Search results for "Spacecraft"

showing 10 items of 75 documents

Some Improvements on Relativistic Positioning Systems

2018

[EN] We make some considerations about Relativistic Positioning Systems (RPS). Four satellites are needed to position a user. First of all we define the main concepts. Errors should be taken into account. Errors depend on the Jacobian transformation matrix. Its Jacobian is proportional to the tetrahedron volume whose vertexes are the four tips of the receiver-satellite unit vectors. If the four satellites are seen by the user on a circumference in the sky, then, the Jacobian and the tetrahedron volume vanish. The users we consider are spacecraft. Spacecraft to be positioned cannot be close to a null Jacobian satellites-user configuration. These regions have to be avoided choosing an appropr…

General RelativityGeneral Computer ScienceTopology01 natural sciencessymbols.namesakeTransformation matrixUnit vectorPosition (vector)Numerical Methods35Q850103 physical sciences010303 astronomy & astrophysicsEngineering (miscellaneous)Mathematical Physics83C05Spacecraft010308 nuclear & particles physicsbusiness.industryApplied MathematicsNumerical analysisAstronomy and AstrophysicsRelativistic Positioning SystemsModeling and SimulationJacobian matrix and determinantPhysics::Space PhysicsTetrahedronsymbols37M99SatellitebusinessMATEMATICA APLICADA
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The enhanced X-ray Timing and Polarimetry mission—eXTP

2019

In this paper we present the enhanced X-ray Timing and Polarimetry mission - eXTP. eXTP is a space science mission designed to study fundamental physics under extreme conditions of density, gravity and magnetism. The mission aims at determining the equation of state of matter at supra-nuclear density, measuring effects of QED, and understanding the dynamics of matter in strong-field gravity. In addition to investigating fundamental physics, eXTP will be a very powerful observatory for astrophysics that will provide observations of unprecedented quality on a variety of galactic and extragalactic objects. In particular, its wide field monitoring capabilities will be highly instrumental to det…

Gravity (chemistry)Computer sciencespace mission: eXTPX-ray timingPolarimetryGeneral Physics and AstronomyFOS: Physical sciences01 natural sciences7. Clean energyPhysics and Astronomy (all)Settore FIS/05 - Astronomia E AstrofisicaObservatoryX-ray instrumentation0103 physical sciencesX-ray polarimetryGround segmentAerospace engineering010306 general physics010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)High Energy Astrophysical Phenomena (astro-ph.HE)Spacecraftsezelebusiness.industryPayloadGravitational waveAstrophysics::Instrumentation and Methods for Astrophysicsspace mission: eXTP; X-ray instrumentation; X-ray polarimetry; X-ray timing; Physics and Astronomy (all)Space SciencebusinessAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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A next generation Ultra-Fast Flash Observatory (UFFO-100) for IR/optical observations of the rise phase of gamma-ray bursts

2012

The Swift Gamma-ray Burst (GRB) observatory responds to GRB triggers with optical observations in ~ 100 s, but cannot respond faster than ~ 60 s. While some ground-based telescopes respond quickly, the number of sub-60 s detections remains small. In mid- to late-2013, the Ultra-Fast Flash Observatory-Pathfinder is to be launched on the Lomonosov spacecraft to investigate early optical GRB emission. This pathfinder mission is necessarily limited in sensitivity and event rate; here we discuss a next generation rapid-response space observatory. We list science topics motivating our instruments, those that require rapid optical-IR GRB response, including: A survey of GRB rise shapes/times, meas…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSpacecraftbusiness.industryApertureAstrophysics::High Energy Astrophysical PhenomenaExtinction (astronomy)Astrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomyAstrophysics::Cosmology and Extragalactic AstrophysicsOrbital mechanicslaw.inventionTelescopeFlash (photography)ObservatorylawbusinessGamma-ray burstAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaInstrumentation and Methods for Astrophysics (astro-ph.IM)
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Sampled-Data Control of Spacecraft Rendezvous with Discontinuous Lyapunov Approach

2013

Published version of an article in the journal: Mathematical Problems in Engineering. Also available from the publisher at: http://dx.doi.org/10.1155/2013/814271 Open Access This paper investigates the sampled-data stabilization problem of spacecraft relative positional holding with improved Lyapunov function approach. The classical Clohessy-Wiltshire equation is adopted to describe the relative dynamic model. The relative position holding problem is converted into an output tracking control problem using sampling signals. A time-dependent discontinuous Lyapunov functionals approach is developed, which will lead to essentially less conservative results for the stability analysis and control…

Lyapunov functionSpacecraftArticle Subjectbusiness.industryGeneral Mathematicslcsh:MathematicsGeneral EngineeringSampling (statistics)lcsh:QA1-939Stability (probability)symbols.namesakeExponential stabilityControl theoryPosition (vector)lcsh:TA1-2040symbolsLyapunov equationVDP::Matematikk og Naturvitenskap: 400::Matematikk: 410::Anvendt matematikk: 413businesslcsh:Engineering (General). Civil engineering (General)MathematicsMathematical Problems in Engineering
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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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Structural Stability of Hafnia-Based Materials at Ultra-High Temperature

2018

This study assesses the structural stability at ultra-high temperature of the following selected compositions: 6.5 and 14 mol. % of RE2O3 (RE = Dy, Y, Er, Yb, and Lu) doped HfO2. Under thermal cycling and thermal shock, the structural stability was evaluated at 2400°C with water vapor flux using a specific test bench with a 3 kW CO2 laser. The cubic phase stability, which is theoretically important in the broad temperature range from 25 to 2800°C, was determined by a quantitative analysis of the X-ray diffractograms. Fully and partially stabilized HfO2, obtained respectively with 14 mol. % and 6.5 mol. % of dopants, showed different behaviors to thermal damage. Thermal expansion was measure…

Materials sciencebiologySpacecraft propulsionPhase stability020502 materialsMechanical Engineering02 engineering and technologyCondensed Matter PhysicsHafniabiology.organism_classification01 natural sciencesThermal expansion010309 optics0205 materials engineeringMechanics of MaterialsStructural stability0103 physical sciencesGeneral Materials ScienceComposite materialMaterials Science Forum
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Robust control for autonomous spacecraft evacuation with model uncertainty and upper bound of performance with constraints

2014

Published version of an article in the journal: Mathematical Problems in Engineering. Also available from the publisher at: http://dx.doi.org/10.1155/2014/589381 This paper studies the problem of guaranteed cost control for spacecraft evacuation. The relative dynamic model is established based on Clohessy-Wiltshire (C-W) equations. The paper has taken parameter uncertainty, output tracking, disturbance attenuation, and fuel cost into consideration. The paper introduces a new Lyapunov approach, so the controller design problem can be transferred into a convex optimization problem subject to linear matrix inequality (LMI) constraints. By using the controller, the spacecraft evacuation can be …

Mathematical optimizationEngineeringArticle SubjectSpacecraftbusiness.industryGeneral Mathematicslcsh:MathematicsControl (management)VDP::Technology: 500::Mechanical engineering: 570General EngineeringLinear matrix inequalityComputerApplications_COMPUTERSINOTHERSYSTEMSTracking (particle physics)lcsh:QA1-939Upper and lower boundsEngineering (all)Control theorylcsh:TA1-2040Convex optimizationMathematics (all)Robust controlbusinesslcsh:Engineering (General). Civil engineering (General)Mathematics (all); Engineering (all)
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In situ evidence for an ancient aqueous environment at Meridiani Planum, Mars.

2004

Sedimentary rocks at Eagle crater in Meridiani Planum are composed of fine-grained siliciclastic materials derived from weathering of basaltic rocks, sulfate minerals (including magnesium sulfate and jarosite) that constitute several tens of percent of the rock by weight, and hematite. Cross-stratification observed in rock outcrops indicates eolian and aqueous transport. Diagenetic features include hematite-rich concretions and crystal-mold vugs. We interpret the rocks to be a mixture of chemical and siliciclastic sediments with a complex diagenetic history. The environmental conditions that they record include episodic inundation by shallow surface water, evaporation, and desiccation. The …

Meridiani PlanumGeologic SedimentsExtraterrestrial EnvironmentGeochemistryMineralogyMarsWeatheringengineering.materialFerric CompoundsLifeConcretionExobiologyComposition of MarsSpacecraftgeographyMineralsMultidisciplinarygeography.geographical_feature_categorySulfatesSilicatesSpectrum AnalysisWaterDiagenesisVolcanic rockengineeringSedimentary rockSiliciclasticGeologySulfurScience (New York, N.Y.)
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Two Years at Meridiani Planum: Results from the Opportunity Rover

2006

The Mars Exploration Rover Opportunity has spent more than 2 years exploring Meridiani Planum, traveling ∼8 kilometers and detecting features that reveal ancient environmental conditions. These include well-developed festoon (trough) cross-lamination formed in flowing liquid water, strata with smaller and more abundant hematite-rich concretions than those seen previously, possible relict “hopper crystals” that might reflect the formation of halite, thick weathering rinds on rock surfaces, resistant fracture fills, and networks of polygonal fractures likely caused by dehydration of sulfate salts. Chemical variations with depth show that the siliciclastic fraction of outcrop rock has undergon…

Meridiani PlanumGeologic SedimentsExtraterrestrial EnvironmentOutcropGeochemistryMarsMineralogyWeatheringengineering.materialFerric CompoundsTimeConcretionSpacecraftMineralsMultidisciplinarySulfatesSilicatesWaterHematitevisual_artengineeringvisual_art.visual_art_mediumHaliteSedimentary rockSiliciclasticAcidsGeologyScience
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Jarosite and hematite at Meridiani Planum from Opportunity's Mossbauer Spectrometer.

2004

Mössbauer spectra measured by the Opportunity rover revealed four mineralogical components in Meridiani Planum at Eagle crater: jarosite- and hematite-rich outcrop, hematite-rich soil, olivine-bearing basaltic soil, and a pyroxene-bearing basaltic rock (Bounce rock). Spherules, interpreted to be concretions, are hematite-rich and dispersed throughout the outcrop. Hematitic soils both within and outside Eagle crater are dominated by spherules and their fragments. Olivine-bearing basaltic soil is present throughout the region. Bounce rock is probably an impact erratic. Because jarosite is a hydroxide sulfate mineral, its presence at Meridiani Planum is mineralogical evidence for aqueous proc…

Meridiani PlanumGeologic SedimentsExtraterrestrial EnvironmentOutcropMineralogyMagnesium CompoundsMarsengineering.materialFerric CompoundsSpectroscopy MossbauerImpact craterConcretionJarositeComposition of MarsSpacecraftMineralsMultidisciplinaryMineralSulfatesSilicatesWaterHematitevisual_artvisual_art.visual_art_mediumengineeringGeologyIron CompoundsScience (New York, N.Y.)
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