Littérature scientifique sur le sujet « Evolution du système solaire »
Créez une référence correcte selon les styles APA, MLA, Chicago, Harvard et plusieurs autres
Sommaire
Consultez les listes thématiques d’articles de revues, de livres, de thèses, de rapports de conférences et d’autres sources académiques sur le sujet « Evolution du système solaire ».
À côté de chaque source dans la liste de références il y a un bouton « Ajouter à la bibliographie ». Cliquez sur ce bouton, et nous générerons automatiquement la référence bibliographique pour la source choisie selon votre style de citation préféré : APA, MLA, Harvard, Vancouver, Chicago, etc.
Vous pouvez aussi télécharger le texte intégral de la publication scolaire au format pdf et consulter son résumé en ligne lorsque ces informations sont inclues dans les métadonnées.
Articles de revues sur le sujet "Evolution du système solaire"
Césarsky, Catherine, et Richard Bonneville. « Perspectives d'exploration du système solaire ». Annales des Mines - Réalités industrielles Mai 2012, no 2 (2012) : 55. http://dx.doi.org/10.3917/rindu.122.0055.
Texte intégralNaroua, Illiassou, Abdoulkadri Laouali, Souley Issaka, Maman Rachid Salissou Issoufou et Hassoumi Djibo. « Etude Comparative De La Rentabilité Des Systèmes De Pompage Solaire Et Thermique Sur Le Périmètre Irrigué De Soumarana Au Niger ». European Scientific Journal ESJ 17, no 43 (31 décembre 2021) : 246–59. http://dx.doi.org/10.19044/esj.2021.v17n43p246.
Texte intégralMenhoudj, Sayeh, Djamel Sifodil et Abderrahmane Mokhtari. « Etude expérimentale d’un système solaire actif-PSD ». Journal of Renewable Energies 15, no 3 (23 octobre 2023) : 479–88. http://dx.doi.org/10.54966/jreen.v15i3.337.
Texte intégralMerabti, Leila, Mustapha Merzouk, Nachida Kasbadji, Nesrine Hatraf et Mohamed Abbas. « Rafraîchissement solaire par dessiccation ». Journal of Renewable Energies 17, no 3 (19 octobre 2023) : 403–9. http://dx.doi.org/10.54966/jreen.v17i3.453.
Texte intégralBlamont, Jacques. « La vie dans le système solaire ». Comptes Rendus de l'Académie des Sciences - Series IIA - Earth and Planetary Science 331, no 8 (octobre 2000) : 515–24. http://dx.doi.org/10.1016/s1251-8050(00)01446-4.
Texte intégralMauger, Charlotte. « Les garde-fous du Système solaire ». Pour la Science N° 549 – juillet, no 7 (3 juillet 2023) : 14. http://dx.doi.org/10.3917/pls.549.0014.
Texte intégralBoyle, Rebecca. « Réinventer la formation du Système solaire ». Pour la Science N° 541 – novembre, no 11 (19 octobre 2022) : 46–53. http://dx.doi.org/10.3917/pls.541.0046.
Texte intégralChaouachi, Béchir, et Slimane Gabsi. « Etude expérimentale d’un chauffe-eau solaire à stockage intégré dans des conditions réelles ». Journal of Renewable Energies 9, no 2 (30 juin 2006) : 75–82. http://dx.doi.org/10.54966/jreen.v9i2.816.
Texte intégralImessad, Kkaled, et Maiouf Belhamel. « Analyse Thermique d’un Système de Chauffage Solaire Passif ». Journal of Renewable Energies 4, no 1 (30 juin 2001) : 61–67. http://dx.doi.org/10.54966/jreen.v4i1.998.
Texte intégralRoddier, Claude. « Observations du système solaire avec l'optique adaptive ». Comptes Rendus de l'Académie des Sciences - Series IIB - Mechanics-Physics-Chemistry-Astronomy 325, no 2 (juillet 1997) : 109–14. http://dx.doi.org/10.1016/s1251-8069(97)83254-x.
Texte intégralThèses sur le sujet "Evolution du système solaire"
Morgado, Correia Alexandre Carlos. « Evolution à long terme de la rotation de Vénus ». Paris 7, 2001. http://www.theses.fr/2001PA077222.
Texte intégralAuger, Anne-Thérèse. « Formation et évolution des morphologies de surface des petits corps du système solaire, à partir des images de la sonde spatiale Rosetta ». Thesis, Aix-Marseille, 2016. http://www.theses.fr/2016AIXM4721/document.
Texte intégralResiduals from the accretion disk in which planets formed, asteroids and comets provide important constraints on the solar system formation and evolution processes. Based on the images from the Rosetta mission, the main objectives of this thesis are to characterize the morphologies at the surface of these small bodies and to study the processes responsible for their formation and evolution.On asteroid (21) Lutetia, the relief is controlled by impacts, forming craters, ejecta blankets, fractures and boulders.On the nucleus of comet 67P, the Imhotep region, located at the equator of the nucleus, presents smooth terrains and consolidated terrains, heavily fractured. It is the only region that shows tens of circular features less than 60 m in size, probably ancient, which we find associated with layers of several meters thick. During the passage at perihelion, major changes occurred in smooth terrains ; they may be linked to mechanical stresses acting in the nucleus subsurface. A particular type of fractures observed at the surface of 67P has also been studied in detail. These fractures join each other in polygons of roughly 3 m in size. These polygons probably result from the strong variations of temperature at the surface and subsurface. More generally, the observations and their interpretation from Rosetta data show that the morphologies at the surface of 67P can result from its formation and endogeneous processes, as well as from exogeneous and evolutionary processes such as the sublimation of ices or thermal stresses
Le, Pivert-Jolivet Tania. « Composition, origine et évolution de Ryugu à travers les analyses de MicrOmega/Curation ». Electronic Thesis or Diss., université Paris-Saclay, 2023. http://www.theses.fr/2023UPASP192.
Texte intégralPrimitive asteroids are small bodies that have evolved relatively little since their formation. They contain information about the chemical composition of the early solar system and its evolution up to the present day. Before the 2020s, the only potential analogs of these objects available for laboratory analysis were carbonaceous chondrites (CCs). But the link between CCs and their asteroidal parent bodies is not yet clear, and the primitive composition of CCs is partially altered by interaction with the terrestrial atmosphere. This is why, in the 2010s, two space missions observed and collected samples from the surface of primitive asteroids: they represent the first laboratory study of fragments representing their parent bodies. The C-type near-Earth asteroid (162173) Ryugu, was the target of the Hayabusa2 mission (JAXA). The spacecraft performed two samplings, collecting surface and subsurface samples excavated by an artificial impactor. In December 2020, the sealed capsule containing 5.4g of samples returned to Earth and was opened in the Curation Facility (Sagamihara, Japan), a complex containing a set of clean chambers for carrying out an initial analysis of the grains, preserving their integrity and without exposing them to the terrestrial atmosphere. The aim of my thesis was to characterize the composition of Ryugu samples to retrace the evolution of the primitive matter at different stages in the history of the solar system. Thus, I analysed data acquired by the near-infrared (0.99 – 3.65 μm) hyperspectral microscope MicrOmega, installed in the Curation Facility. MicrOmega enables a non-invasive characterization of the mineral and organic composition of the grains. I studied the 2.7 μm band, characteristic of the vibration of the -OH group in the phyllosilicates of the samples. I carried out a statistical study of the variations in the position and depth of the band between several hundred millimetre-sized grains, which indicate a variation in the composition of the phyllosilicates. This analysis suggests that some of the grains collected at the surface experienced space weathering, a process that affects the composition and microstructure of the surface of airless bodies. Conversely, all the grains from the subsurface have undergone a limited exposure to the space environment. This study also shows that the Ryugu samples are depleted in water (H₂O) compared with CI chondrites, despite their similar mineralogy, and suggests that a significant proportion of the water in the CIs could be of terrestrial origin. I then studied the variations in the shape and position of the 2.7 μm band at the surface of the grains. I showed that the spectral heterogeneity of the surface varies from one grain to another. This variation in heterogeneity could be linked to variations in the degree of aqueous alteration and/or the degree of space weathering on surfaces with different roughnesses. This study shows the potential of infrared hyperspectral imaging to detect variations in the water content between the grains, without any bias by the terrestrial atmosphere. This work provides a better understanding of the physical and chemical evolution of the surface and the near subsurface of primitive asteroids. It also provides new insights on the terrestrial alteration of carbonaceous chondrites, with implications for the quantity of water in the asteroidal parent bodies of CI chondrites
Leconte, Jérémy. « Un nouveau regard sur la Structure interne et l'évolution des planètes géantes solaires et extrasolaires ». Phd thesis, Ecole normale supérieure de lyon - ENS LYON, 2011. http://tel.archives-ouvertes.fr/tel-00707629.
Texte intégralComito, Carlo. « Numerical N-body approach to binary asteroid formation and evolution ». Phd thesis, Université de Nice Sophia-Antipolis, 2012. http://tel.archives-ouvertes.fr/tel-00703696.
Texte intégralGkotsinas, Anastasios. « On the pristine nature of cometary nuclei : coupled modeling of their thermal and dynamical evolution ». Electronic Thesis or Diss., Lyon 1, 2023. http://www.theses.fr/2023LYO10144.
Texte intégralComets are a population of small Solar System bodies, often described as the most primitive population in our Solar System, holding valuable information on its formation and evolution. Formed early, at the same time as the giant planets, in the outer parts of the protoplanetary disk and scattered outwards shortly after their formation towards distant and cold reservoirs, they are considered to have preserved their primordial composition and properties to a great extent. However, the level of this primitive nature has started to be reevaluated recently, as a growing body of observational evidence and an important number of theoretical studies are suggesting the possibility of thermally-induced alterations before their return to the inner parts of the Solar System, where they are usually studied and observed. In this context, our work aims to examine the level of the primitive nature of different cometary families in our Solar System. To do so, we developed a dedicated thermal evolution model, designed for an efficient coupling to N-body simulations, tracking the long-term orbital evolution of planetesimals, originating in the outer parts of the protoplanetary disk and evolving into planetary-crossing orbits after a prolonged stay in outer Solar System reservoirs. Our results reveal the possibility of thermal processing, affecting mainly the primordial condensed hyper-volatile content and on a lesser extent the primordial moderately-volatile and amorphous water ice content, during the early phases of a comet's lifetime. A comparative study is indicating that long-period comets are expected to be the least altered population. Intense, yet sporadic, activity is also recorded in the planetary region, as comets return in the inner Solar System, compatible with the current observables on the Centaur population. These results indicate that the thermal evolution of cometary nuclei is inextricably related to their orbital evolution. They are also indicating that the cometary activity observed in the inner parts of the Solar System is very likely triggered from thermally processed subsurface layers, highlighting the necessity of considering the past evolutionary history of comets when interpreting the current observations in a broader context
Philipot, Florian. « Vers une recherche exhaustive des planètes géantes autour des étoiles proches de type solaire ». Electronic Thesis or Diss., Université Paris sciences et lettres, 2023. http://www.theses.fr/2023UPSLO008.
Texte intégralThe detection of the first exoplanets in the 1990s opened a new era in the study of planets. Today, thanks to increasingly powerful instruments, several hundred exoplanets (hot Jupiters, Super-Earths, multiple systems...) are discovered every year. Thanks to this wide variety of exoplanets, it is possible to study the distribution (distance, mass, eccentricity...) of these objects in order to better constrain the formation and evolution models of planetary system. Nevertheless, each detection method has its own limitations and detection biases. One aim of this thesis was to identify the limitations of the various detection methods, in particular those related to radial velocities (RV), and to improve the characterization of companions detected by RV.As a first step, I tested the robustness of studies aimed at determining the radial distribution of giant planets. Analysis of RV data from stars hosting long-period planets, the impact of stellar activity and the hypothesis made in completeness calculations, allowed us to demonstrate that statistical RV studies were not robust beyond 7-8 AU. Subsequently, I combined RV data with available absolute and relative astrometry measurements to improve the characterization of long-period sub-stellar companions. This study allowed us to precisely constrain the orbital parameters and, above all, the mass of seven companions detected in RV. It also highlighted the importance of coupling RV data with other measurements to accurately determine the nature of a companion. Finally, I used measurements of stars' proper motion anomalies (PMa), derived from Hipparcos and Gaia absolute astrometry, to search for new sub-stellar companions in the HARPS/VLT spectrograph archive. This analysis enabled me to improve the characterization of 14 sub-stellar companions, and to discover three new brown dwarfs and seven new exoplanets. I also demonstrated the effectiveness of using PMa measurements to optimize the search for sub-stellar companions
Benbakoura, Mansour. « Evolution des étoiles de faible masse en interaction : observations multi-techniques et modélisation des systèmes multiples ». Thesis, Université de Paris (2019-....), 2019. http://www.theses.fr/2019UNIP7027.
Texte intégralThis thesis is devoted to the study of low-mass stars having other stars or planets in their immediate environment. We focused on the influence of interactions with these companions on stellar evolution and their observable consequences.In the first part, we present the model of evolution of star–planet systems that we developed during this thesis, called ESPEM (French acronym for Evolution of Planetary Systems and Magnetism). This model incorporates ab-initio prescriptions to quantify the effects of magnetized stellar wind and tidal dissipation on stellar rotation and planetary orbit, simultaneously with the star's structural evolution. First, we use it to study the secular evolution of the rotation of planet-host stars and show that this evolution can be significantly different from that of isolated stars. Next, we examine the predictions of this model regarding the orbital architecture of star–planet systems. Our results suggest an interpretation to the observed distributions of orbital and stellar rotation periods.In the second part of the manuscript, we show how the observation of advanced binary stars allows us to test astrophysical theories, in particular asteroseismology and tidal interaction. First, we present the results of an observation program that we conducted for more than two years and that allowed us to characterize 16 eclipsing binary systems. Then, we compare these results with those obtained by analyzing this sample using asteroseismic tools to verify the accuracy of the latter. Finally, by extending the studied sample to 30 other advanced binary stars including an evolved primary, we test the theory of tidal evolution. This allows us both to validate the theory and to understand the evolution of the systems observed in this work.This work highlights two aspects of the specificity of multiple systems. First, it shows how the evolution of stars is affected by the presence of a stellar or planetary companion. Second, it emphasizes the interest of binary stars in testing astrophysical theories and reinforces the current understanding of stellar evolution
Hersant, Franck. « Turbulence dans la nébuleuse solaire primitive et formation du système solaire externe ». Phd thesis, Université Paris-Diderot - Paris VII, 2002. http://tel.archives-ouvertes.fr/tel-00316082.
Texte intégralKhalfallaoui, Saoussen. « Comportement dynamique et automatisation d’un système solaire thermique muni d’un traqueur solaire ». Rouen, 2009. http://www.theses.fr/2009ROUES020.
Texte intégralThis work deals with the study of a thermal solar system. The thermal behaviour is investigated in unsteady state with regard to the intermittency of sunlight. The modelling of this system was carried out taking into account a global approach to make an energy balance for each component of the thermal solar system. A simulation tool was developed under the MATLAB environment using Simulink ® tool for solving this knowledge model. This model is validated by comparing simulation results to measurement data obtained on the experimental set-up. Energy efficiency of the solar system and the instantaneous efficiency of solar collectors have been studied in unsteady state. The realisation of a solar tracker has been completed. The gain in thermal energy with solar tracker has been studied in comparison with the configuration in which the solar collectors are fixed at different inclinations
Livres sur le sujet "Evolution du système solaire"
Le système solaire. Chamalières, France : Proxima, 2002.
Trouver le texte intégralJenkins, Alvin W. Le système solaire. [France?] : Circonflexe, 2005.
Trouver le texte intégralMist, Rosalind. Le système solaire. Montréal (Québec) : Bayard Canada, 2013.
Trouver le texte intégralLilensten, Jean, et Mathieu Barthélémy. Le système solaire revisité. Paris : Eyrolles, 2006.
Trouver le texte intégralLa terre et le système solaire. Paris : France Loisirs, 1995.
Trouver le texte intégralTavel, Jonathan. Voyage au coeur du système solaire. Saint-Constant, Qc : Broquet, 2005.
Trouver le texte intégralAnne, Willemez, et Gracieux Serge, dir. Le système solaire : De sa découverte à sa conquête. Paris : Fleurus, 2015.
Trouver le texte intégralKelly, Beatty J., Petersen Carolyn Collins et Chaikin Andrew 1956-, dir. The new solar system. 4e éd. Cambridge : Sky Pub., 1999.
Trouver le texte intégralClark, Stuart. L'astrophysique. Paris : France Loisirs, 1995.
Trouver le texte intégralWhyman, Kathryn. Visa pour la sciences : Le système solaire/ Kathryn Whyman, François Carlier. Ville Saint-Laurent : Éditions de Trécarré, 1988.
Trouver le texte intégralChapitres de livres sur le sujet "Evolution du système solaire"
Poincaré, Henri. « Sur la Stabilité du Système Solaire (1898) ». Dans Scientific Opportunism L’Opportunisme scientifique, 77–83. Basel : Birkhäuser Basel, 2002. http://dx.doi.org/10.1007/978-3-0348-8112-8_5.
Texte intégralBreuer, Doris. « 4.2.3.4 Dynamics and thermal evolution ». Dans Solar System, 323–44. Berlin, Heidelberg : Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-88055-4_19.
Texte intégralMilone, Eugene F., et William J. F. Wilson. « The Moon’s Surface, Structure, and Evolution ». Dans Solar System Astrophysics, 197–230. New York, NY : Springer New York, 2013. http://dx.doi.org/10.1007/978-1-4614-8848-4_8.
Texte intégralBeaver, John. « Evolution of the Solar System ». Dans The Big Picture, 105–17. Cham : Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-031-02080-3_8.
Texte intégralTrimble, Virginia. « Chemical Evolution Tomorrow ». Dans Origin of Elements in the Solar System, 175–88. Boston, MA : Springer US, 2002. http://dx.doi.org/10.1007/0-306-46927-8_15.
Texte intégralSchubert, G., H. Hussmann, V. Lainey, D. L. Matson, W. B. McKinnon, F. Sohl, C. Sotin, G. Tobie, D. Turrini et T. Van Hoolst. « Evolution of Icy Satellites ». Dans Satellites of the Outer Solar System, 445–82. New York, NY : Springer New York, 2010. http://dx.doi.org/10.1007/978-1-4419-7439-6_17.
Texte intégralBertotti, Bruno, Paolo Farinella et David Vokrouhlický. « Dynamical Evolution of the Solar System ». Dans Astrophysics and Space Science Library, 459–508. Dordrecht : Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0233-2_15.
Texte intégralBertotti, Bruno, et Paolo Farinella. « Dynamical Evolution of the Solar System ». Dans Physics of the Earth and the Solar System, 304–37. Dordrecht : Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-1916-7_15.
Texte intégralGrevesse, N. « Solar Abundances : The Reference System ». Dans Evolution of Stars : The Photospheric Abundance Connection, 63–69. Dordrecht : Springer Netherlands, 1991. http://dx.doi.org/10.1007/978-94-011-3416-3_7.
Texte intégral« Le système solaire ». Dans Cahier Découverte Astronomie, 14–17. EDP Sciences, 2009. http://dx.doi.org/10.1051/978-2-7598-0332-3.c004.
Texte intégralActes de conférences sur le sujet "Evolution du système solaire"
Lagarde, Quentin, Serge Mazen, Bruno Beillard, Julien Leylavergne, Joel Andrieu, Jean-Pierre Cancès, Vahid Meghdadi, Michelle Lalande, Edson Martinod et Marie-Sandrine Denis. « Étude et conception de système de management pour batteries innovantes, Batterie Sodium (NA-ion) ». Dans Les journées de l'interdisciplinarité 2022. Limoges : Université de Limoges, 2022. http://dx.doi.org/10.25965/lji.581.
Texte intégralPalouš, Jan, Richard Wünsch, Vasile Mioc, Cristiana Dumitrache et Nedelia A. Popescu. « Star Formation and Evolution of Galaxies ». Dans EXPLORING THE SOLAR SYSTEM AND THE UNIVERSE. AIP, 2008. http://dx.doi.org/10.1063/1.2993679.
Texte intégralLiu, Ming-Chang. « Short-lived radionuclides in the early Solar System ». Dans ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2011. AIP, 2012. http://dx.doi.org/10.1063/1.4763372.
Texte intégralBassino, Lilia P., Vasile Mioc, Cristiana Dumitrache et Nedelia A. Popescu. « Extragalactic Globular Clusters : Tracers of Galaxy Evolution ». Dans EXPLORING THE SOLAR SYSTEM AND THE UNIVERSE. AIP, 2008. http://dx.doi.org/10.1063/1.2993677.
Texte intégralNittler, Larry R. « Presolar supernova and nova dust in the solar system ». Dans ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2011. AIP, 2012. http://dx.doi.org/10.1063/1.4763371.
Texte intégralKSANFOMALITY, LEONID. « EVOLUTION OF SOLAR SYSTEM BODIES AND THEIR COMPARISON WITH EXOPLANETARY SYSTEMS ». Dans Proceedings of the Conference on Future of the Universe and the Future of Our Civilization. WORLD SCIENTIFIC, 2000. http://dx.doi.org/10.1142/9789812793324_0017.
Texte intégralFranck, S., et Ch Bounama. « Mantle devolatilization and rheology in the framework of planetary evolution ». Dans Volatiles in the Earth and solar system. AIP, 1995. http://dx.doi.org/10.1063/1.48749.
Texte intégralLodders, K., et B. Fegley. « The origin and evolution of the terrestrial alkali element budget ». Dans Volatiles in the Earth and solar system. AIP, 1995. http://dx.doi.org/10.1063/1.48754.
Texte intégralCarvajal, Javier López, Jose M. Barea, Jose Barragan et Thomas Altmann. « Developer view of the CSP evolution ». Dans SOLARPACES 2016 : International Conference on Concentrating Solar Power and Chemical Energy Systems. Author(s), 2017. http://dx.doi.org/10.1063/1.4984575.
Texte intégralMarov, M. Ya, et I. I. Shevchenko. « Planets — a modern view ». Dans ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES. Proceedings of the VAK-2021 conference, Aug 23–28, 2021. Crossref, 2022. http://dx.doi.org/10.51194/vak2021.2022.1.1.005.
Texte intégralRapports d'organisations sur le sujet "Evolution du système solaire"
Sussman, Gerald J., et Jack Wisdom. Chaotic Evolution of the Solar System. Fort Belvoir, VA : Defense Technical Information Center, mars 1992. http://dx.doi.org/10.21236/ada260055.
Texte intégralThees, Oliver, Matthias Erni, Vanessa Burg, Gillianne Bowman, Serge Biollaz, Theodoros Damartzis, Timothy Griffin et al. Le bois-énergie en Suisse : potentiel énergétique, développement technologique, mobilisation des ressources et rôle dans la transition énergétique. Livre blanc. Swiss Federal Institute for Forest, Snow and Landscape Research, WSL, avril 2023. http://dx.doi.org/10.55419/wsl:32793.
Texte intégral