudinal Aridity Gradient in the Atacama Desert. MICROBIAL ECOLOGY 2021; 82:442-458. [PMID: 33438074 PMCID: PMC8384830 DOI: 10.1007/s00248-020-01672-w] [Citation(s) in RCA: 11] [Impact Index Per Article: 3.7] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/13/2020] [Accepted: 12/21/2020] [Indexed: 05/13/2023]
Abstract
Over the past 150 million years, the Chilean Atacama Desert has been transformed into one of the most inhospitable landscapes by geophysical changes, which makes it an ideal Mars analog that has been explored for decades. However, a heavy rainfall that occurred in the Atacama in 2017 provides a unique opportunity to study the response of resident extremophiles to rapid environmental change associated with excessive water and salt shock. Here we combine mineral/salt composition measurements, amendment cell culture experiments, and next-generation sequencing analyses to study the variations in salts and microbial communities along a latitudinal aridity gradient of the Atacama Desert. In addition, we examine the reshuffling of Atacama microbiomes after the rainfall event. Analysis of microbial community composition revealed that soils within the southern arid desert were consistently dominated by Actinobacteria, Chloroflexi, Proteobacteria, Firmicutes, Bacteroidetes, Gemmatimonadetes, Planctomycetes, and Acidobacteria, and Verrucomicrobia. Intriguingly, the hyperarid microbial consortia exhibited a similar pattern to the more southern desert. Salts at the shallow subsurface were dissolved and leached down to a deeper layer, challenging indigenous microorganisms with the increasing osmotic stress. Microbial viability was found to change with aridity and rainfall events. This study sheds light on the structure of xerotolerant, halotolerant, and radioresistant microbiomes from the hyperarid northern desert to the less arid southern transition region, as well as their response to changes in water availability.
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Affiliation(s)
- Jianxun Shen
- School of Earth and Environmental Sciences and Centre for Exoplanet Science, University of St Andrews, St Andrews, KY16 9AL, UK.
| | - Adam J Wyness
- Sediment Ecology Research Group, Scottish Oceans Institute, School of Biology, University of St Andrews, St Andrews, KY16 8LB, UK
- Coastal Research Group, Department of Zoology and Entomology, Rhodes University, Grahamstown, 6139, South Africa
| | - Mark W Claire
- School of Earth and Environmental Sciences and Centre for Exoplanet Science, University of St Andrews, St Andrews, KY16 9AL, UK
| | - Aubrey L Zerkle
- School of Earth and Environmental Sciences and Centre for Exoplanet Science, University of St Andrews, St Andrews, KY16 9AL, UK
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Shen J, Smith AC, Claire MW, Zerkle AL. Unraveling biogeochemical phosphorus dynamics in hyperarid Mars-analogue soils using stable oxygen isotopes in phosphate. GEOBIOLOGY 2020; 18:760-779. [PMID: 32822094 DOI: 10.1111/gbi.12408] [Citation(s) in RCA: 5] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/02/2019] [Revised: 05/14/2020] [Accepted: 07/20/2020] [Indexed: 05/27/2023]
Abstract
With annual precipitation less than 20 mm and extreme UV intensity, the Atacama Desert in northern Chile has long been utilized as an analogue for recent Mars. In these hyperarid environments, water and biomass are extremely limited, and thus, it becomes difficult to generate a full picture of biogeochemical phosphate-water dynamics. To address this problem, we sampled soils from five Atacama study sites and conducted three main analyses-stable oxygen isotopes in phosphate, enzyme pathway predictions, and cell culture experiments. We found that high sedimentation rates decrease the relative size of the organic phosphorus pool, which appears to hinder extremophiles. Phosphoenzyme and pathway prediction analyses imply that inorganic pyrophosphatase is the most likely catalytic agent to cycle P in these environments, and this process will rapidly overtake other P utilization strategies. In these soils, the biogenic δ18 O signatures of the soil phosphate (δ18 OPO4 ) can slowly overprint lithogenic δ18 OPO4 values over a timescale of tens to hundreds of millions of years when annual precipitation is more than 10 mm. The δ18 OPO4 of calcium-bound phosphate minerals seems to preserve the δ18 O signature of the water used for biogeochemical P cycling, pointing toward sporadic rainfall and gypsum hydration water as key moisture sources. Where precipitation is less than 2 mm, biological cycling is restricted and bedrock δ18 OPO4 values are preserved. This study demonstrates the utility of δ18 OPO4 values as indicative of biogeochemical cycling and hydrodynamics in an extremely dry Mars-analogue environment.
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Affiliation(s)
- Jianxun Shen
- School of Earth and Environmental Sciences and Centre for Exoplanet Science, University of St Andrews, St Andrews, UK
| | - Andrew C Smith
- NERC Isotope Geosciences Facilities, British Geological Survey, Nottingham, UK
| | - Mark W Claire
- School of Earth and Environmental Sciences and Centre for Exoplanet Science, University of St Andrews, St Andrews, UK
| | - Aubrey L Zerkle
- School of Earth and Environmental Sciences and Centre for Exoplanet Science, University of St Andrews, St Andrews, UK
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Shen J, Zerkle AL, Stueeken E, Claire MW. Nitrates as a Potential N Supply for Microbial Ecosystems in a Hyperarid Mars Analog System. Life (Basel) 2019; 9:life9040079. [PMID: 31635024 PMCID: PMC6958444 DOI: 10.3390/life9040079] [Citation(s) in RCA: 5] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/24/2019] [Revised: 10/08/2019] [Accepted: 10/17/2019] [Indexed: 11/16/2022] Open
Abstract
Nitrate is common in Mars sediments owing to long-term atmospheric photolysis, oxidation, and potentially, impact shock heating. The Atacama Desert in Chile, which is the driest region on Earth and rich in nitrate deposits, is used as a Mars analog in this study to explore the potential effects of high nitrate levels on growth of extremophilic ecosystems. Seven study sites sampled across an aridity gradient in the Atacama Desert were categorized into 3 clusters—hyperarid, middle, and arid sites—as defined by essential soil physical and chemical properties. Intriguingly, the distribution of nitrate concentrations in the shallow subsurface suggests that the buildup of nitrate is not solely controlled by precipitation. Correlations of nitrate with SiO2/Al2O3 and grain sizes suggest that sedimentation rates may also be important in controlling nitrate distribution. At arid sites receiving more than 10 mm/yr precipitation, rainfall shows a stronger impact on biomass than nitrate does. However, high nitrate to organic carbon ratios are generally beneficial to N assimilation, as evidenced both by soil geochemistry and enriched culturing experiments. This study suggests that even in the absence of precipitation, nitrate levels on a more recent, hyperarid Mars could be sufficiently high to benefit potentially extant Martian microorganisms.
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Affiliation(s)
- Jianxun Shen
- School of Earth and Environmental Sciences and Centre for Exoplanet Science, University of St Andrews, St Andrews KY16 9AL, Scotland, UK.
| | - Aubrey L Zerkle
- School of Earth and Environmental Sciences and Centre for Exoplanet Science, University of St Andrews, St Andrews KY16 9AL, Scotland, UK.
| | - Eva Stueeken
- School of Earth and Environmental Sciences and Centre for Exoplanet Science, University of St Andrews, St Andrews KY16 9AL, Scotland, UK.
| | - Mark W Claire
- School of Earth and Environmental Sciences and Centre for Exoplanet Science, University of St Andrews, St Andrews KY16 9AL, Scotland, UK.
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Hargitai HI, Gulick VC, Glines NH. Paleolakes of Northeast Hellas: Precipitation, Groundwater-Fed, and Fluvial Lakes in the Navua-Hadriacus-Ausonia Region, Mars. ASTROBIOLOGY 2018; 18:1435-1459. [PMID: 30289279 DOI: 10.1089/ast.2018.1816] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/08/2023]
Abstract
The slopes of northeastern Hellas Basin, Mars exhibit a wide variety of fluvial landforms. In addition to the Dao-Niger-Harmakhis-Reull Valles outflow channels, many smaller channels and valleys cut into this terrain, several of which include discontinuous sections. We have mapped these channels and channel-associated depressions to investigate potential paleolakes from the Navua Valles in the West, through the Hadriacus Mons volcano in the center, to the Ausonia Montes in the East. We have identified three groups of candidate paleolakes at the source regions of major drainages and a fourth paleolake type scattered along the lower reaches of these drainages. Each paleolake group has a distinct character, determined by different formative processes, including precipitation and groundwater for lakes at the channel sources, and fluvially transported water at the lower channel reaches. Only one of these 34 basins had been cataloged previously in paleolake basin databases. Several of these sites are at proximity to the Hadriacus volcanic center, where active dikes during the Hesperian could have produced hydrothermal systems and habitable environments. Deposits within these paleolake depressions and at the termini of channels connected to these candidate paleolakes contain the geological and potentially biological record of these environments.
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Affiliation(s)
- Henrik I Hargitai
- 1 NASA Ames Research Center, Space Science Division, Moffett Field, California
- 2 Department of Media and Communication, Eötvös Loránd University , Budapest, Hungary
| | - Virginia C Gulick
- 1 NASA Ames Research Center, Space Science Division, Moffett Field, California
- 3 SETI Institute , Mountain View, California
| | - Natalie H Glines
- 1 NASA Ames Research Center, Space Science Division, Moffett Field, California
- 3 SETI Institute , Mountain View, California
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Tosca NJ, Ahmed IA, Tutolo BM, Ashpitel A, Hurowitz JA. Magnetite Authigenesis and the Warming of Early Mars. NATURE GEOSCIENCE 2018; 11:635-639. [PMID: 30123317 PMCID: PMC6092749 DOI: 10.1038/s41561-018-0203-8] [Citation(s) in RCA: 13] [Impact Index Per Article: 2.2] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/12/2018] [Accepted: 07/10/2018] [Indexed: 05/14/2023]
Abstract
The Curiosity rover has documented lacustrine sediments at Gale Crater, but how liquid water became physically stable on the early Martian surface is a matter of significant debate. To constrain the composition of the early Martian atmosphere during sediment deposition, we experimentally investigated the nucleation and growth kinetics of authigenic Fe-minerals in Gale Crater mudstones. Experiments show that pH variations within anoxic basaltic waters trigger a series of mineral transformations that rapidly generate magnetite and H2(aq). Magnetite continues to form through this mechanism despite high PCO2 and supersaturation with respect to Fe-carbonate minerals. Reactive transport simulations that incorporate these experimental data show that groundwater infiltration into a lake equilibrated with a CO2-rich atmosphere can trigger the production of both magnetite and H2(aq) in the mudstones. H2(aq), generated at concentrations that would readily exsolve from solution, is capable of increasing annual mean surface temperatures above freezing in CO2-dominated atmospheres. We therefore suggest that magnetite authigenesis could have provided a short-term feedback for stabilizing liquid water, as well as a principal feedstock for biologically relevant chemical reactions, at the early Martian surface.
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Affiliation(s)
- Nicholas J. Tosca
- Dept. of Earth Sciences, University of Oxford, South Parks Road, Oxford, OX1 3AN, UK
| | - Imad A.M. Ahmed
- Dept. of Earth Sciences, University of Oxford, South Parks Road, Oxford, OX1 3AN, UK
| | - Benjamin M. Tutolo
- Department of Geoscience, University of Calgary, Calgary, AB, T2N 1N4, Canada
| | - Alice Ashpitel
- Dept. of Earth Sciences, University of Oxford, South Parks Road, Oxford, OX1 3AN, UK
| | - Joel A. Hurowitz
- Department of Geosciences, Stony Brook University, Stony Brook, NY 11794-2100, USA
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Baker VR, Hamilton CW, Burr DM, Gulick VC, Komatsu G, Luo W, Rice JW, Rodriguez J. Fluvial geomorphology on Earth-like planetary surfaces: A review. GEOMORPHOLOGY (AMSTERDAM, NETHERLANDS) 2015; 245:149-182. [PMID: 29176917 PMCID: PMC5701759 DOI: 10.1016/j.geomorph.2015.05.002] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.9] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/07/2023]
Abstract
Morphological evidence for ancient channelized flows (fluvial and fluvial-like landforms) exists on the surfaces of all of the inner planets and on some of the satellites of the Solar System. In some cases, the relevant fluid flows are related to a planetary evolution that involves the global cycling of a volatile component (water for Earth and Mars; methane for Saturn's moon Titan). In other cases, as on Mercury, Venus, Earth's moon, and Jupiter's moon Io, the flows were of highly fluid lava. The discovery, in 1972, of what are now known to be fluvial channels and valleys on Mars sparked a major controversy over the role of water in shaping the surface of that planet. The recognition of the fluvial character of these features has opened unresolved fundamental questions about the geological history of water on Mars, including the presence of an ancient ocean and the operation of a hydrological cycle during the earliest phases of planetary history. Other fundamental questions posed by fluvial and fluvial-like features on planetary bodies include the possible erosive action of large-scale outpourings of very fluid lavas, such as those that may have produced the remarkable canali forms on Venus; the ability of exotic fluids, such as methane, to create fluvial-like landforms, as observed on Saturn's moon, Titan; and the nature of sedimentation and erosion under different conditions of planetary surface gravity. Planetary fluvial geomorphology also illustrates fundamental epistemological and methodological issues, including the role of analogy in geomorphological/geological inquiry.
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Affiliation(s)
- Victor R. Baker
- Department of Hydrology and Water Resources, University of Arizona, Tucson, AZ 85721, USA
- Lunar and Planetary Laboratory, Department of Planetary Sciences, University of Arizona, Tucson, AZ 85721, USA
| | - Christopher W. Hamilton
- Lunar and Planetary Laboratory, Department of Planetary Sciences, University of Arizona, Tucson, AZ 85721, USA
| | - Devon M. Burr
- Earth and Planetary Sciences Department, University of Tennessee-Knoxville, Knoxville, TN 37996-1410, USA
| | - Virginia C. Gulick
- SETI Institute, Mountain View, CA 94043, USA
- NASA Ames Research Center, MS 239-20, Moffett Field, CA 94035, USA
| | - Goro Komatsu
- International Research School of Planetary Sciences, Università d’Annunzio, Viale Pindaro 42, 65127 Pescara, Italy
| | - Wei Luo
- Department of Geography, Northern Illinois University, DeKalb, IL 60115, USA
| | | | - J.A.P. Rodriguez
- NASA Ames Research Center, MS 239-20, Moffett Field, CA 94035, USA
- Planetary Science Institute, Tucson, AZ 85719, USA
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Goudge TA, Mustard JF, Head JW, Fassett CI. Constraints on the history of open-basin lakes on Mars from the composition and timing of volcanic resurfacing. ACTA ACUST UNITED AC 2012. [DOI: 10.1029/2012je004115] [Citation(s) in RCA: 36] [Impact Index Per Article: 3.0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
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9
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van Berk W, Fu Y, Ilger JM. Reproducing early Martian atmospheric carbon dioxide partial pressure by modeling the formation of Mg-Fe-Ca carbonate identified in the Comanche rock outcrops on Mars. ACTA ACUST UNITED AC 2012. [DOI: 10.1029/2012je004173] [Citation(s) in RCA: 14] [Impact Index Per Article: 1.2] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022]
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10
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Carr MH. The fluvial history of Mars. PHILOSOPHICAL TRANSACTIONS. SERIES A, MATHEMATICAL, PHYSICAL, AND ENGINEERING SCIENCES 2012; 370:2193-2215. [PMID: 22474681 DOI: 10.1098/rsta.2011.0500] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/31/2023]
Abstract
River channels and valleys have been observed on several planetary bodies in addition to the Earth. Long sinuous valleys on Venus, our Moon and Jupiter's moon Io are clearly formed by lava, and branching valleys on Saturn's moon Titan may be forming today by rivers of methane. But by far the most dissected body in our Solar System apart from the Earth is Mars. Branching valleys that in plan resemble terrestrial river valleys are common throughout the most ancient landscapes preserved on the planet. Accompanying the valleys are the remains of other indicators of erosion and deposition, such as deltas, alluvial fans and lake beds. There is little reason to doubt that water was the erosive agent and that early in Mars' history, climatic conditions were very different from the present cold conditions and such that, at least episodically, water could flow across the surface. In addition to the branching valley networks, there are large flood features, termed outflow channels. These are similar to, but dwarf, the largest terrestrial flood channels. The consensus is that these channels were also cut by water although there are other possibilities. The outflow channels mostly postdate the valley networks, although most are still very ancient. They appear to have formed at a time when surface conditions were similar to those that prevail today. There is evidence that glacial activity has modified some of the water-worn valleys, particularly in the 30-50° latitude belts, and ice may also be implicated in the formation of geologically recent, seemingly water-worn gullies on steep slopes. Mars also has had a long volcanic history, and long, sinuous lava channels similar to those on the Moon and Venus are common on and around the large volcanoes. These will not, however, be discussed further; the emphasis here is on the effects of running water on the evolution of the surface.
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Affiliation(s)
- Michael H Carr
- US Geological Survey, 345 Middlefield Road, Menlo Park, CA 94025, USA.
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11
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Howard AD, Moore JM. Late Hesperian to early Amazonian midlatitude Martian valleys: Evidence from Newton and Gorgonum basins. ACTA ACUST UNITED AC 2011. [DOI: 10.1029/2010je003782] [Citation(s) in RCA: 47] [Impact Index Per Article: 3.6] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
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13
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Wray JJ, Milliken RE, Dundas CM, Swayze GA, Andrews-Hanna JC, Baldridge AM, Chojnacki M, Bishop JL, Ehlmann BL, Murchie SL, Clark RN, Seelos FP, Tornabene LL, Squyres SW. Columbus crater and other possible groundwater-fed paleolakes of Terra Sirenum, Mars. ACTA ACUST UNITED AC 2011. [DOI: 10.1029/2010je003694] [Citation(s) in RCA: 121] [Impact Index Per Article: 9.3] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
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14
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Mest SC, Crown DA, Harbert W. Watershed modeling in the Tyrrhena Terra region of Mars. ACTA ACUST UNITED AC 2010. [DOI: 10.1029/2009je003429] [Citation(s) in RCA: 14] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
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15
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Affiliation(s)
- Michael P. Lamb
- Department of Earth and Planetary Science, University of California, Berkeley, California 94720, USA
| | - William E. Dietrich
- Department of Earth and Planetary Science, University of California, Berkeley, California 94720, USA
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16
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Banks ME, McEwen AS, Kargel JS, Baker VR, Strom RG, Mellon MT, Gulick VC, Keszthelyi L, Herkenhoff KE, Pelletier JD, Jaeger WL. High Resolution Imaging Science Experiment (HiRISE) observations of glacial and periglacial morphologies in the circum-Argyre Planitia highlands, Mars. ACTA ACUST UNITED AC 2008. [DOI: 10.1029/2007je002994] [Citation(s) in RCA: 33] [Impact Index Per Article: 2.1] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022]
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17
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Thomson BJ, Bridges NT, Greeley R. Rock abrasion features in the Columbia Hills, Mars. ACTA ACUST UNITED AC 2008. [DOI: 10.1029/2007je003018] [Citation(s) in RCA: 25] [Impact Index Per Article: 1.6] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
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18
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Golombek MP, Grant JA, Crumpler LS, Greeley R, Arvidson RE, Bell JF, Weitz CM, Sullivan R, Christensen PR, Soderblom LA, Squyres SW. Erosion rates at the Mars Exploration Rover landing sites and long-term climate change on Mars. ACTA ACUST UNITED AC 2006. [DOI: 10.1029/2006je002754] [Citation(s) in RCA: 181] [Impact Index Per Article: 10.1] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Affiliation(s)
- M. P. Golombek
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - J. A. Grant
- Center for Earth and Planetary Studies, National Air and Space Museum; Smithsonian Institution; Washington, DC USA
| | - L. S. Crumpler
- New Mexico Museum of Natural History and Science; Albuquerque New Mexico USA
| | - R. Greeley
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - R. E. Arvidson
- Department of Earth and Planetary Sciences; Washington University; St. Louis Missouri USA
| | - J. F. Bell
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - C. M. Weitz
- Planetary Science Institute; Tucson Arizona USA
| | - R. Sullivan
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - P. R. Christensen
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | | | - S. W. Squyres
- Department of Astronomy; Cornell University; Ithaca New York USA
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Cabrol NA, Farmer JD, Grin EA, Richter L, Soderblom L, Li R, Herkenhoff K, Landis GA, Arvidson RE. Aqueous processes at Gusev crater inferred from physical properties of rocks and soils along the Spirit traverse. ACTA ACUST UNITED AC 2006. [DOI: 10.1029/2005je002490] [Citation(s) in RCA: 23] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Affiliation(s)
- N. A. Cabrol
- Space Science Division; NASA Ames Research Center; Moffett Field California USA
- SETI Institute; Mountain View California USA
| | - J. D. Farmer
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - E. A. Grin
- Space Science Division; NASA Ames Research Center; Moffett Field California USA
- SETI Institute; Mountain View California USA
| | - L. Richter
- DLR Institut für Raumsimulation; Cologne Germany
| | | | - R. Li
- Department of Civil and Environmental Engineering and Geodetic Science; Ohio State University; Columbus Ohio USA
| | | | - G. A. Landis
- Photovoltaics and Space Environment Branch; NASA John Glenn Research Center; Cleveland Ohio USA
| | - R. E. Arvidson
- Department of Earth and Planetary Sciences; Washington University; St. Louis Missouri USA
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20
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Golombek MP, Crumpler LS, Grant JA, Greeley R, Cabrol NA, Parker TJ, Rice JW, Ward JG, Arvidson RE, Moersch JE, Fergason RL, Christensen PR, Castaño A, Castaño R, Haldemann AFC, Li R, Bell JF, Squyres SW. Geology of the Gusev cratered plains from the Spirit rover transverse. ACTA ACUST UNITED AC 2006. [DOI: 10.1029/2005je002503] [Citation(s) in RCA: 97] [Impact Index Per Article: 5.4] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022]
Affiliation(s)
- M. P. Golombek
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - L. S. Crumpler
- New Mexico Museum of Natural History and Science; Albuquerque New Mexico USA
| | | | - R. Greeley
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - N. A. Cabrol
- NASA Ames Research Center; Moffett Field California USA
| | - T. J. Parker
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - J. W. Rice
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - J. G. Ward
- Department of Earth and Planetary Sciences; Washington University; St. Louis Missouri USA
| | - R. E. Arvidson
- Department of Earth and Planetary Sciences; Washington University; St. Louis Missouri USA
| | - J. E. Moersch
- Department of Geological Sciences; University of Tennessee; Knoxville Tennessee USA
| | - R. L. Fergason
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - P. R. Christensen
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - A. Castaño
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - R. Castaño
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - A. F. C. Haldemann
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - R. Li
- Department of Civil and Environmental Engineering and Geodetic Science; Ohio State University; Columbus Ohio USA
| | - J. F. Bell
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - S. W. Squyres
- Department of Astronomy; Cornell University; Ithaca New York USA
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Kraal ER, Asphaug E, Moore JM, Lorenz RD. Quantitative geomorphic modeling of Martian bedrock shorelines. ACTA ACUST UNITED AC 2006. [DOI: 10.1029/2005je002567] [Citation(s) in RCA: 21] [Impact Index Per Article: 1.2] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
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22
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Kleinhans MG. Flow discharge and sediment transport models for estimating a minimum timescale of hydrological activity and channel and delta formation on Mars. ACTA ACUST UNITED AC 2005. [DOI: 10.1029/2005je002521] [Citation(s) in RCA: 126] [Impact Index Per Article: 6.6] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
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23
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Martínez-Alonso S. A volcanic interpretation of Gusev Crater surface materials from thermophysical, spectral, and morphological evidence. ACTA ACUST UNITED AC 2005. [DOI: 10.1029/2004je002327] [Citation(s) in RCA: 49] [Impact Index Per Article: 2.6] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022]
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Grant JA, Arvidson R, Bell JF, Cabrol NA, Carr MH, Christensen P, Crumpler L, Des Marais DJ, Ehlmann BL, Farmer J, Golombek M, Grant FD, Greeley R, Herkenhoff K, Li R, McSween HY, Ming DW, Moersch J, Rice JW, Ruff S, Richter L, Squyres S, Sullivan R, Weitz C. Surficial Deposits at Gusev Crater Along Spirit Rover Traverses. Science 2004; 305:807-10. [PMID: 15297659 DOI: 10.1126/science.1099849] [Citation(s) in RCA: 71] [Impact Index Per Article: 3.6] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
The Mars Exploration Rover Spirit has traversed a fairly flat, rock-strewn terrain whose surface is shaped primarily by impact events, although some of the landscape has been altered by eolian processes. Impacts ejected basaltic rocks that probably were part of locally formed lava flows from at least 10 meters depth. Some rocks have been textured and/or partially buried by windblown sediments less than 2 millimeters in diameter that concentrate within shallow, partially filled, circular impact depressions referred to as hollows. The terrain traversed during the 90-sol (martian solar day) nominal mission shows no evidence for an ancient lake in Gusev crater.
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Affiliation(s)
- J A Grant
- Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, Washington, DC 20560, USA.
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Leverington DW. Differential subsidence and rebound in response to changes in water loading on Mars: Possible effects on the geometry of ancient shorelines. ACTA ACUST UNITED AC 2004. [DOI: 10.1029/2003je002141] [Citation(s) in RCA: 19] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
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Irwin RP. Geomorphology of Ma'adim Vallis, Mars, and associated paleolake basins. ACTA ACUST UNITED AC 2004. [DOI: 10.1029/2004je002287] [Citation(s) in RCA: 117] [Impact Index Per Article: 5.9] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022]
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Cabrol NA, Grin EA, Carr MH, Sutter B, Moore JM, Farmer JD, Greeley R, Kuzmin RO, DesMarais DJ, Kramer MG, Newsom H, Barber C, Thorsos I, Tanaka KL, Barlow NG, Fike DA, Urquhart ML, Grigsby B, Grant FD, de Goursac O. Exploring Gusev Crater with Spirit: Review of science objectives and testable hypotheses. ACTA ACUST UNITED AC 2003. [DOI: 10.1029/2002je002026] [Citation(s) in RCA: 41] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022]
Affiliation(s)
| | | | | | - Brad Sutter
- NASA Ames Research Center; Moffett Field California USA
| | | | - Jack D. Farmer
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - Ronald Greeley
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | | | | | | | - Horton Newsom
- Institute of Meteoritics and Department of Earth and Planetary Sciences; University of New Mexico; Albuquerque New Mexico USA
| | - Charles Barber
- Institute of Meteoritics and Department of Earth and Planetary Sciences; University of New Mexico; Albuquerque New Mexico USA
| | - Ivan Thorsos
- Institute of Meteoritics and Department of Earth and Planetary Sciences; University of New Mexico; Albuquerque New Mexico USA
| | - Kenneth L. Tanaka
- Department of Physics and Astronomy; Northern Arizona University; Flagstaff Arizona USA
| | | | - David A. Fike
- Department of Earth, Atmospheric, and Planetary Sciences; Massachussetts Institute of Technology; Cambridge Massachusetts USA
| | - Mary L. Urquhart
- Department of Science and Mathematics Education; University of Texas at Dallas; Richardson Texas USA
| | | | - Frederick D. Grant
- Department of Geology; University of Mississippi; Jackson Mississippi USA
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Golombek MP, Grant JA, Parker TJ, Kass DM, Crisp JA, Squyres SW, Haldemann AFC, Adler M, Lee WJ, Bridges NT, Arvidson RE, Carr MH, Kirk RL, Knocke PC, Roncoli RB, Weitz CM, Schofield JT, Zurek RW, Christensen PR, Fergason RL, Anderson FS, Rice JW. Selection of the Mars Exploration Rover landing sites. ACTA ACUST UNITED AC 2003. [DOI: 10.1029/2003je002074] [Citation(s) in RCA: 126] [Impact Index Per Article: 6.0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Affiliation(s)
- M. P. Golombek
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - J. A. Grant
- Center for Earth and Planetary Studies; National Air and Space Museum, Smithsonian Institution; Washington DC USA
| | - T. J. Parker
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - D. M. Kass
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - J. A. Crisp
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - S. W. Squyres
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - A. F. C. Haldemann
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - M. Adler
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - W. J. Lee
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - N. T. Bridges
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - R. E. Arvidson
- Department of Earth and Space Sciences; Washington University; St. Louis Missouri USA
| | - M. H. Carr
- U.S. Geological Survey; Menlo Park California USA
| | - R. L. Kirk
- U.S. Geological Survey; Flagstaff Arizona USA
| | - P. C. Knocke
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - R. B. Roncoli
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | | | - J. T. Schofield
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - R. W. Zurek
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - P. R. Christensen
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - R. L. Fergason
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - F. S. Anderson
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - J. W. Rice
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
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Affiliation(s)
- Robert A. Craddock
- Center for Earth and Planetary Studies, National Air and Space Museum; Smithsonian Institution; Washington District of Columbia USA
| | - Alan D. Howard
- Department of Environmental Sciences; University of Virginia; Charlottesville Virginia USA
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