Search results for "Mars Exploration Program"

showing 10 items of 63 documents

Quartz OSL dating of late quaternary Chinese and Serbian loess: A cross Eurasian comparison of dust mass accumulation rates

2019

© 2018 Elsevier Ltd and INQUA. Reconstructing dust Mass Accumulation Rate (MAR) from loess deposits is critical to understanding past atmospheric mineral dust activity and requires accurate independent age models from loess deposits across Europe and Asia. Previous correlations of loess in Europe and China have tended to focus on multi-millennial timescales, with no detailed examination of dust MAR at the two ends of the Eurasian loess belt on shorter, sub-orbital scales. Here we present a detailed quartz optically stimulated luminescence (OSL) chronology from the Serbian Titel Loess Plateau (Veliki Surduk loess core) and the Chinese Loess Plateau (Lingtai section). The luminescence ages pa…

010506 paleontologyTitel loess plateau010504 meteorology & atmospheric sciencesOptically stimulated luminescenceOSL datingGeochemistryLoessDustMars Exploration ProgramMineral dust01 natural sciencesMARLoessChinese Loess PlateauGlacial periodQuaternary[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]QuartzGeologyComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciencesEarth-Surface ProcessesChronology
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Report of the COSPAR Mars special regions colloquium

2010

International audience; In this paper we present the findings of a COSPAR Mars Special Regions Colloquium held in Rome in 2007. We review and discuss the definition of Mars Special Regions, the physical parameters used to define Mars Special Regions, and physical features on Mars that can be interpreted as Mars Special Regions. We conclude that any region experiencing temperatures > -25 degrees C for a few hours a year and a water activity > 0.5 can potentially allow the replication of terrestrial microorganisms. Physical features on Mars that can be interpreted as meeting these conditions constitute a Mars Special Region. Based on current knowledge of the martian environment and the conser…

Atmospheric Science010504 meteorology & atmospheric sciencesPlanetary protectionLiquid waterAerospace EngineeringTerrainBACTERIAL-ACTIVITY01 natural sciencesSPACECRAFT SURFACESAstrobiologyWater-vaporSouth-pole snow0103 physical sciencesBacterial activitySpace research010303 astronomy & astrophysicsBacterial activity0105 earth and related environmental sciencesMartianCommittee on Space ResearchCOSPAR mars special regions colloquiumNear-surfaceAstronomy and AstrophysicsMars Exploration Program15. Life on landGround ice[PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph]GeophysicsLiquid water13. Climate actionSpace and Planetary ScienceGeneral Earth and Planetary SciencesHigh obliquitySea-iceUpper martian surfaceSpace-craft surfacesGeology
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FIDO science payload simulating the Athena Payload

2002

[1] The Jet Propulsion Laboratory's Field Integrated Development and Operations rover (FIDO) emulates and tests operational rover capabilities for advanced Mars rover missions, such as those originally planned for the Mars Surveyor 2001 Rover and currently planned for the Athena Payload on the Mars Exploration Rovers scheduled for launch in 2003. This paper describes FIDO's science instrument payload, which is fully integrated with rover hardware and software. Remote science teams visualize instrument suite data and generate FIDO commands using the Web Interface for Telescience. FIDO's instrument suite has been used in terrestrial laboratory and field tests to simulate Mars operations, to t…

Atmospheric ScienceComputer scienceSoil ScienceAquatic ScienceOceanographyExploration of Marslaw.inventionSoftwareGeochemistry and PetrologylawEarth and Planetary Sciences (miscellaneous)Earth-Surface ProcessesWater Science and TechnologyRemote sensingEcologySpectrometerbusiness.industryPaleontologyForestryMars Exploration ProgramRobot end effectorMars roverGeophysicsStereo imagingSpace and Planetary ScienceRadiancebusinessJournal of Geophysical Research: Planets
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Spirit Mars Rover Mission: Overview and selected results from the northern Home Plate Winter Haven to the side of Scamander crater

2010

Spirit Mars Rover Mission : Overview and selected results from the northern Home Plate Winter Haven to the side of Scamander crater

Atmospheric ScienceEcologyEarth sciencePaleontologySoil ScienceMars exploration roverForestryMars Exploration ProgramAquatic ScienceOceanographyExploration of MarsHavenAstrobiologyMars roverGeophysicsImpact craterSpace and Planetary ScienceGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)GeologyEarth-Surface ProcessesWater Science and TechnologyJournal of Geophysical Research
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Meteorites on Mars observed with the Mars Exploration Rovers

2008

[1] Reduced weathering rates due to the lack of liquid water and significantly greater typical surface ages should result in a higher density of meteorites on the surface of Mars compared to Earth. Several meteorites were identified among the rocks investigated during Opportunity's traverse across the sandy Meridiani plains. Heat Shield Rock is a IAB iron meteorite and has been officially recognized as “Meridiani Planum.” Barberton is olivine-rich and contains metallic Fe in the form of kamacite, suggesting a meteoritic origin. It is chemically most consistent with a mesosiderite silicate clast. Santa Catarina is a brecciated rock with a chemical and mineralogical composition similar to Bar…

Atmospheric ScienceEcologyPaleontologySoil ScienceForestryMars Exploration ProgramAquatic ScienceOceanographyIron meteoriteStrewn fieldAstrobiologyKamaciteMesosideriteGeophysicsImpact craterMeteoriteSpace and Planetary ScienceGeochemistry and PetrologyChondriteEarth and Planetary Sciences (miscellaneous)GeologyEarth-Surface ProcessesWater Science and TechnologyJournal of Geophysical Research
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Evidence for montmorillonite or its compositional equivalent in Columbia Hills, Mars

2007

During its exploration of the Columbia Hills, the Mars Exploration Rover ‘‘Spirit’’ encountered several similar samples that are distinctly different from Martian meteorites and known Gusev crater soils, rocks, and sediments. Occurring in a variety of contexts and locations, these ‘‘Independence class’’ samples are rough-textured, iron-poor (equivalent FeO 4 wt%), have high Al/Si ratios, and often contain unexpectedly high concentrations of one or more minor or trace elements (including Cr, Ni, Cu, Sr, and Y). Apart from accessory minerals, the major component common to these samples has a compositional profile of major and minor elements whic…

Atmospheric ScienceGeochemistryMarsSoil ScienceMineralogymontmorilloniteAquatic ScienceOceanographychemistry.chemical_compoundImpact craterGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)chemical compositionEarth-Surface ProcessesWater Science and TechnologyGusevMineralEcologyPaleontologyForestryColumbia HillsclayMars Exploration ProgramMars explorationSilicateGeophysicsMontmorilloniteMeteoritechemistrySpace and Planetary ScienceroverGusev CraterSoil horizonClay mineralsGeologyJournal of Geophysical Research
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Depth selective Mössbauer spectroscopy: Analysis and simulation of 6.4 keV and 14.4 keV spectra obtained from rocks at Gusev Crater, Mars, and layere…

2008

[1] The miniaturized Mossbauer spectrometer (MIMOS) II Mossbauer spectrometers on the Mars Exploration Rovers (MER) simultaneously obtained 6.4 keV and 14.4 keV Mossbauer spectra from rock and soil targets. Because photons with lower energy have a shallower penetration depth, 6.4 keV spectra contain more mineralogical information about the near-surface region of a sample than do 14.4 keV spectra. The influence of surface layers of varying composition and thickness on Mossbauer spectra was investigated by Monte Carlo simulation and by measurement using a copy of the MER MIMOS II instrument and samples with one or two layers of known thicknesses. Thin sections of minerals or metallic Fe foil …

Atmospheric ScienceMaterials scienceMonte Carlo methodSoil ScienceMineralogyAquatic Scienceengineering.materialOceanographyPhysics::GeophysicsGeochemistry and PetrologyMössbauer spectroscopyEarth and Planetary Sciences (miscellaneous)Surface layerPenetration depthEarth-Surface ProcessesWater Science and TechnologyThin layersOlivineEcologySpectrometerPaleontologyForestryMars Exploration ProgramGeophysicsSpace and Planetary ScienceengineeringJournal of Geophysical Research
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Overview of the magnetic properties experiments on the Mars Explorations Rovers

2009

[1] The Mars Exploration Rovers have accumulated airborne dust on different types of permanent magnets. Images of these magnets document the dynamics of dust capture and removal over time. The strongly magnetic subset of airborne dust appears dark brown to black in Panoramic Camera (Pancam) images, while the weakly magnetic one is bright red. Images returned by the Microscopic Imager reveal the formation of magnetic chains diagnostic of magnetite-rich grains with substantial magnetization (>8 Am2 kg−1). On the basis of Mossbauer spectra the dust contains magnetite, olivine, pyroxene, and nanophase oxides in varying proportions, depending on wind regime and landing site. The dust contains a …

Atmospheric ScienceSoil ScienceMineralogyPyroxeneAquatic Scienceengineering.materialOceanographychemistry.chemical_compoundMagnetizationGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)Earth-Surface ProcessesWater Science and TechnologyMagnetiteBasaltOlivineEcologySpinelPaleontologyForestryMars Exploration Programequipment and suppliesSilicateGeophysicschemistrySpace and Planetary ScienceengineeringGeology
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Spirit Mars Rover Mission to the Columbia Hills, Gusev Crater: Mission overview and selected results from the Cumberland Ridge to Home Plate

2008

This paper summarizes the Spirit rover operations in the Columbia Hills of Gusev Crater from sols 513 to 1476 and provides an overview of selected findings that focus on synergistic use of the Athena Payload and comparisons to orbital data. Results include discovery of outcrops (Voltaire) on Husband Hill that are interpreted to be altered impact melt deposits that incorporated local materials during emplacement. Evidence for extensive volcanic activity and aqueous alteration in the Inner Basin is also detailed, including discovery and characterization of accretionary lapilli and formation of sulfate, silica, and hematite-rich deposits. Use of Spirit's data to understand the range of spectra…

Atmospheric Sciencegeographygeography.geographical_feature_categoryEcologyWater on MarsPaleontologySoil ScienceForestryMars Exploration ProgramAquatic ScienceOceanographyExploration of MarsCRISMAstrobiologyMars roverGeophysicsVolcanoImpact craterSpace and Planetary ScienceGeochemistry and PetrologyRidgeEarth and Planetary Sciences (miscellaneous)GeologyEarth-Surface ProcessesWater Science and TechnologyJournal of Geophysical Research
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Visible and near-infrared multispectral analysis of geochemically measured rock fragments at the Opportunity landing site in Meridiani Planum

2010

[1] We have used visible and near-infrared Panoramic Camera (Pancam) spectral data acquired by the Opportunity rover to analyze 15 rock fragments at the Meridiani Planum landing site. These spectral results were then compared to geochemistry measurements made by the in situ instruments Mossbauer (MB) and Alpha Particle X-ray Spectrometer (APXS) to determine the feasibility of mineralogic characterization from Pancam data. Our results suggest that dust and alteration rinds coat many rock fragments, which limits our ability to adequately measure the mineralogy of some rocks from Pancam spectra relative to the different field of view and penetration depths of MB and APXS. Viewing and lighting …

BasaltMeridiani PlanumAtmospheric ScienceEcologyOutcropNear-infrared spectroscopyMultispectral imagePaleontologySoil ScienceMineralogyForestryMars Exploration ProgramAquatic ScienceOceanographyGeophysicsMeteoriteRock fragmentSpace and Planetary ScienceGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)GeologyEarth-Surface ProcessesWater Science and TechnologyJournal of Geophysical Research
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