Auswahl der wissenschaftlichen Literatur zum Thema „Formation of the solar system“
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Zeitschriftenartikel zum Thema "Formation of the solar system"
Smith, Keith T. „Timing Solar System formation“. Science 370, Nr. 6518 (12.11.2020): 805.13–807. http://dx.doi.org/10.1126/science.370.6518.805-m.
Der volle Inhalt der QuelleMorfill, G. E. „Models of solar system formation“. Chemical Geology 70, Nr. 1-2 (August 1988): 32. http://dx.doi.org/10.1016/0009-2541(88)90268-9.
Der volle Inhalt der QuelleRawal, J. J. „Formation of the solar system“. Astrophysics and Space Science 119, Nr. 1 (Januar 1986): 159–66. http://dx.doi.org/10.1007/bf00648837.
Der volle Inhalt der QuellePfalzner, S., M. B. Davies, M. Gounelle, A. Johansen, C. Münker, P. Lacerda, S. Portegies Zwart, L. Testi, M. Trieloff und D. Veras. „The formation of the solar system“. Physica Scripta 90, Nr. 6 (21.04.2015): 068001. http://dx.doi.org/10.1088/0031-8949/90/6/068001.
Der volle Inhalt der QuelleRussell, Sara S. „The Formation of the Solar System“. Journal of the Geological Society 164, Nr. 3 (Mai 2007): 481–92. http://dx.doi.org/10.1144/0016-76492006-054.
Der volle Inhalt der QuelleChambers, John. „Making the Solar System“. Astrophysical Journal 944, Nr. 2 (01.02.2023): 127. http://dx.doi.org/10.3847/1538-4357/aca96f.
Der volle Inhalt der QuelleIda, Shigeru, und Eiichiro Kokubo. „Terrestrial Planet Formation: The Solar System and Other Systems“. Symposium - International Astronomical Union 202 (2004): 159–66. http://dx.doi.org/10.1017/s0074180900217749.
Der volle Inhalt der QuelleImaeda, Yusuke, und Toshikazu Ebisuzaki. „Tandem planet formation for solar system-like planetary systems“. Geoscience Frontiers 8, Nr. 2 (März 2017): 223–31. http://dx.doi.org/10.1016/j.gsf.2016.06.011.
Der volle Inhalt der QuelleYu, Ziyuan, Jin Liu, Chao Pan, Lvqian Guo, Zhiwei Kang und Xin Ma. „Solar TDOA measurement and integrated navigation for formation flying“. Proceedings of the Institution of Mechanical Engineers, Part G: Journal of Aerospace Engineering 233, Nr. 12 (Februar 2019): 4635–45. http://dx.doi.org/10.1177/0954410019827148.
Der volle Inhalt der QuelleSmith, Keith T. „Two-part formation of the Solar System“. Science 371, Nr. 6527 (21.01.2021): 358.4–359. http://dx.doi.org/10.1126/science.371.6527.358-d.
Der volle Inhalt der QuelleDissertationen zum Thema "Formation of the solar system"
Crida, Aurélien. „Planetary migration in solar system formation“. Nice, 2006. http://www.theses.fr/2006NICE4076.
Der volle Inhalt der QuelleLa migration planétaire est un phénomène apparemment inévitable lors de la formation des planètes dans les disques protoplanétaires. Les interactions gravitationnelles entre les embryons de planète et le disque de gaz font décroître le moment cinétique de l'embryon, qui spirale vers l'étoile centrale. Le temps de migration étant plus court que la durée de vie du disque, aucune planète ne devrait survivre (chapitres 1 et 2). Dans cette thèse, nous essayons de trouver des mécanismes qui empêchent ou ralentissent la migration. Dans le chapitre 3, nous montrons qu'un saut dans le profil de densité du disque de gaz bloque la migration et agit comme un piège à planète. Ainsi bloqué, un coeur solide massif peut accrèter une atmosphère gazeuse et devenir une planète géante. La planète est alors assez massive pour repousser le gaz et ouvrir un sillon autour de son orbite. En analysant des simulations numériques, nous mettons en évidence le rôle des effets de pression dans ce processus dans le chapitre 4; un nouveau critère unifié d'ouverture du sillon en découle. Après la présentation dans le chapitre 5 d'un nouvel algorithme fiable et performant pour réaliser des simulations numériques, nous l'utilisons dans le chapitre 6 pour étudier la migration d'une planète géante et son impact sur l'évolution du disque. La formation d'une cavité s'avère moins facile que prévu, mais une possibilité d'arrêter la migration apparaît. Enfin, dans le chapitre 7, nous étudions le cas de Jupiter et Saturne, et trouvons dans quelles conditions les interactions entre les deux planètes en empêchent la migration
Cyr, Kimberly Ellen 1964. „The distribution of water in the solar nebula: Implications for solar system formation“. Diss., The University of Arizona, 1998. http://hdl.handle.net/10150/288870.
Der volle Inhalt der QuelleElliott, Garrett T. „Detecting the debris of solar system formation via stellar occultation“. Connect to resource, 2008. http://hdl.handle.net/1811/32191.
Der volle Inhalt der QuelleMehta, Anand Vivek 1966. „The role of vortices in the formation of the solar system“. Thesis, Massachusetts Institute of Technology, 1998. http://hdl.handle.net/1721.1/50500.
Der volle Inhalt der QuelleIncludes bibliographical references (p. 117-119).
An important part of explaining planet formation is understanding how small particles accumulate into larger bodies. Gas vortices are suggested as a mechanism to enhance the coagulation of dust particles in the solar nebula. An inviscid, barotropic, two-dimensional form of the vorticity equation is derived to study the gas flow. A pseudospectral numerical model uses this equation to calculate the evolution of the vorticity field. The calculations show that locally prograde elliptical vortices with the major axis parallel to the angular axis can persist for at least 103 years with less than 1% change in peak vorticity. The shape of the vortex depends on the strength, similar to analytical expressions for elliptical vortices in a linear shear. Stronger vortices are rounder while weaker vortices are elongated; With ratios of the peak vorticity to the background vorticity of 1.0 and 0.2, the aspect ratios are approximately 0.5 and 0.25. The vortex area is mostly constant, and the linear dimensions change as the shape changes. Two negative vortices within the same radial band tend to merge, forming a larger, stronger vortex in a few orbit periods. A random viscosity field tends to have a few strong vortices form, although not as efficiently as with merging vortices. Dust particles interact with the gas through the Stokes drag force, with the relaxation time specifying how quickly the particle velocity approaches the gas velocity. The particles tend to converge in high pressure vortices and drift out of low pressure systems. The convergence time is dependent on the vortex strength and the particle relaxation time. If the relaxation time is short compared to the period, the particles do not have an appreciable differential velocity compared to the gas, and the Stokes drag force is small. If the relaxation time is long, then the Stokes drag force is not large enough to have a significant effect. If, however, the relaxation time is of the same order as the period, so the dynamical and frictional timescales are similar, then the particles will have the shortest convergence times. This result can be seen analytically in the simple case of an axisymmetric pressure band and numerically in calculations involving the robust vortex. With a robust vortex, the convergence times are approximately 3-4 yr for relaxation times of 0.1-0.2 yr. For typical values of properties of the solar nebula, this relaxation time applies for particles with diameters of around 20 cm. Other particles, both smaller and larger, converge more slowly, but the different times result in more collisions, enhancing the coagulation of larger bodies.
by Anand Vivek Mehta.
Ph.D.
Lawler, Samantha. „The leftovers of planet formation : small body populations of our solar system and exoplanet systems“. Thesis, University of British Columbia, 2013. http://hdl.handle.net/2429/44760.
Der volle Inhalt der QuellePatzelt, Madelein [Verfasser], und Klaus [Akademischer Betreuer] Mezger. „Chondrule formation in the early Solar System / Madelein Patzelt ; Betreuer: Klaus Mezger“. Münster : Universitäts- und Landesbibliothek Münster, 2015. http://d-nb.info/1138279943/34.
Der volle Inhalt der QuelleTheis, Karen Julia. „Iron isotope fractionation of planetary bodies during early solar system formation processes“. Thesis, University of Manchester, 2008. http://www.manchester.ac.uk/escholar/uk-ac-man-scw:163898.
Der volle Inhalt der QuelleGorlova, Nadiya Igorivna. „Debris Disks in Open Stellar Clusters“. Diss., The University of Arizona, 2006. http://hdl.handle.net/10150/195908.
Der volle Inhalt der QuelleMiller, Kelly E., und Kelly E. Miller. „The R Chondrite Record of Volatile-Rich Environments in the Early Solar System“. Diss., The University of Arizona, 2016. http://hdl.handle.net/10150/621016.
Der volle Inhalt der QuelleWilliams, Niel Hamilton. „Titanium isotope cosmochemistry“. Thesis, University of Manchester, 2015. https://www.research.manchester.ac.uk/portal/en/theses/titanium-isotope-cosmochemistry(571ae148-1673-4b85-bc10-937284bb53fc).html.
Der volle Inhalt der QuelleBücher zum Thema "Formation of the solar system"
Ferronsky, V. I., und S. V. Ferronsky. Formation of the Solar System. Dordrecht: Springer Netherlands, 2013. http://dx.doi.org/10.1007/978-94-007-5908-4.
Der volle Inhalt der QuelleRossi, Matteo De. Solar system: Structure, formation, and exploration. Hauppauge, N.Y: Nova Science Publisher's, 2011.
Den vollen Inhalt der Quelle findenAnfilogov, Vsevolod N., und Yurij V. Khachay. Some Aspects of the Formation of the Solar System. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-17831-8.
Der volle Inhalt der QuelleMandt, Kathleen, Olivier Mousis, Dominique Bockelée-Morvan und Christopher Russell, Hrsg. Comets as Tracers of Solar System Formation and Evolution. Dordrecht: Springer Netherlands, 2017. http://dx.doi.org/10.1007/978-94-024-1103-4.
Der volle Inhalt der QuellePessah, Martin, und Oliver Gressel, Hrsg. Formation, Evolution, and Dynamics of Young Solar Systems. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-60609-5.
Der volle Inhalt der QuelleFormation of water and our solar system from a fission process with an. [Place of publication not identified]: Xlibris Corporation, 2011.
Den vollen Inhalt der Quelle findenESLAB Symposium. (24th 1990 Friedrichshafen, Germany). Formation of stars and planets and the evolution of the solar system: Proceedings of the 24th ESLAB Symposium, 17 - 19 September 1990, Friedrichshafen, Germany. Herausgegeben von Battrick B. 1946-, Schwehm G, Stammes P und European Space Agency. Noordwijk, The Netherlands: ESA Publications, 1990.
Den vollen Inhalt der Quelle finden1953-, Weaver Harold A., Danly L und Space Telescope Science Institute (U.S.), Hrsg. The formation and evolution of planetary systems: Proceedings of the Formation and Evolution of Planetary Systems Meeting, Baltimore, 1988, May 9-11. Cambridge: Cambridge University Press, 1989.
Den vollen Inhalt der Quelle findenUnited States. National Aeronautics and Space Administration., Hrsg. Origins of interstellar and solar system carbonaceous materials: Final technical report. [Washington, DC: National Aeronautics and Space Administration, 1994.
Den vollen Inhalt der Quelle findenV, Ferronskiĭ S., Hrsg. Formation of the solar system: A new theory of the creation and decay of the celestial bodies. Dordrecht: Springer, 2013.
Den vollen Inhalt der Quelle findenBuchteile zum Thema "Formation of the solar system"
Crida, Aurélien. „Solar System Formation“. In Reviews in Modern Astronomy, 215–27. Weinheim, Germany: Wiley-VCH Verlag GmbH & Co. KGaA, 2010. http://dx.doi.org/10.1002/9783527629190.ch12.
Der volle Inhalt der QuelleRobert, François. „Solar System Formation (Chronology)“. In Encyclopedia of Astrobiology, 1528–35. Berlin, Heidelberg: Springer Berlin Heidelberg, 2011. http://dx.doi.org/10.1007/978-3-642-11274-4_1797.
Der volle Inhalt der QuelleSouthwood, D. J. „Formation of Magnetotails“. In Magnetotails in the Solar System, 197–215. Hoboken, NJ: John Wiley & Sons, Inc, 2015. http://dx.doi.org/10.1002/9781118842324.ch12.
Der volle Inhalt der QuellePetit, Jean-Marc, und Alessandro Morbidelli. „Chronology of Solar System Formation“. In Lectures in Astrobiology, 61–82. Berlin, Heidelberg: Springer Berlin Heidelberg, 2005. http://dx.doi.org/10.1007/10913406_3.
Der volle Inhalt der QuelleRobert, François. „System Solar Formation, Chronology of“. In Encyclopedia of Astrobiology, 2450–58. Berlin, Heidelberg: Springer Berlin Heidelberg, 2015. http://dx.doi.org/10.1007/978-3-662-44185-5_1797.
Der volle Inhalt der QuelleRawal, J. J. „Formation of the Solar System“. In Third Asian-Pacific Regional Meeting of the International Astronomical Union, 159–66. Dordrecht: Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4630-9_37.
Der volle Inhalt der QuelleRobert, François. „System Solar Formation, Chronology of“. In Encyclopedia of Astrobiology, 1–9. Berlin, Heidelberg: Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-27833-4_1797-2.
Der volle Inhalt der QuelleRobert, François. „System Solar Formation, Chronology of“. In Encyclopedia of Astrobiology, 2985–93. Berlin, Heidelberg: Springer Berlin Heidelberg, 2023. http://dx.doi.org/10.1007/978-3-662-65093-6_1797.
Der volle Inhalt der QuelleBally, John, Alan Boss, Dimitri Papanastassiou, Scott Sandford und Anneila Sargent. „Star Formation and the Solar System“. In Galactic and Extragalactic Star Formation, 311–27. Dordrecht: Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2973-9_19.
Der volle Inhalt der QuellePirronello, Valerio. „Molecule Formation in Cometary Environments“. In Ices in the Solar System, 261–72. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5418-2_17.
Der volle Inhalt der QuelleKonferenzberichte zum Thema "Formation of the solar system"
Palouš, Jan, Richard Wünsch, Vasile Mioc, Cristiana Dumitrache und Nedelia A. Popescu. „Star Formation and Evolution of Galaxies“. In EXPLORING THE SOLAR SYSTEM AND THE UNIVERSE. AIP, 2008. http://dx.doi.org/10.1063/1.2993679.
Der volle Inhalt der QuelleKadik, A. A. „Formation of carbon species in terrestrial magmas“. In Volatiles in the Earth and solar system. AIP, 1995. http://dx.doi.org/10.1063/1.48734.
Der volle Inhalt der QuelleLunine, Jonathan I., Wei Dai und Fatima Ebrahim. „Solar system formation and the distribution of volatile species“. In Volatiles in the Earth and solar system. AIP, 1995. http://dx.doi.org/10.1063/1.48735.
Der volle Inhalt der QuelleBilenko, I. A., Vasile Mioc, Cristiana Dumitrache und Nedelia A. Popescu. „Conditions for the formation of CMEs associated with filament eruptions“. In EXPLORING THE SOLAR SYSTEM AND THE UNIVERSE. AIP, 2008. http://dx.doi.org/10.1063/1.2993659.
Der volle Inhalt der QuelleLichtenberg, Tim, Joanna Drążkowska, Maria Schönbächler, Gregor Golabek und Thomas Hands. „Bifurcation of planetary building blocks during Solar System formation“. In Goldschmidt2021. France: European Association of Geochemistry, 2021. http://dx.doi.org/10.7185/gold2021.4476.
Der volle Inhalt der QuelleLi, Ming, Huizhu Yang, Gedong Jiang, Wenjun Wang und Xuesong Mei. „Formation of nanostructures on the surface of CIGS films by picosecond laser with different beam patterns“. In Photonics for Solar Energy Systems, herausgegeben von Ralf B. Wehrspohn und Alexander N. Sprafke. SPIE, 2018. http://dx.doi.org/10.1117/12.2306814.
Der volle Inhalt der QuelleTakeichi, Noboru. „Feasibility Study of a Solar Power Satellite System Configured by Formation Flying“. In 54th International Astronautical Congress of the International Astronautical Federation, the International Academy of Astronautics, and the International Institute of Space Law. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2003. http://dx.doi.org/10.2514/6.iac-03-r.1.07.
Der volle Inhalt der QuelleYoung, Edward, und Michelle Jordan. „IRON ISOTOPE CONSTRAINTS ON PLANETESIMAL CORE FORMATION IN THE EARLY SOLAR SYSTEM“. In GSA Annual Meeting in Denver, Colorado, USA - 2016. Geological Society of America, 2016. http://dx.doi.org/10.1130/abs/2016am-284424.
Der volle Inhalt der QuelleCassen, Patrick, und Kenneth M. Chick. „The survival of presolar grains during the formation of the solar system“. In ASTROPHYSICAL IMPLICATIONS OF THE LABORATORY STUDY OF PRESOLAR MATERIALS. ASCE, 1997. http://dx.doi.org/10.1063/1.53324.
Der volle Inhalt der QuelleTamura, M., M. Takami, K. Enya, T. Ootsubo, M. Fukagawa, M. Honda, Y. K. Okamoto et al. „Key Sciences of SPICA Mission: Planetary Formation, Exoplanets, and our Solar System“. In SPICA joint European/Japanese Workshop. Les Ulis, France: EDP Sciences, 2009. http://dx.doi.org/10.1051/spica/200902001.
Der volle Inhalt der QuelleBerichte der Organisationen zum Thema "Formation of the solar system"
Brown, W. K. High explosive simulations of supernovae and the supernova shell fragmentation model of solar system formation. Office of Scientific and Technical Information (OSTI), September 1987. http://dx.doi.org/10.2172/6019760.
Der volle Inhalt der QuelleBARKHATOV, NIKOLAY, und SERGEY REVUNOV. A software-computational neural network tool for predicting the electromagnetic state of the polar magnetosphere, taking into account the process that simulates its slow loading by the kinetic energy of the solar wind. SIB-Expertise, Dezember 2021. http://dx.doi.org/10.12731/er0519.07122021.
Der volle Inhalt der QuelleMoens, L., und D. Blake. Mechanism of Hydrogen Formation in Solar Paraboic Trough Receivers. Office of Scientific and Technical Information (OSTI), Februar 2008. http://dx.doi.org/10.2172/924987.
Der volle Inhalt der QuelleHamilton, C. Views of the solar system. Office of Scientific and Technical Information (OSTI), Februar 1995. http://dx.doi.org/10.2172/10116814.
Der volle Inhalt der QuelleSussman, Gerald J., und Jack Wisdom. Chaotic Evolution of the Solar System. Fort Belvoir, VA: Defense Technical Information Center, März 1992. http://dx.doi.org/10.21236/ada260055.
Der volle Inhalt der QuelleWesle, Max, und Robert Buchinger. INFO Sheet C03: One-World-Solar-System. IEA SHC Task 54, November 2017. http://dx.doi.org/10.18777/ieashc-task54-2017-0014.
Der volle Inhalt der QuelleMills, A., A. Botterud, J. Wu, Z. Zhou, B.-M. Hodge und M. Heaney. Integrating Solar PV in Utility System Operations. Office of Scientific and Technical Information (OSTI), November 2013. http://dx.doi.org/10.2172/1107495.
Der volle Inhalt der QuelleBaines, K. H., D. T. Gavel, A. M. Getz, S. G. Gibbartd, B. MacIntosh, C. E. Max, C. P. McKay, E. F. Young und I. de Pater. Solar system events at high spatial resolution. Office of Scientific and Technical Information (OSTI), Februar 1999. http://dx.doi.org/10.2172/12548.
Der volle Inhalt der QuelleMills, A., A. Botterud, J. Wu, Z. Zhou, B.-M. Hodge und M. Heany. Integrating Solar PV in Utility System Operations. Office of Scientific and Technical Information (OSTI), Oktober 2013. http://dx.doi.org/10.2172/1164898.
Der volle Inhalt der QuelleSkordos, Panayotis A. Multistep Methods for Integrating the Solar System. Fort Belvoir, VA: Defense Technical Information Center, Juli 1988. http://dx.doi.org/10.21236/ada201692.
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