Search results for " martian"

showing 2 items of 2 documents

Secondary minerals from salt caves in the Atacama Desert (Chile): a hyperarid and hypersaline environment with potential analogies to the Martian sub…

2017

Over the past 15 years several expeditions by French, American and especially Italian cavers have unveiled over 50 caves in the Cordillera de la Sal (Atacama Desert, Northern Chile). Many of these caves contain a variety of speleothems and minerals, some of which have rarely been observed within karst systems. Most of the secondary deposits in these caves are composed of halite, but also other halide, carbonate, sulphate, nitrate, phosphate, and silicate minerals have been found. Among the sixteen cave mineral species recognized, atacamite, darapskite, blödite, leonite, anhydrite, and especially antarcticite are worth mentioning. In one of the samples an unknown Ca-Sr-bearing chloride miner…

010504 meteorology & atmospheric sciencesQH301-705.5Settore GEO/04 - Geografia Fisica E GeomorfologiaEarth scienceSalt (chemistry)martian010502 geochemistry & geophysics01 natural sciencesAstrobiologyatacamaCaveminerogenesisMinerogenesiBiology (General)Hyperaridity0105 earth and related environmental sciencesEarth-Surface Processescave mineralschemistry.chemical_classificationMartianQE1-996.5Settore GEO/06 - Mineralogiageographygeography.geographical_feature_categoryDesert (philosophy)Mars analoguesMars analogueCave mineralGeologysalt cavescave minerals atacama martianchemistrySalt cavecave minerals salt caves hyperaridity minerogenesis Mars analoguesGeologyInternational Journal of Speleology
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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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