1
|
Picard A, Gartman A, Girguis PR. Interactions Between Iron Sulfide Minerals and Organic Carbon: Implications for Biosignature Preservation and Detection. ASTROBIOLOGY 2021; 21:587-604. [PMID: 33780638 DOI: 10.1089/ast.2020.2276] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/12/2023]
Abstract
Microbe-mineral interactions can produce unique composite materials, which can preserve biosignatures. Geological evidence suggests that iron sulfide (Fe-S) minerals are abundant in the subsurface of Mars. On Earth, the formation of Fe-S minerals is driven by sulfate-reducing microorganisms (SRM) that produce reactive sulfide. Moreover, SRM metabolites, as well as intact cells, can influence the morphology, particle size, aggregation, and composition of biogenic Fe-S minerals. In this work, we evaluated how simple and complex organic molecules-hexoses and amino acid/peptide mixtures, respectively-influence the formation of Fe-S minerals (simulated prebiotic conditions), and whether the observed patterns mimic the biological influence of SRM. To this end, organo-mineral aggregates were characterized with X-ray diffraction, scanning electron microscopy, and scanning transmission X-ray microscopy coupled to near-edge X-ray absorption fine structure spectroscopy. Overall, Fe-S minerals were found to have a strong affinity for proteinaceous organic matter. Fe-S minerals precipitated at simulated prebiotic conditions yielded organic carbon distributions that were more homogeneous than treatments with whole SRM cells. In prebiotic experiments, spectroscopy detected potential organic transformations during Fe-S mineral formation, including conversion of hexoses to sugar acids and polymerization of amino acids/peptides into larger peptides/proteins. In addition, prebiotic mineral-carbon assemblages produced nanometer-scaled filamentous aggregated morphologies. On the contrary, in biotic treatments with cells, organic carbon in minerals displayed a more heterogeneous distribution. Notably, "hot spots" of organic carbon and oxygen-containing functional groups, with the size, shape, and composition of microbial cells, were preserved in mineral aggregates. We propose a list of characteristics that could be used to help distinguish biogenic from prebiotic/abiotic Fe-S minerals and help refine the search of extant or extinct microbial life in the martian subsurface.
Collapse
Affiliation(s)
- Aude Picard
- Department of Organismic and Evolutionary Biology, Harvard University, Cambridge, Massachusetts, USA
- School of Life Sciences, University of Nevada, Las Vegas, Las Vegas, Nevada, USA
| | - Amy Gartman
- Department of Organismic and Evolutionary Biology, Harvard University, Cambridge, Massachusetts, USA
| | - Peter R Girguis
- Department of Organismic and Evolutionary Biology, Harvard University, Cambridge, Massachusetts, USA
| |
Collapse
|
2
|
Niles PB, Michalski J, Ming DW, Golden DC. Elevated olivine weathering rates and sulfate formation at cryogenic temperatures on Mars. Nat Commun 2017; 8:998. [PMID: 29044111 PMCID: PMC5647339 DOI: 10.1038/s41467-017-01227-7] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/20/2017] [Accepted: 08/31/2017] [Indexed: 11/12/2022] Open
Abstract
Large Hesperian-aged (~3.7 Ga) layered deposits of sulfate-rich sediments in the equatorial regions of Mars have been suggested to be evidence for ephemeral playa environments. But early Mars may not have been warm enough to support conditions similar to what occurs in arid environments on Earth. Instead cold, icy environments may have been widespread. Under cryogenic conditions sulfate formation might be blocked, since kinetics of silicate weathering are typically strongly retarded at temperatures well below 0 °C. But cryo-concentration of acidic solutions may counteract the slow kinetics. Here we show that cryo-concentrated acidic brines rapidly chemically weather olivine minerals and form sulfate minerals at temperatures as low as −60 °C. These experimental results demonstrate the viability of sulfate formation under current Martian conditions, even in the polar regions. An ice-hosted sedimentation and weathering model may provide a compelling description of the origin of large Hesperian-aged layered sulfate deposits on Mars. Sulphate-rich sediments have been taken as evidence of surface water on Mars. Here, the authors show that cryo-concentrated brines chemically weather olivine minerals forming sulfate minerals at up to −60 °C, showing that cryogenic weathering and sulfate formation can occur under current Martian conditions.
Collapse
Affiliation(s)
- Paul B Niles
- Astromaterials Research and Exploration Science Division, NASA Johnson Space Center, Houston, TX, 77058, USA.
| | - Joseph Michalski
- Department of Earth Sciences and Laboratory for Space Research, University of Hong Kong, Hong Kong, China
| | - Douglas W Ming
- Astromaterials Research and Exploration Science Division, NASA Johnson Space Center, Houston, TX, 77058, USA
| | | |
Collapse
|
3
|
Gil-Lozano C, Davila AF, Losa-Adams E, Fairén AG, Gago-Duport L. Quantifying Fenton reaction pathways driven by self-generated H 2O 2 on pyrite surfaces. Sci Rep 2017; 7:43703. [PMID: 28262831 PMCID: PMC5337962 DOI: 10.1038/srep43703] [Citation(s) in RCA: 36] [Impact Index Per Article: 5.1] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/19/2016] [Accepted: 01/26/2017] [Indexed: 01/08/2023] Open
Abstract
Oxidation of pyrite (FeS2) plays a significant role in the redox cycling of iron and sulfur on Earth and is the primary cause of acid mine drainage (AMD). It has been established that this process involves multi-step electron-transfer reactions between surface defects and adsorbed O2 and H2O, releasing sulfoxy species (e.g., S2O32-, SO42-) and ferrous iron (Fe2+) to the solution and also producing intermediate by-products, such as hydrogen peroxide (H2O2) and other reactive oxygen species (ROS), however, our understanding of the kinetics of these transient species is still limited. We investigated the kinetics of H2O2 formation in aqueous suspensions of FeS2 microparticles by monitoring, in real time, the H2O2 and dissolved O2 concentration under oxic and anoxic conditions using amperometric microsensors. Additional spectroscopic and structural analyses were done to track the dependencies between the process of FeS2 dissolution and the degradation of H2O2 through the Fenton reaction. Based on our experimental results, we built a kinetic model which explains the observed trend of H2O2, showing that FeS2 dissolution can act as a natural Fenton reagent, influencing the oxidation of third-party species during the long term evolution of geochemical systems, even in oxygen-limited environments.
Collapse
Affiliation(s)
- C. Gil-Lozano
- Centro de Astrobiología (CSIC-INTA), 28850 Torrejón de Ardoz, Madrid, Spain
| | - A. F. Davila
- Carl Sagan Center at the SETI Institute, 189 Bernardo Avenue, Suite 100, Mountain View, CA 94043, USA
| | - E. Losa-Adams
- Centro de Astrobiología (CSIC-INTA), 28850 Torrejón de Ardoz, Madrid, Spain
- Departamento de Geociencias Marinas, Universidad de Vigo, Lagoas Marcosende, 36310-Vigo, Spain
| | - A. G. Fairén
- Centro de Astrobiología (CSIC-INTA), 28850 Torrejón de Ardoz, Madrid, Spain
- Department of Astronomy, Cornell University, Ithaca, 14853 NY, USA
| | - L. Gago-Duport
- Departamento de Geociencias Marinas, Universidad de Vigo, Lagoas Marcosende, 36310-Vigo, Spain
| |
Collapse
|
4
|
Williams AJ, Sumner DY, Alpers CN, Karunatillake S, Hofmann BA. Preserved Filamentous Microbial Biosignatures in the Brick Flat Gossan, Iron Mountain, California. ASTROBIOLOGY 2015; 15:637-68. [PMID: 26247371 PMCID: PMC4554944 DOI: 10.1089/ast.2014.1235] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.9] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/01/2014] [Accepted: 06/07/2015] [Indexed: 05/21/2023]
Abstract
A variety of actively precipitating mineral environments preserve morphological evidence of microbial biosignatures. One such environment with preserved microbial biosignatures is the oxidized portion of a massive sulfide deposit, or gossan, such as that at Iron Mountain, California. This gossan may serve as a mineralogical analogue to some ancient martian environments due to the presence of oxidized iron and sulfate species, and minerals that only form in acidic aqueous conditions, in both environments. Evaluating the potential biogenicity of cryptic textures in such martian gossans requires an understanding of how microbial textures form biosignatures on Earth. The iron-oxide-dominated composition and morphology of terrestrial, nonbranching filamentous microbial biosignatures may be distinctive of the underlying formation and preservation processes. The Iron Mountain gossan consists primarily of ferric oxide (hematite), hydrous ferric oxide (HFO, predominantly goethite), and jarosite group minerals, categorized into in situ gossan, and remobilized iron deposits. We interpret HFO filaments, found in both gossan types, as HFO-mineralized microbial filaments based in part on (1) the presence of preserved central filament lumina in smooth HFO mineral filaments that are likely molds of microbial filaments, (2) mineral filament formation in actively precipitating iron-oxide environments, (3) high degrees of mineral filament bending consistent with a flexible microbial filament template, and (4) the presence of bare microbial filaments on gossan rocks. Individual HFO filaments are below the resolution of the Mars Curiosity and Mars 2020 rover cameras, but sinuous filaments forming macroscopic matlike textures are resolvable. If present on Mars, available cameras may resolve these features identified as similar to terrestrial HFO filaments and allow subsequent evaluation for their biogenicity by synthesizing geochemical, mineralogical, and morphological analyses. Sinuous biogenic filaments could be preserved on Mars in an iron-rich environment analogous to Iron Mountain, with the Pahrump Hills region and Hematite Ridge in Gale Crater as tentative possibilities.
Collapse
Affiliation(s)
- Amy J. Williams
- Department of Earth and Planetary Sciences, University of California, Davis, Davis, California, USA
| | - Dawn Y. Sumner
- Department of Earth and Planetary Sciences, University of California, Davis, Davis, California, USA
| | - Charles N. Alpers
- U.S. Geological Survey, California Water Science Center, Sacramento, California, USA
| | - Suniti Karunatillake
- Department of Geology and Geophysics, Louisiana State University, Baton Rouge, Louisiana, USA
| | - Beda A. Hofmann
- Naturhistorisches Museum der Burgergemeinde Bern, Bern, Switzerland
| |
Collapse
|
5
|
|
6
|
McHenry LJ, Chevrier V, Schröder C. Jarosite in a Pleistocene East African saline-alkaline paleolacustrine deposit: Implications for Mars aqueous geochemistry. ACTA ACUST UNITED AC 2011. [DOI: 10.1029/2010je003680] [Citation(s) in RCA: 15] [Impact Index Per Article: 1.2] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022]
|
7
|
Greeley R, Schneid BD. Magma generation on Mars: amounts, rates, and comparisons with Earth, moon, and venus. Science 2010; 254:996-8. [PMID: 17731523 DOI: 10.1126/science.254.5034.996] [Citation(s) in RCA: 150] [Impact Index Per Article: 10.7] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
Total extrusive and intrusive magma generated on Mars over the last approximately 3.8 billion years is estimated at 654 x 10(6) cubic kilometers, or 0.17 cubic kilometers per year (km(3)/yr), substantially less than rates for Earth (26 to 34 km(3)/yr) and Venus (less than 20 km(3)/yr) but much more than for the Moon (0.025 km(3)/yr). When scaled to Earth's mass the martian rate is much smaller than that for Earth or Venus and slightly smaller than for the Moon.
Collapse
|
8
|
Chiriţǎ P. Iron monosulfide (FeS) oxidation by dissolved oxygen: characteristics of the product layer. SURF INTERFACE ANAL 2009. [DOI: 10.1002/sia.3041] [Citation(s) in RCA: 11] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/06/2022]
|
9
|
Fernández-Remolar DC, Prieto-Ballesteros O, Rodríguez N, Gómez F, Amils R, Gómez-Elvira J, Stoker CR. Underground habitats in the Río Tinto basin: a model for subsurface life habitats on Mars. ASTROBIOLOGY 2008; 8:1023-1047. [PMID: 19105758 DOI: 10.1089/ast.2006.0104] [Citation(s) in RCA: 38] [Impact Index Per Article: 2.4] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/27/2023]
Abstract
A search for evidence of cryptic life in the subsurface region of a fractured Paleozoic volcanosedimentary deposit near the source waters of the Río Tinto River (Iberian pyrite belt, southwest Spain) was carried out by Mars Astrobiology Research and Technology Experiment (MARTE) project investigators in 2003 and 2004. This conventional deep-drilling experiment is referred to as the MARTE ground truth drilling project. Boreholes were drilled at three sites, and samples from extracted cores were analyzed with light microscopy, scanning electron microscopy-energy dispersive spectroscopy (SEM-EDS), X-ray diffraction (XRD), and Fourier transform infrared spectroscopy. Core leachates were analyzed with ion chromatography, and borehole fluids were analyzed with ion and gas chromatography. Key variables of the groundwater system (e.g., pO(2), pH, and salinity) exhibit huge ranges probably due to surficial oxygenation of overall reducing waters, physical mixing of waters, and biologically mediated water-rock interactions. Mineral distribution is mainly driven by the pH of subsurface solutions, which range from highly acidic to neutral. Borehole fluids contain dissolved gases such as CO(2), CH(4), and H(2). SEM-EDS analyses of core samples revealed evidence of microbes attacking pyrite. The Río Tinto alteration mechanisms may be similar to subsurface weathering of the martian crust and provide insights into the possible (bio)geochemical cycles that may have accompanied underground habitats in extensive early Mars volcanic regions and associated sulfide ores.
Collapse
|
10
|
McAdam AC, Zolotov MY, Mironenko MV, Sharp TG. Formation of silica by low-temperature acid alteration of Martian rocks: Physical-chemical constraints. ACTA ACUST UNITED AC 2008. [DOI: 10.1029/2007je003056] [Citation(s) in RCA: 36] [Impact Index Per Article: 2.3] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
|
11
|
Tosca NJ, McLennan SM, Dyar MD, Sklute EC, Michel FM. Fe oxidation processes at Meridiani Planum and implications for secondary Fe mineralogy on Mars. ACTA ACUST UNITED AC 2008. [DOI: 10.1029/2007je003019] [Citation(s) in RCA: 57] [Impact Index Per Article: 3.6] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
|
12
|
Fishbaugh KE, Poulet F, Chevrier V, Langevin Y, Bibring JP. On the origin of gypsum in the Mars north polar region. ACTA ACUST UNITED AC 2007. [DOI: 10.1029/2006je002862] [Citation(s) in RCA: 77] [Impact Index Per Article: 4.5] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
|
13
|
Minitti ME, Weitz CM, Lane MD, Bishop JL. Morphology, chemistry, and spectral properties of Hawaiian rock coatings and implications for Mars. ACTA ACUST UNITED AC 2007. [DOI: 10.1029/2006je002839] [Citation(s) in RCA: 65] [Impact Index Per Article: 3.8] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
|
14
|
Keller JM, Boynton WV, Karunatillake S, Baker VR, Dohm JM, Evans LG, Finch MJ, Hahn BC, Hamara DK, Janes DM, Kerry KE, Newsom HE, Reedy RC, Sprague AL, Squyres SW, Starr RD, Taylor GJ, Williams RMS. Equatorial and midlatitude distribution of chlorine measured by Mars Odyssey GRS. ACTA ACUST UNITED AC 2006. [DOI: 10.1029/2006je002679] [Citation(s) in RCA: 39] [Impact Index Per Article: 2.2] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
|
15
|
Wang A, Korotev RL, Jolliff BL, Haskin LA, Crumpler L, Farrand WH, Herkenhoff KE, de Souza P, Kusack AG, Hurowitz JA, Tosca NJ. Evidence of phyllosilicates in Wooly Patch, an altered rock encountered at West Spur, Columbia Hills, by the Spirit rover in Gusev crater, Mars. ACTA ACUST UNITED AC 2006. [DOI: 10.1029/2005je002516] [Citation(s) in RCA: 26] [Impact Index Per Article: 1.4] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Affiliation(s)
- Alian Wang
- Department of Earth and Planetary Sciences and McDonnell Center for Space Science; Washington University in St. Louis; St. Louis Missouri USA
| | - Randy L. Korotev
- Department of Earth and Planetary Sciences and McDonnell Center for Space Science; Washington University in St. Louis; St. Louis Missouri USA
| | - Bradley L. Jolliff
- Department of Earth and Planetary Sciences and McDonnell Center for Space Science; Washington University in St. Louis; St. Louis Missouri USA
| | - Larry A. Haskin
- Department of Earth and Planetary Sciences and McDonnell Center for Space Science; Washington University in St. Louis; St. Louis Missouri USA
| | - Larry Crumpler
- New Mexico Museum of Natural History and Science; Albuquerque New Mexico USA
| | | | | | | | | | - Joel A. Hurowitz
- Department of Geosciences; State University of New York; Stony Brook New York USA
| | - Nicholas J. Tosca
- Department of Geosciences; State University of New York; Stony Brook New York USA
| |
Collapse
|
16
|
Affiliation(s)
- Amos Banin
- Department of Soil and Water Sciences, Hebrew University, Rehovot 76100, Israel, and SETI Institute, Mountain View, CA 94043, USA.
| |
Collapse
|
17
|
Langevin Y, Poulet F, Bibring JP, Gondet B. Sulfates in the North Polar Region of Mars Detected by OMEGA/Mars Express. Science 2005; 307:1584-6. [PMID: 15718428 DOI: 10.1126/science.1109091] [Citation(s) in RCA: 98] [Impact Index Per Article: 5.2] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/03/2022]
Abstract
The Observatoire pour la Minéralogie, l'Eau, les Glaces, et l'Activité (OMEGA) imaging spectrometer observed the northern circumpolar regions of Mars at a resolution of a few kilometers. An extended region at 240 degrees E, 85 degrees N, with an area of 60 kilometers by 200 kilometers, exhibits absorptions at wavelengths of 1.45, 1.75, 1.94, 2.22, 2.26, and 2.48 micrometers. These signatures can be unambiguously attributed to calcium-rich sulfates, most likely gypsum. This region corresponds to the dark longitudinal dunes of Olympia Planitia. These observations reveal that water alteration played a major role in the formation of the constituting minerals of northern circumpolar terrains.
Collapse
Affiliation(s)
- Yves Langevin
- Institut d'Astrophysique Spatiale (IAS), Bâtiment 121, 91405 Orsay Campus, France.
| | | | | | | |
Collapse
|
18
|
King PL, McSween HY. Effects of H2O, pH, and oxidation state on the stability of Fe minerals on Mars. ACTA ACUST UNITED AC 2005. [DOI: 10.1029/2005je002482] [Citation(s) in RCA: 124] [Impact Index Per Article: 6.5] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022]
|
19
|
Klingelhöfer G, Morris RV, Bernhardt B, Schröder C, Rodionov DS, de Souza PA, Yen A, Gellert R, Evlanov EN, Zubkov B, Foh J, Bonnes U, Kankeleit E, Gütlich P, Ming DW, Renz F, Wdowiak T, Squyres SW, Arvidson RE. Jarosite and Hematite at Meridiani Planum from Opportunity's Mössbauer Spectrometer. Science 2004; 306:1740-5. [PMID: 15576610 DOI: 10.1126/science.1104653] [Citation(s) in RCA: 193] [Impact Index Per Article: 9.7] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
Mossbauer spectra measured by the Opportunity rover revealed four mineralogical components in Meridiani Planum at Eagle crater: jarosite- and hematite-rich outcrop, hematite-rich soil, olivine-bearing basaltic soil, and a pyroxene-bearing basaltic rock (Bounce rock). Spherules, interpreted to be concretions, are hematite-rich and dispersed throughout the outcrop. Hematitic soils both within and outside Eagle crater are dominated by spherules and their fragments. Olivine-bearing basaltic soil is present throughout the region. Bounce rock is probably an impact erratic. Because jarosite is a hydroxide sulfate mineral, its presence at Meridiani Planum is mineralogical evidence for aqueous processes on Mars, probably under acid-sulfate conditions.
Collapse
Affiliation(s)
- G Klingelhöfer
- Institut für Anorganische und Analytische Chemie, Johannes Gutenberg-Universität, Staudinger Weg 9, D-55128 Mainz, Germany.
| | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | |
Collapse
|
20
|
Klingelhöfer G, Morris RV, Bernhardt B, Rodionov D, de Souza PA, Squyres SW, Foh J, Kankeleit E, Bonnes U, Gellert R, Schröder C, Linkin S, Evlanov E, Zubkov B, Prilutski O. Athena MIMOS II Mössbauer spectrometer investigation. ACTA ACUST UNITED AC 2003. [DOI: 10.1029/2003je002138] [Citation(s) in RCA: 189] [Impact Index Per Article: 9.0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Affiliation(s)
- G. Klingelhöfer
- Institute for Inorganic and Analytical Chemistry; Johannes Gutenberg University; Mainz Germany
| | | | - B. Bernhardt
- Institute for Inorganic and Analytical Chemistry; Johannes Gutenberg University; Mainz Germany
| | - D. Rodionov
- Institute for Inorganic and Analytical Chemistry; Johannes Gutenberg University; Mainz Germany
- Space Research Institute IKI; Moscow Russia
| | - P. A. de Souza
- Institute for Inorganic and Analytical Chemistry; Johannes Gutenberg University; Mainz Germany
- Pelletizing Department; Companhia Vale do Rio Doce; Vitoria Brazil
| | - S. W. Squyres
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - J. Foh
- Institute for Inorganic and Analytical Chemistry; Johannes Gutenberg University; Mainz Germany
| | - E. Kankeleit
- Nuclear Physics Institute; Darmstadt University of Technology; Darmstadt Germany
| | - U. Bonnes
- Nuclear Physics Institute; Darmstadt University of Technology; Darmstadt Germany
| | - R. Gellert
- Institute for Inorganic and Analytical Chemistry; Johannes Gutenberg University; Mainz Germany
| | - C. Schröder
- Institute for Inorganic and Analytical Chemistry; Johannes Gutenberg University; Mainz Germany
| | - S. Linkin
- Space Research Institute IKI; Moscow Russia
| | - E. Evlanov
- Space Research Institute IKI; Moscow Russia
| | - B. Zubkov
- Space Research Institute IKI; Moscow Russia
| | | |
Collapse
|
21
|
Bell JF, McSween HY, Crisp JA, Morris RV, Murchie SL, Bridges NT, Johnson JR, Britt DT, Golombek MP, Moore HJ, Ghosh A, Bishop JL, Anderson RC, Brückner J, Economou T, Greenwood JP, Gunnlaugsson HP, Hargraves RM, Hviid S, Knudsen JM, Madsen MB, Reid R, Rieder R, Soderblom L. Mineralogic and compositional properties of Martian soil and dust: Results from Mars Pathfinder. ACTA ACUST UNITED AC 2000. [DOI: 10.1029/1999je001060] [Citation(s) in RCA: 230] [Impact Index Per Article: 9.6] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
|
22
|
Morris RV, Golden DC, Bell JF, Shelfer TD, Scheinost AC, Hinman NW, Furniss G, Mertzman SA, Bishop JL, Ming DW, Allen CC, Britt DT. Mineralogy, composition, and alteration of Mars Pathfinder rocks and soils: Evidence from multispectral, elemental, and magnetic data on terrestrial analogue, SNC meteorite, and Pathfinder samples. ACTA ACUST UNITED AC 2000. [DOI: 10.1029/1999je001059] [Citation(s) in RCA: 257] [Impact Index Per Article: 10.7] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
|
23
|
|