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301por Fitzpatrick, Richard“…A clear, concise introduction to all the major features of solar system dynamics, ideal for a first course.…”
Publicado 2012
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302“…Full of data about the Solar System, our Galaxy and the Universe, this is a one-stop reference for all astronomers.…”
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303por Kelley, Michael S. P., Hsieh, Henry H., Bodewits, Dennis, Saki, Mohammad, Villanueva, Geronimo L., Milam, Stefanie N., Hammel, Heidi B.“…Main-belt comets are small Solar System bodies located in the asteroid belt that repeatedly exhibit comet-like activity (that is, dust comae or tails) during their perihelion passages, strongly indicating ice sublimation(1,2). …”
Publicado 2023
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304por Mun, Hong-Seok, Dilawar, Muhammad Ammar, Mahfuz, Shad, Ampode, Keiven Mark B., Chem, Veasna, Kim, Young-Hwa, Moon, Jong-Pil, Yang, Chul-Ju“…SIMPLE SUMMARY: A combined geothermal heat pump and solar system (GHPS) was installed at a pig house to check the effects on electricity consumption, greenhouse gas emission (GHE), internal farm temperature, the concentration of noxious gases and growth performance. …”
Publicado 2022
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307por Ollivier, Marc, Roques, Francoise, Casoli, Fabienne, Encrenaz, Thérèse, Selsis, Franck“…They then consider the observations of young stars and circumstellar disks and address the case of the solar system as a specific example, different from the newly discovered systems. …”
Publicado 2009
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308por Encrenaz, Thérèse“…In contrast, our knowledge of Solar System planets has made huge progress over the past decades, thanks, especially, to space planetary exploration. …”
Publicado 2014
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309“…Spectroscopy and radiative transfer are rapidly growing fields within atmospheric and planetary science with implications for weather, climate, biogeochemical cycles, air quality on Earth, as well as the physics and evolution of planetary atmospheres in our solar system and beyond. Remote sensing and modeling atmospheric composition of the Earth, of other planets in our solar system, or of planets orbiting other stars require detailed knowledge of how radiation and matter interact in planetary atmospheres. …”
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310“…It reveals how we can all come to grips with some of the most fundamental questions about our Earth, Sun, and solar system--and the star-filled galaxies beyond. How big is our solar system? …”
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311“…Greek atomists such as Epicurus were convinced of the existence of an infinite number of solar systems like our own, but it was only in 1995 that a real answer began to emerge. …”
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312por Mazziotta, M.N., De La Torre Luque, P., Di Venere, L., Fassò, A., Ferrari, A., Loparco, F., Sala, P.R., Serini, D.“…The results are sensitive to the assumptions on the magnetic field nearby the Sun and to the cosmic-ray transport in the magnetic field in the inner Solar System.…”
Publicado 2020
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313por Nadeau, Jay, Lindensmith, Chris, Deming, Jody W., Fernandez, Vicente I., Stocker, Roman“…Meaningful motion is an unambiguous biosignature, but because life in the Solar System is most likely to be microbial, the question is whether such motion may be detected effectively on the micrometer scale. …”
Publicado 2016
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314por Hurford, T.A., Henning, W.G., Maguire, R., Lekic, V., Schmerr, N., Panning, M., Bray, V.J., Manga, M., Kattenhorn, S.A., Quick, L.C., Rhoden, A.R.“…We then apply this model to predict the amount of seismic energy release and largest seismic events on other moons in our Solar System and exoplanetary bodies. We find that many moons in the Solar System should be more seismically active than the Earth’s Moon and many exoplanets should exhibit more seismic activity than the Earth. …”
Publicado 2020
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315“…Robotic space exploration to the outer solar system is difficult and expensive and the space science community works inventively and collaboratively to maximize the scientific return of missions. …”
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316“…This concept’s first task is to find, prepare, and use dynamic three-dimensional models of the motion of celestial bodies and spacecraft or human-crewed spaceships in the solar system’s relativistic frame. The second task is to prepare the FPDS’ architecture and computer simulation space missions’ initial concepts in the internal part of the solar system. …”
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317Publicado 2003“…"A Jupiter-like planet has been discovered giving astronomers their best hope yet of finding another solar system similar to our own" (1/2 page).…”
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318por Jain, Pankaj“…IntroductionOverviewScales and DimensionsNight SkyConstellationsEarth, Sun, and the Solar SystemRetrograde Motion of PlanetsSidereal TimeAstronomical Catalogs and SoftwareObservationsElectromagnetic WavesElectromagnetic SpectrumTelescopesRefractor TelescopeReflecting TelescopeObservations at Visible FrequenciesTheoretical Limit on ResolutionSeeingMounting of TelescopeEquatorial MountAzimuthal MountInterferometerObservations at Other WavelengthsAstrometryCoordinate SystemsThe Horizontal SystemEquatorial Coordinate SystemEcliptic SystemGalactic Coordinate SystemSupergalactic Coordinate SystemSpace Velocity and Proper Motion of StarsDoppler EffectParallaxAberrationCoordinate TransformationsTransformation between Equatorial and Ecliptic Coordinate SystemsPrecession of EquinoxesEquatorial Mounting of a TelescopePhotometryIntroductionFlux Density and IntensityBlackbody RadiationEnergy Density in an Isotropic Radiation FieldMagnitude ScaleApparent MagnitudeAbsolute MagnitudeThe Color IndexBolometric MagnitudeStellar TemperaturesEffective TemperatureColor TemperatureAppendix: Solid AngleGravitation and Kepler's LawsTwo-Body ProblemApplication to Solar SystemVirial TheoremTidal Forces and Roche LimitStars, Stellar Spectra, and ClassificationIntroductionStellar Spectra Harvard Classification of Stellar SpectraSaha Equation Derivation of the Saha Equation Number of States of a Free Particle in a BoxHR DiagramStar Clusters and AssociationsDistance and Age Determination of Clusters using Color-Magnitude DiagramRadiation from Astronomical SourcesContinuous SpectraSynchrotron RadiationBremsstrahlungCompton ScatteringBound-Free TransitionsAbsorption and Emission Line SpectrumRadial Velocity due to Doppler EffectCauses of Finite Width of Spectral LinesMolecular Band SpectraExtinctionExtinction CoefficientColor ExcessStellar StructurePressure GradientMass DistributionEnergy ProductionTemperature GradientRadiative TransportConvective TransportBoundary ConditionsRosseland Mean OpacityEquation of StateIdeal Gas LawStellar Energy SourcesAppendix: Maxwell-Boltzmann DistributionStellar Nuclear ReactionsFundamental InteractionsFundamental ParticlesA Brief Introduction to NeutrinosPP Chain Nuclear Reaction RateNuclear Reaction Rate: DerivationNuclear Cross-SectionEstimating the Nuclear Reaction RateEnergy Released in Nuclear ReactionsStandard Solar ModelStar Formation and Stellar EvolutionEarly Stage of Star FormationFragmentationEvolution on the Main SequenceDegenerate Free Electron GasEvolution beyond the Main SequencePopulation I and II StarsWhite DwarfsNeutron StarBlack HolesSupernovaThe SunSolar AtmospherePhotosphereChromosphereCoronaDynamo Mechanism for Magnetic Field EnhancementSunspots and the Solar CycleSome Transient Phenomena The Solar SystemOrbital Properties of PlanetsRetrograde Motion of PlanetsAlbedo and Temperature of PlanetsTerrestrial Planets: Interior StructureJovian PlanetsThe MoonEclipses and OccultationsWhy Did Pluto Lose Its Planetship?…”
Publicado 2015
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319Publicado 2003“…"British astronomers say that Vega, one of the brightest stars in the sky, has a planetary system that is closer to our own Solar System than any other so far discovered" (1/2 page).…”
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320por Hanslmeier, Arnold“…This is followed by chapters dealing with our current knowledge of water in the solar system, followed by a discussion concerning the potential presence and possible detection of water on exoplanets. …”
Publicado 2011
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