Search results for " Solar System"

showing 10 items of 16 documents

Philae's first days on the comet

2015

On 12 November 2014, Philae landed on the surface of comet 67P/Churyumov-Gerasimenko (67P), making an almost 30-year dream a reality. The pioneering flybys of 1P/Halley in 1986 revealed that despite being made primarily of ice, it was covered in highly absorbing carbonrich molecules. What is their composition? When did they form, and through which chemical routes? Might they have constituted prebiotic molecules necessary for life? At a larger scale, what can one learn from comets that has relevance to the evolution of the solar system and planets? ![Figure][1] 12 NOVEMBER 2014: PHILAE LANDED ON THE NUCLEUS OF COMET 67P CREDIT: ESA/ROSETTA/MPS FOR OSIRIS TEAM MPS/UPD/LAM/IAA/SSO/INTA/UPM/DAS…

Asteroiden und KometenSolar SystemMultidisciplinaryInstitut für PlanetenforschungCometAstronomical unitRegolithPhilaelaw.inventionAstrobiologyNutzerzentrum für Weltraumexperimente (MUSC)OrbiterChondritelawPlanetRosettaFormation and evolution of the Solar SystemComet 67P Churyumov GerasimenkoGeology
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Demand side management and Distributed on Site actions benefits

2013

Global warming and energy demand are nowadays becoming one of the major issues of the third millennium, mainly because human activities seem to have a clear impact on the raise of CO2 emissions as never it has been experienced in the past. Among the different factors affecting CO2 emissions, energy demand from buildings constitutes one of the most important actors. Energy Management (EM) actions can reduce the energy consumption of the system and minimize peaks-level, by using a distributed control over every house. These local actions can greatly contribute to reduce the impact on the global CO2 emissions. An evaluation of the potential energy saving and CO2 emissions reduction on building…

Building management systemEngineeringZero-energy buildingCO2 reduction power system Combined Photovoltaic Solar system grid simulatorEnergy managementbusiness.industryPhotovoltaic systemEnvironmental engineeringEnergy consumptionEnvironmental economicsSettore ING-IND/32 - Convertitori Macchine E Azionamenti ElettriciSettore ING-INF/01 - ElettronicaSettore ING-IND/33 - Sistemi Elettrici Per L'EnergiaElectric power systemSmart gridBuilding-integrated photovoltaicsbusiness
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Resonances in the solar system

2010

We give a description of orbital and spin-orbit resonances in the solar system, providing several examples which include planets, satel- lites, asteroids, rings, Kuiper objects.

Celestial Mechanics Resonances Solar SystemSettore MAT/07 - Fisica Matematica
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Protoplanetary Disks, Solar System Minor Bodies and Origin of Life

2001

In the last decade, planetary science researchers have obtained significant advances on the origin and evolution of life on Earth. The increasing resolution and the development of new instruments (as space telescopes and adaptative optics) has provided first detailed images on protoplanetary disks and star formation regions. Moreover, in the last few years, doppler spectroscopic technique has confirmed the presence of extrasolar planets. These evidence shows planetary formation as a continuous and very common process in the Cosmos, indicating that our Solar System is not too special as was suggested in the past.

Debris diskSolar SystemPlanetesimalPlanetary scienceStar formationAstrophysics::Solar and Stellar AstrophysicsAstronomyAstrophysics::Earth and Planetary AstrophysicsFormation and evolution of the Solar SystemProtoplanetary diskExoplanetGeologyAstrobiology
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Do soils exist outside Earth?

2010

Abstract On Earth, soils form thanks to the combined action of at least five factors: parent rock, climate, topography, biota, and time. However, the necessity of biota as unavoidable soil forming factor is debated, as important parts of our planet experiencing extreme climates host virtually life-free soils with advanced horizonation. Now that space exploration has greatly expanded our understanding of the Solar System, providing consistent evidences that the loose, unconsolidated "skin" of some nearby rocky bodies is lifeless, it is time to establish if the latter can be considered to be soil in a pedological sense. Our feeling is that, since the concept of soil chiefly bases on the occur…

Earth scienceSettore ING-IND/05 - Impianti E Sistemi AerospazialiAstronomy and AstrophysicsWeatheringBiotaGeophysicsMars Exploration ProgramRegolithSoil Regolith Solar System Weathering PedologySettore AGR/14 - PedologiaSpace and Planetary ScienceSoil waterEarth (chemistry)PedologyParent rockGeologyPlanetary and Space Science
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DIRECT EVIDENCE FOR CONDENSATION IN THE EARLY SOLAR SYSTEM AND IMPLICATIONS FOR NEBULAR COOLING RATES

2009

We have identified in an acid resistant residue of the carbonaceous chondrite Murchison a large number (458) of highly refractory metal nuggets (RMNs) that once were most likely hosted by Ca,Al-rich inclusions (CAIs). While osmium isotopic ratios of two randomly selected particles rule out a presolar origin, the bulk chemistry of 88 particles with sizes in the submicron range determined by energy dispersive X-ray (EDX) spectroscopy shows striking agreement with predictions of single-phase equilibrium condensation calculations. Both chemical composition and morphology strongly favor a condensation origin. Particularly important is the presence of structurally incompatible elements in particl…

PhysicsMurchison meteoriteRange (particle radiation)AstrochemistrySpace and Planetary ScienceChemical physicsChondriteCarbonaceous chondriteCondensationAstronomy and AstrophysicsAstrophysicsFormation and evolution of the Solar SystemChemical compositionThe Astrophysical Journal
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An idealized mechanism for the orbital migration of protoplanets

1993

We report here how the action of radiation forces on small solid particles in a circumstellar disc could induce a suitable mechanism for orbital migration of protoplanets. The ratio of radiation-to-gravitational forces acting on a particle depends on its physical and chemical properties. As a consequence of this fact, we show that different particles following the same trajectory would move with different velocities. Sufficiently large bodies, insensitive to radiation forces, would accrete dust particles that are moving more slowly, thus spiralling towards the central star and transporting mass and angular momentum from the outer to the inner parts of the circumstellar disc. In the case of …

PhysicsSolar SystemAngular momentumAstronomy and AstrophysicsPlanetary systemAccretion (astrophysics)Classical mechanicsRadiation pressureSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsFormation and evolution of the Solar SystemProtoplanetAstrophysics::Galaxy AstrophysicsCosmic dustMonthly Notices of the Royal Astronomical Society
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Extraterrestrial Mössbauer Spectroscopy

2011

To understand the origin of the Solar system and the origin of Life itself is one of the longest standing goals of human thought. Our Sun and its planets have formed out of an interstellar cloud which collapsed due to gravitational forces, forming a disk shaped so-called protosolar nebula, with the young star in the centre. Such disk shaped and dust grain containing protosolar nebulae have been observed. One of them is surrounding the young star Beta pictoris [1, 2]. Silicates, carbon and metal grains, oxides and sulfides should have been present. One of the important elements with relatively high abundance is iron. It is believed that simple molecules, such as water (H2O), carbon monoxide …

Planetary bodySolar SystemNebulaPlanetExtraterrestrial lifePhysics::Space PhysicsAstrophysics::Solar and Stellar AstrophysicsBeta PictorisAstrophysics::Earth and Planetary AstrophysicsPlanetary systemFormation and evolution of the Solar SystemAstrophysics::Galaxy AstrophysicsAstrobiology
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ON THE “SOLAR SYSTEM SMALL BODIES” ASTROPLATE PROJECT OF THE UKRAINIAN VIRTUAL OBSERVATORY

2019

The UkrVO Joint Digital Archive of astro- plates and the newest digitized data processing services al- lowed us to form a new approach for the creation of catalogs of astrometric and photometric characteristics of the Solar System bodies. Given this, the main goal of this approach was not only to complete the processing with the best possi- ble accuracy of high-quality and unprocessed earlier photo- graphic observations of the Solar System bodies but also to find new original data from these observations. As a result, more than 6,500 new astrometric positions and stellar magnitudes of asteroids, and 3,036 positions of outer planets (Pluto, Uranus, Neptune, Saturn, Jupiter) and their satelli…

Plutolcsh:QB1-991Outer planetsObservatoryAsteroidNeptunelcsh:AstronomyUranusAstronomyarchives; catalog; positions; Solar System bodiesVirtual observatoryEphemerisGeologyOdessa Astronomical Publications
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An Embedded System for the integration of a Combined Photovoltaic Solar (CPS) system into a ZigBee Home Area Network

2011

In this paper is reported the design and implementation of an electronic system capable of communicating over a standard ZigBee network in order to let a residential gateway collector, named agent, gain access to the parameters of a Combined Photovoltaic and Solar thermal (CPS) plant, thus realizing a networked energy production appliance . The system is made of three parts: a PV metering device, a boiler metering device also capable of controlling a heating resistor embedded within the boiler tank, and a data collector acting as a ZigBee node. The data collector device periodically retrieves the following parameters from the metering devices: instantaneous photovoltaic power production, ac…

Settore ING-INF/03 - TelecomunicazioniBEYWATCH (Building EnergY WATCHer) CPS (Combined Photovoltaic Solar System) grid hot water electrical energy ZigBEE Wireless Sensor Networks.Settore ING-INF/01 - Elettronica
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