Search results for "Mars Exploration Program"

showing 10 items of 63 documents

Bounce Rock-A shergottite-like basalt encountered at Meridiani Planum, Mars

2011

Additional co-authors: Thanasis ECONOMOU, Steven P. GOREVAN, Brian C. HAHN, Gostar KLINGELHOFER, Timothy J. McCOY, Harry Y. McSWEEN Jr, Douglas W. MING, Richard V. MORRIS, Daniel S. RODIONOV, Steven W. SQUYRES, Heinrich WANKE, Shawn P. WRIGHT, Michael B. WYATT, Albert S. YEN

BasaltMeridiani PlanumGeophysicsWater on MarsSpace and Planetary ScienceComposition of MarsMars Exploration ProgramGeologyAstrobiologyMeteoritics & Planetary Science
researchProduct

Fe Mossbauer spectroscopy as a tool in astrobiology

2006

The element Fe and Fe-bearing minerals occur ubiquitously throughout the field of astrobiology. Cycling between the various oxidation states of Fe provides a source of energy available for life. Banded iron formations may record the rise of oxygenic photosynthesis. The distribution of Fe between Fe-bearing minerals and its oxidation states can help to characterize and understand ancient environments with respect to the suitability for life by constraining the primary rock type and the redox conditions under which it crystallized, the extent of alteration and weathering, the type of alteration and weathering products, and the processes and environmental conditions for alteration and weatheri…

BasaltMeridiani PlanumMaterials scienceGoethiteMössbauer spectroscopyastrobiologyMarsAstronomy and AstrophysicsWeatheringMars Exploration Programengineering.materialHematitehydrothermal ventAstrobiologySpace and Planetary Sciencebiogeochemistryvisual_artJarositevisual_art.visual_art_mediumengineeringBanded iron formation
researchProduct

Spectral, mineralogical, and geochemical variations across Home Plate, Gusev Crater, Mars indicate high and low temperature alteration

2009

Over the last ~3 years in Gusev Crater, Mars, the Spirit rover observed coherent variations in color, mineralogy, and geochemistry across Home Plate, an ~80 m-diameter outcrop of basaltic tephra. Observations of Home Plate from orbit and from the summit of Husband Hill reveal clear differences in visible/near-infrared (VNIR) colors between its eastern and western regions that are consistent with mineralogical compositions indicated by Mössbauer spectrometer (MB) and by Miniature Thermal Emission Spectrometer (Mini-TES). Pyroxene and magnetite dominate the east side, while olivine, nanophase Fe oxide (npOx) and glass are more abundant on the western side. Alpha Particle X-Ray Spectromet…

BasaltOlivineThermal Emission SpectrometerRecrystallization (geology)GeochemistryMineralogyMars Exploration ProgramPyroxeneengineering.materialMars geologyGeophysicsImpact craterSpace and Planetary ScienceGeochemistry and PetrologyGusev CraterEarth and Planetary Sciences (miscellaneous)engineeringhydrothermal alterationTephraGeologyEarth and Planetary Science Letters
researchProduct

The Spirit Rover's Athena science investigation at Gusev Crater, Mars.

2004

The Mars Exploration Rover Spirit and its Athena science payload have been used to investigate a landing site in Gusev crater. Gusev is hypothesized to be the site of a former lake, but no clear evidence for lacustrine sedimentation has been found to date. Instead, the dominant lithology is basalt, and the dominant geologic processes are impact events and eolian transport. Many rocks exhibit coatings and other characteristics that may be evidence for minor aqueous alteration. Any lacustrine sediments that may exist at this location within Gusev apparently have been buried by lavas that have undergone subsequent impact disruption.

BasaltgeographyGeologic SedimentsGeological PhenomenaMineralsMultidisciplinarygeography.geographical_feature_categoryExtraterrestrial EnvironmentLithologyAtmosphereMarsWaterGeologyMars Exploration ProgramWindGeologic SedimentsAstrobiologyVolcanic rockIgneous rockMagneticsImpact craterComposition of MarsGeologyScience (New York, N.Y.)
researchProduct

Martian zeolites as a source of atmospheric methane

2016

The origin of the martian methane is still poorly understood. A plausible explanation is that methane could have been produced either by hydrothermal alteration of basaltic crust or by serpentinization of ultramafic rocks producing hydrogen and reducing crustal carbon into methane. Once formed, methane storage on Mars is commonly associated with the presence of hidden clathrate reservoirs. Here, we alternatively suggest that chabazite and clinoptilolite, which belong to the family of zeolites, may form a plausible storage reservoir of methane in the martian subsurface. Because of the existence of many volcanic terrains, zeolites are expected to be widespread on Mars and their Global Equival…

Chabazite010504 meteorology & atmospheric sciencesClathrate hydrateFOS: Physical sciences01 natural sciencesMethaneAstrobiologychemistry.chemical_compound0103 physical sciences010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciencesEarth and Planetary Astrophysics (astro-ph.EP)BasaltMartianAtmospheric methaneAstronomy and AstrophysicsMars Exploration ProgramAtmosphere of Marschemistry13. Climate actionSpace and Planetary Science[SDU]Sciences of the Universe [physics]Environmental science[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph][ SDU ] Sciences of the Universe [physics]Astrophysics - Earth and Planetary Astrophysics
researchProduct

Do soils exist outside Earth?

2010

Abstract On Earth, soils form thanks to the combined action of at least five factors: parent rock, climate, topography, biota, and time. However, the necessity of biota as unavoidable soil forming factor is debated, as important parts of our planet experiencing extreme climates host virtually life-free soils with advanced horizonation. Now that space exploration has greatly expanded our understanding of the Solar System, providing consistent evidences that the loose, unconsolidated "skin" of some nearby rocky bodies is lifeless, it is time to establish if the latter can be considered to be soil in a pedological sense. Our feeling is that, since the concept of soil chiefly bases on the occur…

Earth scienceSettore ING-IND/05 - Impianti E Sistemi AerospazialiAstronomy and AstrophysicsWeatheringBiotaGeophysicsMars Exploration ProgramRegolithSoil Regolith Solar System Weathering PedologySettore AGR/14 - PedologiaSpace and Planetary ScienceSoil waterEarth (chemistry)PedologyParent rockGeologyPlanetary and Space Science
researchProduct

A numerical study of the Schumann resonances in Mars with the FDTD method

2007

[1] Natural electromagnetic waves generated near the surface by electrostatic discharges in dust storms (dust devils) or by geological activity could be trapped in the resonant cavity formed by the surface and lower ionosphere of Mars, as it occurs on Earth giving rise to Schumann resonances. The finite difference time-domain technique (FDTD) is applied to model the atmosphere of Mars in order to determine Schumann resonant frequencies, and natural electromagnetic fields at the extremely low frequency range (ELF). A numerical tool is provided to analyze the electrical conductivity profile of the Martian atmosphere, with the aim of obtaining Schumann resonance frequencies and their dependenc…

Electromagnetic fieldAtmospheric ScienceSoil ScienceAquatic ScienceOceanographyElectromagnetic radiationAtmosphereOpticsGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)Extremely low frequencyEarth-Surface ProcessesWater Science and TechnologyPhysicsEcologySchumann resonancesbusiness.industryPaleontologyForestryMars Exploration ProgramAtmosphere of MarsComputational physicsGeophysicsSpace and Planetary SciencePhysics::Space PhysicsAstrophysics::Earth and Planetary AstrophysicsIonospherebusinessJournal of Geophysical Research: Space Physics
researchProduct

Entertainment virtual reality system for simulation of spaceflights over the surface of the planet Mars

2006

In recent years Virtual Reality technologies have enabled astronomers to recreate and explore three dimensional structures of the Universe for scientific purposes. Mars, due to its scientific interest,has been the focal point of numerous research projects using these technologies, however, none of these virtual reality tools have been developed specifically for entertainment purposes.The focus of this paper is to present MarsVR, as an entertainment research project that educates people on the topography and orography of the planet Mars from the perspective of popular science. Some projects have been designed MarsVR for entertainment purposes and include the latest advances in 3D real time a…

EntertainmentFocus (computing)MultimediaComputer scienceVirtual machineMars Exploration ProgramVirtual realityPlanet Marscomputer.software_genrePopular sciencecomputerMixed realityProceedings of the ACM symposium on Virtual reality software and technology
researchProduct

Astrobiology of life on Earth

2021

Astrobiology is mistakenly regarded by some as a field confined to studies of life beyond Earth. Here, we consider life on Earth through an astrobiological lens. Whereas classical studies of microbiology historically focused on various anthropocentric sub-fields (such as fermented foods or commensals and pathogens of crop plants, livestock and humans), addressing key biological questions via astrobiological approaches can further our understanding of all life on Earth. We highlight potential implications of this approach through the articles in this Environmental Microbiology special issue ‘Ecophysiology of Extremophiles’. They report on the microbiology of places/processes including low-te…

Extraterrestrial EnvironmentEarth Planetterrestrial life.BiologyMicrobiologyAstrobiology[SDU] Sciences of the Universe [physics]/dk/atira/pure/sustainabledevelopmentgoals/life_below_water03 medical and health sciencesMicrobial ecologyhalophilesExobiologyEnvironmental MicrobiologyExtremophileHumansSDG 14 - Life Below WaterEcology Evolution Behavior and SystematicsEcosystemextremophiles030304 developmental biology2. Zero hunger0303 health sciencesExtremophile Viruses030306 microbiologyterrestrial lifeBiosphereMars Exploration Program15. Life on landMars explorationAstrobiologyBiología y Biomedicina / BiologíahabitabilityHabitat13. Climate action[SDU]Sciences of the Universe [physics]planetary protectionEarth (chemistry)astrobiology; extremophiles; habitability; halophiles; Mars exploration; planetary protection; terrestrial lifeextremophilehalophile
researchProduct

Optimal slope units partitioning in landslide susceptibility mapping

2020

In landslide susceptibility modeling, the selection of the mapping units is a very relevant topic both in terms of geomorphological adequacy and suitability of the models and final maps. In this paper, a test to integrate pixels and slope units is presented. MARS (Multivariate Adaptive Regression Splines) modeling was applied to assess landslide susceptibility based on a 12 predictors and a 1608 cases database. A pixel-based model was prepared and the scores zoned into 10 different types of slope units, obtained by differently combining two half-basin (HB) and four landform classification (LCL) coverages. The predictive performance of the 10 models were then compared to select the best perf…

G3180-9980010504 meteorology & atmospheric sciencesGeography Planning and DevelopmentLand managementland managementimera settentrionale river basin (sicily)Mars Exploration ProgramLandslide susceptibility010502 geochemistry & geophysics01 natural sciencesmapping unitsImera Settentrionale river basin (Sicily) land management Landslide susceptibility mapping units MARSMapsEarth and Planetary Sciences (miscellaneous)landslide susceptibilitymarsCartographyGeologySelection (genetic algorithm)0105 earth and related environmental sciences
researchProduct