Search results for " MARS"

showing 10 items of 163 documents

Field reconnaissance geologic mapping of the Columbia Hills, Mars, based on Mars Exploration Rover Spirit and MRO HiRISE observations

2011

Chemical, mineralogic, and lithologic ground truth was acquired for the first time on Mars in terrain units mapped using orbital Mars Reconnaissance Orbiter's High Resolution Imaging Science Experiment (MRO HiRISE) image data. Examination of several dozen outcrops shows that Mars is geologically complex at meter length scales, the record of its geologic history is well exposed, stratigraphic units may be identified and correlated across significant areas on the ground, and outcrops and geologic relationships between materials may be analyzed with techniques commonly employed in terrestrial field geology. Despite their burial during the course of Martian geologic time by widespread epiclasti…

MartianAtmospheric ScienceEcologyWater on MarsOutcropEarth scienceGeochemistryPaleontologySoil ScienceForestryEvidence of water on Mars from Mars OdysseyMars Exploration ProgramAquatic ScienceOceanographyGeologic recordGeologic mapGeophysicsSpace and Planetary ScienceGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)Period (geology)GeologyEarth-Surface ProcessesWater Science and TechnologyJournal of Geophysical Research
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The new Athena alpha particle X-ray spectrometer for the Mars Exploration Rovers

2003

[1] The new alpha particle X-ray spectrometer (APXS) is part of the Athena payload of the two Mars Exploration Rovers (MER). The APXS sensor head is attached to the turret of the instrument deployment device (IDD) of the rover. The APXS is a very light-weight instrument for determining the major and minor elemental composition of Martian soils, rocks, and other geological materials at the MER landing sites. The sensor head has simply to be docked by the IDD on the surface of the selected sample. X-ray radiation, excited by alpha particles and X rays of the radioactive sources, is recorded by a high-resolution X-ray detector. The X-ray spectra show elements starting from sodium up to yttrium…

MartianMeridiani PlanumAtmospheric ScienceEcologySpectrometerPaleontologySoil ScienceMineralogyForestryAlpha particleMars Exploration ProgramAquatic ScienceAlpha particle X-ray spectrometerOceanographyExploration of MarsAstrobiologyGeophysicsSpace and Planetary ScienceGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)Composition of MarsGeologyEarth-Surface ProcessesWater Science and TechnologyJournal of Geophysical Research: Planets
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Weathering of Fe-bearing minerals under Martian conditions, investigated by Mössbauer spectroscopy

2004

Abstract The surface of Mars is covered by weathered material. Mars' rusty red colour in particular is commonly ascribed to ferric iron-bearing minerals. The planet's surface is generally iron rich. Mossbauer spectroscopy is a powerful tool for quantitative mineralogical analysis of Fe-bearing minerals. Consequently, the miniaturized Mossbauer spectrometer MIMOS II is part of the payload of NASA's twin Mars Exploration Rovers “Spirit” and “Opportunity”, and ESA's ill-fated Mars Express lander “Beagle 2”. Both Mars Exploration Rovers are currently conducting successful surface operations on Mars. In this paper, we give a brief insight into mission operations with respect to the reconstructio…

MartianMineralOre resources on MarsMeteoriteSpace and Planetary ScienceAstronomy and AstrophysicsComposition of MarsWeatheringMars Exploration ProgramExploration of MarsGeologyAstrobiologyPlanetary and Space Science
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Identification of carbonate-rich outcrops on Mars by the Spirit rover.

2010

Ancient Carbonate Minerals on Mars The historical presence of liquid water on Mars together with a CO 2 -rich atmosphere should have resulted in the accumulation of large deposits of carbonate minerals. Yet, evidence for the presence of carbonates on the surface of Mars has been scarce. Using data collected by the Mars Exploration Rover, Spirit, Morris et al. (p. 421 , published online 3 June; see the Perspective by Harvey ) now present evidence for carbonate-rich outcrops in the Comanche outcrops within the Gusev crater. The carbonate is a major outcrop component and may have formed in the Noachian era (∼4 billion years ago) by precipitation from hydrothermal solutions that passed through …

MartianMultidisciplinaryWater on MarsExtraterrestrial EnvironmentAtmosphereClimateNoachianCarbonate mineralsCarbonatesTemperatureMarsWaterMars Exploration ProgramMeteoroidsCarbon DioxideAstrobiologychemistry.chemical_compoundImpact craterMeteoritechemistryCarbonateMagnesiumFerrous CompoundsSpacecraftGeologyScience (New York, N.Y.)
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Multi proxy analysis for reconstructing the late Holocene evolution of a Mediterranean Coastal Lagoon: Environmental variables within foraminiferal a…

2020

Abstract This study reconstructs the evolution of foraminiferal assemblages and the environmental variables (type of substrate, content in calcium carbonate and content in organic matter) in the Valencia lagoon (western Mediterranean) in response to changes in the late Holocene. In this area of low tidal range, several multiproxy analyses were carried out to determine which environmental variables influence the distribution of the fossil assemblage, and its association with global, regional or local climatic phenomena. The statistical results show that in environments with higher exposure to marine conditions, the calcium carbonate content is the dominant factor, whereas in more restricted …

Mediterranean climategeographygeography.geographical_feature_categoryTidal range010504 meteorology & atmospheric sciencesBrackish waterFluvial04 agricultural and veterinary sciences01 natural sciencesSubstrate (marine biology)OceanographyBrackish marsh040103 agronomy & agriculture0401 agriculture forestry and fisheriesProgradationHoloceneGeology0105 earth and related environmental sciencesEarth-Surface ProcessesCATENA
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Athena MIMOS II Mössbauer spectrometer investigation

2003

[1] Mossbauer spectroscopy is a powerful tool for quantitative mineralogical analysis of Fe-bearing materials. The miniature Mossbauer spectrometer MIMOS II is a component of the Athena science payload launched to Mars in 2003 on both Mars Exploration Rover missions. The instrument has two major components: (1) a rover-based electronics board that contains power supplies, a dedicated central processing unit, memory, and associated support electronics and (2) a sensor head that is mounted at the end of the instrument deployment device (IDD) for placement of the instrument in physical contact with soil and rock. The velocity transducer operates at a nominal frequency of ∼25 Hz and is equipped…

Meridiani PlanumAtmospheric ScienceEcologySpectrometerInstrumentationPaleontologySoil ScienceMineralogyForestryMars Exploration ProgramAquatic ScienceOceanographyTemperature measurementGeophysicsSpace and Planetary ScienceGeochemistry and PetrologyMartian surfaceEarth and Planetary Sciences (miscellaneous)CalibrationComposition of MarsGeologyEarth-Surface ProcessesWater Science and TechnologyJournal of Geophysical Research: Planets
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Alpha Particle X-Ray Spectrometer (APXS): Results from Gusev crater and calibration report

2006

The chemical composition of rocks and soils on Mars analyzed during the Mars Exploration Rover Spirit Mission was determined by X-ray analyses with the Alpha Particle X-Ray Spectrometer (APXS). Details of the data analysis method and the instrument calibration are presented. Measurements performed on Mars to address geometry effects and background contributions are shown. Cross calibration measurements among several instrument sensors and sources are discussed. An unintentional swap of the two flight instruments is evaluated. New concentration data acquired during the first 470 sols of rover Spirit in Gusev Crater are presented. There are two geological regions, the Gusev plains and the Col…

Meridiani PlanumAtmospheric Sciencegeographygeography.geographical_feature_categoryEcologyPaleontologySoil ScienceMineralogyForestryWeatheringMars Exploration ProgramAquatic ScienceAlpha particle X-ray spectrometerOceanographyVolcanic rockGeophysicsImpact craterSpace and Planetary ScienceGeochemistry and PetrologyRocknestEarth and Planetary Sciences (miscellaneous)Composition of MarsGeologyEarth-Surface ProcessesWater Science and TechnologyJournal of Geophysical Research: Planets
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In situ evidence for an ancient aqueous environment at Meridiani Planum, Mars.

2004

Sedimentary rocks at Eagle crater in Meridiani Planum are composed of fine-grained siliciclastic materials derived from weathering of basaltic rocks, sulfate minerals (including magnesium sulfate and jarosite) that constitute several tens of percent of the rock by weight, and hematite. Cross-stratification observed in rock outcrops indicates eolian and aqueous transport. Diagenetic features include hematite-rich concretions and crystal-mold vugs. We interpret the rocks to be a mixture of chemical and siliciclastic sediments with a complex diagenetic history. The environmental conditions that they record include episodic inundation by shallow surface water, evaporation, and desiccation. The …

Meridiani PlanumGeologic SedimentsExtraterrestrial EnvironmentGeochemistryMineralogyMarsWeatheringengineering.materialFerric CompoundsLifeConcretionExobiologyComposition of MarsSpacecraftgeographyMineralsMultidisciplinarygeography.geographical_feature_categorySulfatesSilicatesSpectrum AnalysisWaterDiagenesisVolcanic rockengineeringSedimentary rockSiliciclasticGeologySulfurScience (New York, N.Y.)
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Jarosite and hematite at Meridiani Planum from Opportunity's Mossbauer Spectrometer.

2004

Mössbauer 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 proc…

Meridiani PlanumGeologic SedimentsExtraterrestrial EnvironmentOutcropMineralogyMagnesium CompoundsMarsengineering.materialFerric CompoundsSpectroscopy MossbauerImpact craterConcretionJarositeComposition of MarsSpacecraftMineralsMultidisciplinaryMineralSulfatesSilicatesWaterHematitevisual_artvisual_art.visual_art_mediumengineeringGeologyIron CompoundsScience (New York, N.Y.)
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The Opportunity Rover's Athena Science Investigation at Meridiani Planum, Mars

2004

The Mars Exploration Rover Opportunity has investigated the landing site in Eagle crater and the nearby plains within Meridiani Planum. The soils consist of fine-grained basaltic sand and a surface lag of hematite-rich spherules, spherule fragments, and other granules. Wind ripples are common. Underlying the thin soil layer, and exposed within small impact craters and troughs, are flat-lying sedimentary rocks. These rocks are finely laminated, are rich in sulfur, and contain abundant sulfate salts. Small-scale cross-lamination in some locations provides evidence for deposition in flowing liquid water. We interpret the rocks to be a mixture of chemical and siliciclastic sediments formed by e…

Meridiani PlanumGeologic SedimentsMineralsMultidisciplinaryExtraterrestrial EnvironmentAtmosphereSilicatesGeochemistryMarsWaterMineralogyWindMars Exploration Programengineering.materialFerric CompoundsDiagenesisImpact craterConcretionengineeringSiliciclasticSedimentary rockComposition of MarsSpacecraftEvolution PlanetaryGeologyScience
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