Search results for "Meteoroids"

showing 6 items of 6 documents

Did the ancient crenarchaeal viruses from the dawn of life survive exceptionally well the eons of meteorite bombardment?

2009

The viruses of Crenarchaeota are unexpectedly diverse in their morphologies, and most have no, or few, genes related to bacterial, eukaryal, euryarchaeal, or other crenarchaeal viruses. Though several different virus morphotypes have been discovered in enrichment cultures of microbial communities collected from geothermally heated environments around the world, the origins of such differences are unknown. We present a model that combines consideration of Earth's geological history, the early emergence of hyperthermophiles, and the early formation of viruses from primordial genes with the intent to explain this vast diversity of crenarchaeal viruses. Several meteorite- or flood basalt-induce…

Extinction eventArchaeal VirusesbiologyEcologyvirusesCrenarchaeotaMeteoroidsrespiratory systembiology.organism_classificationExtinction BiologicalAgricultural and Biological Sciences (miscellaneous)HyperthermophileMeteoriteSpace and Planetary ScienceCrenarchaeotaEvolutionary biologyHost-Pathogen Interactionshuman activitiesAstrobiology
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Cavezzo, the first Italian meteorite recovered by the PRISMA fireball network. Orbit, trajectory, and strewn-field

2020

ABSTRACT Two meteorite pieces have been recovered in Italy, near the town of Cavezzo (Modena), on 2020 January 4th. The associated fireball was observed on the evening of New Year’s Day 2020 by eight all-sky cameras of the PRISMA fireball network, a partner of FRIPON. The computed trajectory had an inclination angle of approximately 68° and a velocity at infinity of 12.8 km s−1. Together with the relatively low terminal height, estimated as 21.5 km, those values were indicating the significant possibility of a meteorite dropping event, as additionally confirmed by the non-zero residual total mass. The strewn-field was computed taking into account the presence of two bright light flashes, re…

meteoroids -methods: data analysis -techniques: image processing010502 geochemistry & geophysics01 natural sciencesStrewn fieldmeteorites0103 physical sciencesmeteorsmeteoroids010303 astronomy & astrophysicsmeteoroid0105 earth and related environmental sciencesPhysicsMeteoroidimage processing; meteorites; meteoroids; meteors; methods: data analysis; techniquesmeteorAstronomyAstronomy and Astrophysicsmethods: data analysismeteoriteimage processingMeteoriteSpace and Planetary Science[SDU]Sciences of the Universe [physics]data analysi [methods]TrajectoryOrbit (control theory)techniques
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Chemical abundances determined from meteor spectra II. Evidence for enlarged sodium abundances in meteoroids

2004

9 pages, 5 figures.-- Printed version published Mar 2004.

PhysicsAstrochemistryMeteoroidSodiumComet dustchemistry.chemical_elementTechniques: spectroscopicgeneral [Comets]Astronomy and AstrophysicsAstrobiologyspectroscopic [Techniques]Comets: generalInterplanetary dust cloudchemistryMeteoriteSpace and Planetary ScienceChondriteAbundance (ecology)Meteors meteoroidsAstrochemistry
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Quantitative colorimetric-imaging analysis of nickel in iron meteorites.

2011

A quantitative analytical imaging approach for determining the nickel content of metallic meteorites is proposed. The approach uses a digital image of a series of standard solutions of the nickel-dimethylglyoxime coloured chelate and a meteorite sample solution subjected to the same treatment as the nickel standards for quantitation. The image is processed with suitable software to assign a colour-dependent numerical value (analytical signal) to each standard. Such a value is directly proportional to the analyte concentration, which facilitates construction of a calibration graph where the value for the unknown sample can be interpolated to calculate the nickel content of the meteorite. The…

INGENIERIA DE LA CONSTRUCCIONbusiness.product_categoryCost effectivenessCalibration curveEconomicsAstronomyAnalytical chemistryImaging analysisStandard solutionCalibration graphsAnalytical ChemistryStandard solutionsDigital imageIron meteoritesSpectro-photometric methodSoftwareNickelCost benefit analysisNational Institutes of HealthProcess engineeringDigital cameraChemistryNumerical valuesMeteoroidsCamerasImageJChemistryAnalytical equipmentPublic domain softwaresSpectrophotometryMeteoriteMeasuring instrumentsColorimetrySpectrophotometersStandardsAnalyte concentrationSample (material)IronColorCost effectivenessArticleColorimetric analysisInstrumentation (computer programming)Digital imageCCDbusiness.industryAnalytical signalsColorimetric-imaging analysisDimethylglyoximeSample solutionVisible spectrophotometrybusinessInstrumentsMeteoritesTalanta
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FRIPON: a worldwide network to track incoming meteoroids

2020

Context. Until recently, camera networks designed for monitoring fireballs worldwide were not fully automated, implying that in case of a meteorite fall, the recovery campaign was rarely immediate. This was an important limiting factor as the most fragile - hence precious - meteorites must be recovered rapidly to avoid their alteration. Aims. The Fireball Recovery and InterPlanetary Observation Network (FRIPON) scientific project was designed to overcome this limitation. This network comprises a fully automated camera and radio network deployed over a significant fraction of western Europe and a small fraction of Canada. As of today, it consists of 150 cameras and 25 European radio receiver…

DYNAMICS[INFO.INFO-AR]Computer Science [cs]/Hardware Architecture [cs.AR]MeteorsComputer scienceRadio receiver[INFO.INFO-DM]Computer Science [cs]/Discrete Mathematics [cs.DM]Surveys010502 geochemistry & geophysicsTrack (rail transport)01 natural sciencesMeteorites meteors meteoroidslaw.inventionPlanets and planetary system[INFO.INFO-TS]Computer Science [cs]/Signal and Image ProcessingMethods: observationallaw[INFO.INFO-RB]Computer Science [cs]/Robotics [cs.RO]meteoroids010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSObservational methodsEarth and Planetary Astrophysics (astro-ph.EP)meteoroids -surveys -methods: observational -interplanetary medium[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]ORIGIN[INFO.INFO-AO]Computer Science [cs]/Computer Arithmeticmeteorites meteors meteoroids – surveys – methods: observational – interplanetary mediumMeteoroidsRECOVERYORBITMeteoriteFully automatedInterplanetary medium; Meteorites meteors meteoroids; Methods: observational; Surveys[INFO.INFO-TI]Computer Science [cs]/Image Processing [eess.IV][INFO.INFO-DC]Computer Science [cs]/Distributed Parallel and Cluster Computing [cs.DC]Astrophysics - Instrumentation and Methods for Astrophysics[SPI.SIGNAL]Engineering Sciences [physics]/Signal and Image processingFLUXReal-time computingfripon[INFO.INFO-DS]Computer Science [cs]/Data Structures and Algorithms [cs.DS]FOS: Physical sciencesContext (language use)CAMERA[INFO.INFO-SE]Computer Science [cs]/Software Engineering [cs.SE][SPI.AUTO]Engineering Sciences [physics]/Automatic[SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology0103 physical sciencesFIREBALL NETWORKobservational [Methods]meteorsInstrumentation and Methods for Astrophysics (astro-ph.IM)0105 earth and related environmental sciencesMeteoroidINNISFREE METEORITE[INFO.INFO-CV]Computer Science [cs]/Computer Vision and Pattern Recognition [cs.CV]Astronomy and AstrophysicsMETEORITE FALLMeteorites meteors meteoroidCamera networkSpace and Planetary Science[SDU]Sciences of the Universe [physics]Interplanetary spaceflightmeteroids trackingmeteoroids - surveys - methods: observationalSYSTEMInterplanetary mediumAstrophysics - Earth and Planetary AstrophysicsMeteorites
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Identification of carbonate-rich outcrops on Mars by the Spirit rover.

2010

Ancient Carbonate Minerals on Mars The historical presence of liquid water on Mars together with a CO 2 -rich atmosphere should have resulted in the accumulation of large deposits of carbonate minerals. Yet, evidence for the presence of carbonates on the surface of Mars has been scarce. Using data collected by the Mars Exploration Rover, Spirit, Morris et al. (p. 421 , published online 3 June; see the Perspective by Harvey ) now present evidence for carbonate-rich outcrops in the Comanche outcrops within the Gusev crater. The carbonate is a major outcrop component and may have formed in the Noachian era (∼4 billion years ago) by precipitation from hydrothermal solutions that passed through …

MartianMultidisciplinaryWater on MarsExtraterrestrial EnvironmentAtmosphereClimateNoachianCarbonate mineralsCarbonatesTemperatureMarsWaterMars Exploration ProgramMeteoroidsCarbon DioxideAstrobiologychemistry.chemical_compoundImpact craterMeteoritechemistryCarbonateMagnesiumFerrous CompoundsSpacecraftGeologyScience (New York, N.Y.)
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