0000000000252844

AUTHOR

John Parnell

showing 2 related works from this author

Identification of Morphological Biosignatures in Martian Analogue Field Specimens Using In Situ Planetary Instrumentation

2008

International audience; We have investigated how morphological biosignatures (i.e., features related to life) might be identified with an array of viable instruments within the framework of robotic planetary surface operations at Mars. This is the first time such an integrated lab-based study has been conducted that incorporates space-qualified instrumentation designed for combined in situ imaging, analysis, and geotechnics ( sampling). Specimens were selected on the basis of feature morphology, scale, and analogy to Mars rocks. Two types of morphological criteria were considered: potential signatures of extinct life ( fossilized microbial filaments) and of extant life (crypto-chasmoendolit…

Meridiani PlanumIn situGeologic Sediments010504 meteorology & atmospheric sciencesMOSSBAUER-SPECTROSCOPYInstrumentationOrigin of LifeAntarctic RegionsMarsGUSEV CRATERExploration of MarsCalcium Sulfate01 natural sciencesCRYPTOENDOLITHIC LICHENSCalcium CarbonateAstrobiologyRAMAN-SPECTROSCOPIC DETECTIONGermanyExobiology0103 physical sciences010303 astronomy & astrophysics0105 earth and related environmental sciencesRemote sensingMartianMineralsPlanetary surfaceSpectrometerMERIDIANI-PLANUMWESTERN-AUSTRALIAMars Exploration ProgramAgricultural and Biological Sciences (miscellaneous)YELLOWSTONE-NATIONAL-PARK13. Climate actionSpace and Planetary ScienceMARS EXPLORATIONAmericasANTARCTIC HABITATSIron CompoundsGeologyHAUGHTON IMPACT STRUCTUREAstrobiology
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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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