Literatura científica selecionada sobre o tema "Formation and evolution of planetary systems"
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Artigos de revistas sobre o assunto "Formation and evolution of planetary systems"
Burke, Bernard F. "Planetary systems: Formation, evolution, and detection - introduction". Astrophysics and Space Science 212, n.º 1-2 (fevereiro de 1994): xi—xii. http://dx.doi.org/10.1007/bf00984502.
Texto completo da fonteHoredt, G. P. "The Formation and evolution of planetary systems". Physics of the Earth and Planetary Interiors 67, n.º 3-4 (julho de 1991): 392–94. http://dx.doi.org/10.1016/0031-9201(91)90035-g.
Texto completo da fonteOwen, Tobias. "The formation and evolution of planetary systems". Icarus 91, n.º 2 (junho de 1991): 334–35. http://dx.doi.org/10.1016/0019-1035(91)90029-s.
Texto completo da fonteLipschutz, Michael E. "The formation and evolution of planetary systems". Geochimica et Cosmochimica Acta 54, n.º 4 (abril de 1990): 1196. http://dx.doi.org/10.1016/0016-7037(90)90455-t.
Texto completo da fonteKley, Wilhelm. "Formation and Orbital Evolution of Planets". Proceedings of the International Astronomical Union 7, S282 (julho de 2011): 429–36. http://dx.doi.org/10.1017/s1743921311027980.
Texto completo da fonteVeras, Dimitri. "Post-main-sequence planetary system evolution". Royal Society Open Science 3, n.º 2 (fevereiro de 2016): 150571. http://dx.doi.org/10.1098/rsos.150571.
Texto completo da fonteLin, D. N. C. "Planetary Formation in Protostellar Disks". International Astronomical Union Colloquium 163 (1997): 321–30. http://dx.doi.org/10.1017/s0252921100042792.
Texto completo da fonteMarzari, Francesco, e Philippe Thebault. "Planets in Binaries: Formation and Dynamical Evolution". Galaxies 7, n.º 4 (16 de outubro de 2019): 84. http://dx.doi.org/10.3390/galaxies7040084.
Texto completo da fonteKawai, Toshio. "Pattern Formation by Inelastic Collisions, Especially in Planetary Systems". International Journal of Modern Physics B 12, n.º 03 (30 de janeiro de 1998): 309–60. http://dx.doi.org/10.1142/s0217979298000247.
Texto completo da fonteSalnikova, T. V., S. Ya Stepanov e E. I. Kugushev. "Possible models of the planetary systems formations". International Journal of Modern Physics A 35, n.º 02n03 (30 de janeiro de 2020): 2040061. http://dx.doi.org/10.1142/s0217751x20400618.
Texto completo da fonteTeses / dissertações sobre o assunto "Formation and evolution of planetary systems"
Inamdar, Niraj K. "The formation and evolution of planetary systems". Thesis, Massachusetts Institute of Technology, 2016. http://hdl.handle.net/1721.1/107104.
Texto completo da fonteCataloged from PDF version of thesis.
Includes bibliographical references (pages 299-311).
The Kepler space observatory and other surveys have revealed thousands of planets and planetary systems that look significantly different from our own. In particular, the preponderance of super-Earths and mini-Neptunes (planets with radii smaller than Neptune's but larger than Earth's) at short orbital radii has challenged planet formation theories developed in the context of our own Solar System. How and where these planets form remains an outstanding question. Given the large frequency with which such planets occur around other stars, understanding the formation pathways of these planets has the potential to reveal dominant mechanisms for planet formation and evolution and to place our own Solar System within a broader context. The purpose of this thesis is to address and develop frameworks by which these questions can be answered. The thesis is comprised of two parts. In Part I, we consider the question of how and where close-in exoplanets formed. We do this in two ways. First, we use that fact that many close-in super-Earths and mini-Neptunes possess gaseous envelopes that comprise several percent or more of the total planet mass in order to construct a self-consistent planet formation history that accounts for core accretion, thermal evolution, and dynamical interactions during the core assembly process via giant impacts. We find that envelope masses accreted from the gas disc by planetary embryos are typically much smaller than those inferred for many exoplanets, and that the envelope mass fraction is further reduced substantially during the assembly phase when embryos merge. Fully assembled planets can accrete observed envelope masses from the residual disc only if energy exchange between the envelope and the underlying core is totally inhibited. It is therefore very unlikely that such planets formed at their observed semimajor axes, but instead formed further out and migrated inwards. Second, we consider the late-stage evolution of exoplanets after gas disc dissipation in order to explain the bulk structural diversity of observed super-Earths and mini-Neptunes. Whereas naive application of core accretion models suggests a narrow mass-radius relationship for these exoplanets, the population possesses a great deal of diversity in mean density. While photoevaporative mass loss from the host star is the most-commonly invoked explanation for this diversity, we use the fact that many exoplanetary systems are in tightly packed orbital configurations to propose instead that late-stage collisions are at least in part responsible for the observed diversity. We infer envelope mass fractions for planets in the literature whose masses and radii have been measured, and on the basis of this, we identify multiplanet systems whose bulk structural diversity favors late-stage impacts as opposed to photoevaporative devolatilization. In Part II, we turn our attention to the formation and evolution of our own Solar System. We do this within the context of NASA's OSIRIS-REx asteroid sample return mission. OSIRIS-REx, which launches in September 2016, will arrive at the near-Earth asteroid 101955 Bennu in 2019 with the objective of constraining its composition, orbit, and other bulk properties. In order to better understand the composition of Bennu, an instrument designed to measure its elemental abundances via X-ray fluorescence spectroscopy called REXIS was developed and built at MIT. In this part of the thesis, we investigate the ability of REXIS to constrain the composition of Bennu via fluorescence spectroscopy, as well as its potential to place Bennu within an analogue meteorite class. We carry out our analysis by modeling Solar X-ray activity and the X-ray fluorescence from Bennu, as well as by simulating data product and analysis from the instrument in order to predict REXIS's ability to carry out its goal of contextualizing Bennu within the asteroid and meteorite population.
by Niraj K. Inamdar.
Ph. D. in Planetary Science
Payne, Matthew John. "On the formation and evolution of planetary systems". Thesis, University of Cambridge, 2009. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.611755.
Texto completo da fonteHands, Thomas Oliver. "The enthralling tale of the formation and evolution of compact planetary systems". Thesis, University of Leicester, 2016. http://hdl.handle.net/2381/38766.
Texto completo da fonteDavies, Claire L. "Revolution evolution : tracing angular momentum during star and planetary system formation". Thesis, University of St Andrews, 2015. http://hdl.handle.net/10023/7557.
Texto completo da fonteMeng, Huan Y. A., George H. Rieke, Kate Y. L. Su e András Gáspár. "The First 40 Million Years of Circumstellar Disk Evolution: The Signature of Terrestrial Planet Formation". IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/623246.
Texto completo da fonteTrilling, David Eric. "A theoretical and observational study of the formation and evolution of planetary systems and extrasolar planets". Diss., The University of Arizona, 1999. http://hdl.handle.net/10150/288998.
Texto completo da fonteNgo, Henry, Heather A. Knutson, Sasha Hinkley, Marta Bryan, Justin R. Crepp, Konstantin Batygin, Ian Crossfield et al. "FRIENDS OF HOT JUPITERS. IV. STELLAR COMPANIONS BEYOND 50 au MIGHT FACILITATE GIANT PLANET FORMATION, BUT MOST ARE UNLIKELY TO CAUSE KOZAI–LIDOV MIGRATION". IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621385.
Texto completo da fontePhilipot, 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.
Texto completo da fonteThe 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
Tabera, Martin Luis. "Evolution and properties of planetary systems". Thesis, Uppsala universitet, Observationell astrofysik, 2020. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-438128.
Texto completo da fonteBonsor, Amy Hannah Clay. "Post-main sequence evolution of planetary systems". Thesis, University of Cambridge, 2011. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.609856.
Texto completo da fonteLivros sobre o assunto "Formation and evolution of planetary systems"
Burke, Bernard F., Jürgen H. Rahe e Elizabeth E. Roettger, eds. Planetary Systems: Formation, Evolution, and Detection. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6.
Texto completo da fonte1953-, Weaver Harold A., Danly L e Space Telescope Science Institute (U.S.), eds. 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.
Encontre o texto completo da fonteN, Kylafis, e Lada Charles J, eds. The Origin of stars and planetary systems. Boston, Mass: Kluwer Academic, 1999.
Encontre o texto completo da fonteJ, Lada Charles, Kylafis N e NATO Advanced Study Institute on the Physics of Star Formation and Early Stellar Evolution (2nd : 1998 : Crete, Greece), eds. The origin of stars and planetary systems. Dordrecht: Kluwer Academic Publishers, 1999.
Encontre o texto completo da fonteUnited States. National Aeronautics and Space Administration., ed. Formation of the giant planets by concurrent accretion of solids and gas: Final technical report : grant number: NAG2-984. [Washington, DC: National Aeronautics and Space Administration, 1997.
Encontre o texto completo da fonte1928-, Burke Bernard F., Rahe Jürgen H. Rahe e Roettger Elizabeth E, eds. Planetary systems: Formation, evolution, and detection : proceedings of the first international conference, held in Pasadena, California on December 8-10, 1992. Dordrecht: Kluwer Academic, 1994.
Encontre o texto completo da fontePackevich, Alla. Architecture of Evolution. ru: INFRA-M Academic Publishing LLC., 2021. http://dx.doi.org/10.12737/1079356.
Texto completo da fonteAlessandro, Sozzetti, Lattanzi Mario G, Boss Alan 1951- e International Astronomical Union, eds. The astrophysics of planetary systems: Formation, structure, and dynamical evolution : proceedings of the 276th Symposium of the International Astronomical Union, held in Torino, Italy, October 10-15, 2010. Cambridge, U.K: Cambridge University Press, 2011.
Encontre o texto completo da fonteAlan, Penny, ed. Planetary systems in the universe: Observation, formation and evolution : proceedings of the 202nd Symposium of the International Astronomical Union held at University of Manchester, Manchester, United Kingdom, August 7-10, 2000. [San Francisco, Calif.]: Published on behalf of the IAU by Astronomical Society of the Pacific, 2004.
Encontre o texto completo da fonteDvorak, R., e J. Henrard, eds. Long Term Evolution of Planetary Systems. Dordrecht: Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2285-3.
Texto completo da fonteCapítulos de livros sobre o assunto "Formation and evolution of planetary systems"
Bonsor, Amy, e Siyi Xu. "White Dwarf Planetary Systems: Insights Regarding the Fate of Planetary Systems". In Formation, Evolution, and Dynamics of Young Solar Systems, 229–52. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-60609-5_8.
Texto completo da fonteSafronov, V. S., e E. L. Ruskol. "Formation and Evolution of Planets". In Planetary Systems: Formation, Evolution, and Detection, 13–22. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6_2.
Texto completo da fonteFierro, J. "Interaction of Planetary Nebulae with Prenebulae Debris". In Planetary Systems: Formation, Evolution, and Detection, 61–65. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6_8.
Texto completo da fonteCruikshank, D. P., M. W. Werner e D. E. Backman. "SIRTF: Capabilities for the Study of Planetary Systems". In Planetary Systems: Formation, Evolution, and Detection, 407–15. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6_42.
Texto completo da fonteDonn, Bertram, e J. Mark Duva. "Formation and Properties of Fluffy Planetesimals". In Planetary Systems: Formation, Evolution, and Detection, 43–47. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6_5.
Texto completo da fonteWetherill, George W. "Possible Consequences of Absence of “Jupiters“ in Planetary Systems". In Planetary Systems: Formation, Evolution, and Detection, 23–32. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6_3.
Texto completo da fonteSargent, A. I., e S. V. W. Beckwith. "The Detection and Study of Pre-Planetary Disks". In Planetary Systems: Formation, Evolution, and Detection, 181–89. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6_20.
Texto completo da fonteOwen, T. "The Search for Other Planets: Clues from the Solar System". In Planetary Systems: Formation, Evolution, and Detection, 1–11. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6_1.
Texto completo da fontePeale, S. J. "On the Detection of Mutual Perturbations as Proof of Planets Around PSR1257+12". In Planetary Systems: Formation, Evolution, and Detection, 77–89. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6_10.
Texto completo da fontePhillips, J. A., e S. E. Thorsett. "Planets Around Pulsars: A Review". In Planetary Systems: Formation, Evolution, and Detection, 91–106. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6_11.
Texto completo da fonteTrabalhos de conferências sobre o assunto "Formation and evolution of planetary systems"
Grady, C. A., Michael E. Van Steenberg, George Sonneborn, H. Warren Moos e William P. Blair. "Planetary System Formation and Evolution: The FUSE Legacy and Future FUV Potential". In FUTURE DIRECTIONS IN ULTRAVIOLET SPECTROSCOPY: A Conference Inspired by the Accomplishments of the Far Ultraviolet Spectroscopic Explorer Mission. AIP, 2009. http://dx.doi.org/10.1063/1.3154058.
Texto completo da fonteMarov, M. Ya, e I. I. Shevchenko. "Planets — a modern view". In 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.
Texto completo da fonteOtsuka, M., H. Izumiura, A. Tajitsu, S. Hyung, Takuma Suda, Takaya Nozawa, Akira Ohnishi et al. "The Origin and Evolution of the Extremely Metal-Poor Halo Planetary Nebulae". In ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: The 10th International Symposium on Origin of Matter and Evolution of Galaxies: From the Dawn of Universe to the Formation of Solar System. AIP, 2008. http://dx.doi.org/10.1063/1.2943614.
Texto completo da fonteAbdulmyanov, T. "Comparison of the dynamics of Jupiter’s coorbital asteroids and the dynamics of bodies in debris disks". In 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/vak2021.2022.1.1.018.
Texto completo da fonteAthanassoula, E. "Formation and Dynamical Evolution of Galaxies and of their Components". In PLANETARY NEBULAE AS ASTRONOMICAL TOOLS: International Conference on Planetary Nebulae as Astronomical Tools. AIP, 2005. http://dx.doi.org/10.1063/1.2146306.
Texto completo da fonteChiappini, Cristina. "Low and Intermediate Mass Stars as Tools to Understand Stellar Evolution and the Formation of the Milky Way". In PLANETARY NEBULAE AS ASTRONOMICAL TOOLS: International Conference on Planetary Nebulae as Astronomical Tools. AIP, 2005. http://dx.doi.org/10.1063/1.2146288.
Texto completo da fonteSavage, Paul, e Frédéric Moynier. "Planetary formation and evolution through the lens of zinc and copper isotopes". In Goldschmidt2023. France: European Association of Geochemistry, 2023. http://dx.doi.org/10.7185/gold2023.20371.
Texto completo da fonteRein, Hanno, John C. B. Papaloizou, Tomonori Usuda, Motohide Tamura e Miki Ishii. "Formation of Multi-planetary Systems in Turbulent Disks". In EXOPLANETS AND DISKS: THEIR FORMATION AND DIVERSITY: Proceedings of the International Conference. AIP, 2009. http://dx.doi.org/10.1063/1.3215915.
Texto completo da fonteRein, Hanno, John C. B. Papaloizou, Tomonori Usuda, Motohide Tamura e Miki Ishii. "Formation of Multi-planetary Systems in Turbulent Disks". In EXOPLANETS AND DISKS: THEIR FORMATION AND DIVERSITY: Proceedings of the International Conference. AIP, 2009. http://dx.doi.org/10.1063/1.3215914.
Texto completo da fonteBonsor, Amy, e Mark C. Wyatt. "Post-Main Sequence Evolution of Debris Discs". In PLANETARY SYSTEMS BEYOND THE MAIN SEQUENCE: Proceedings of the International Conference. AIP, 2011. http://dx.doi.org/10.1063/1.3556183.
Texto completo da fonte