0000000000798013

AUTHOR

M. Olsen

showing 4 related works from this author

Indication of drier periods on Mars from the chemistry and mineralogy of atmospheric dust

2005

The cover shows part of the Larry's Lookout panorama, seen from the Mars Exploration Rover (MER) Spirit during its drive up Husband Hill: the summit is about 200 metres from the rover. Six papers this week report in detail on the MER mission. An Analysis compares predictions used to select a landing site with the conditions actually encountered. This ‘ground truth’ will be invaluable for interpreting future remote-sensing data. Surface chemistry suggests that the upper layer of soil may contain 1% meteoritic material. MER provides a unique glimpse of solar transits of the moons Phobos and Deimos. Rover Opportunity examined wind-related processes, and spectroscopy indicates a dry origin for …

Moons of MarsBasaltMultidisciplinaryImpact craterDust stormMineralogyContext (language use)Mars Exploration ProgramAtmosphere of MarsExploration of MarsAstrobiologyNature
researchProduct

Search for magnetic minerals in Martian rocks: Overview of the Rock Abrasion Tool (RAT) magnet investigation on Spirit and Opportunity

2008

[1] The Rock Abrasion Tool (RAT) on board the Mars Exploration Rovers (MER) is a grinding tool designed to remove dust coatings and/or weathering rinds from rocks and expose fresh rock material. Four magnets of different strengths that are built into the structure of the RAT have been attracting substantial amounts of magnetic material during RAT activities from rocks throughout both rover missions. The RAT magnet experiment as performed on Spirit demonstrates the presence of a strongly ferrimagnetic phase in Gusev crater rocks, which based on Mossbauer and visible/near-infrared reflectance spectra is interpreted as magnetite. The amount of abraded rock material adhering to the magnets vari…

MartianAtmospheric ScienceEcologyPaleontologySoil ScienceMineralogyForestryWeatheringMars Exploration ProgramAquatic ScienceOceanographyAbrasion (geology)chemistry.chemical_compoundMagnetizationGeophysicschemistryImpact craterSpace and Planetary ScienceGeochemistry and PetrologyFerrimagnetismEarth and Planetary Sciences (miscellaneous)GeologyEarth-Surface ProcessesWater Science and TechnologyMagnetiteJournal of Geophysical Research
researchProduct

Poster contributions

1989

Nuclear and High Energy PhysicsMaterials sciencePhysical and Theoretical ChemistryCondensed Matter PhysicsAtomic and Molecular Physics and OpticsHyperfine Interactions
researchProduct

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
researchProduct