Готові списки джерел за темами / Formation and evolution of planetary systems

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  1. Статті в журналах
  2. Дисертації
  3. Книги
  4. Частини книг
  5. Тези доповідей конференцій
  6. Звіти організацій

Добірка наукової літератури з теми "Formation and evolution of planetary systems"

Автор: Grafiati
Опубліковано: 8 червня 2024
Оновлено: 31 липня 2025

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Статті в журналах з теми "Formation and evolution of planetary systems"

1

Burke, Bernard F. "Planetary systems: Formation, evolution, and detection - introduction." Astrophysics and Space Science 212, no. 1-2 (1994): xi—xii. http://dx.doi.org/10.1007/bf00984502.

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Horedt, G. P. "The Formation and evolution of planetary systems." Physics of the Earth and Planetary Interiors 67, no. 3-4 (1991): 392–94. http://dx.doi.org/10.1016/0031-9201(91)90035-g.

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Owen, Tobias. "The formation and evolution of planetary systems." Icarus 91, no. 2 (1991): 334–35. http://dx.doi.org/10.1016/0019-1035(91)90029-s.

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Lipschutz, Michael E. "The formation and evolution of planetary systems." Geochimica et Cosmochimica Acta 54, no. 4 (1990): 1196. http://dx.doi.org/10.1016/0016-7037(90)90455-t.

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5

Kley, Wilhelm. "Formation and Orbital Evolution of Planets." Proceedings of the International Astronomical Union 7, S282 (2011): 429–36. http://dx.doi.org/10.1017/s1743921311027980.

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AbstractThe formation of planetary systems is a natural byproduct of the star formation process. Planets can form inside the protoplanetary disk by two alternative processes. Either through a sequence of sticking collisions, the so-called sequential accretion scenario, or via gravitational instability from an over-dense clump inside the protoplanetary disk. The first process is believed to have occurred in the solar system. The most important steps in this process will be outlined. The observed orbital properties of exoplanetary systems are distinctly different from our own Solar System. In pa
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6

Veras, Dimitri. "Post-main-sequence planetary system evolution." Royal Society Open Science 3, no. 2 (2016): 150571. http://dx.doi.org/10.1098/rsos.150571.

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The fates of planetary systems provide unassailable insights into their formation and represent rich cross-disciplinary dynamical laboratories. Mounting observations of post-main-sequence planetary systems necessitate a complementary level of theoretical scrutiny. Here, I review the diverse dynamical processes which affect planets, asteroids, comets and pebbles as their parent stars evolve into giant branch, white dwarf and neutron stars. This reference provides a foundation for the interpretation and modelling of currently known systems and upcoming discoveries.
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Lin, D. N. C. "Planetary Formation in Protostellar Disks." International Astronomical Union Colloquium 163 (1997): 321–30. http://dx.doi.org/10.1017/s0252921100042792.

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AbstractRecent discoveries of planets around other stars suggest that planets are ubiquitous and their dynamical properties are diverse. We reviewed the formation mechanism for protoplanets and the post-formation planet-disk tidal interaction which may have led the short-period planets to their present configuration. We suggest that these planets may be the survivors of a populations of similar planets which have plunged into and contaminated the stellar convection zone. In the context of the solar system, the mass of the giant planets and the present distribution of the minor planets may be u
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8

Cuello, Nicolás, Antoine Alaguero, and Pedro P. Poblete. "Circumstellar and Circumbinary Discs in Multiple Stellar Systems." Symmetry 17, no. 3 (2025): 344. https://doi.org/10.3390/sym17030344.

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The interplay between stellar multiplicity and protoplanetary discs represents a cornerstone of modern astrophysics, offering key insights into the processes behind planet formation. Protoplanetary discs act as cradles for planetary systems, yet their evolution and capacity to form planets are profoundly affected by gravitational forces within multiple stellar systems. This review synthesizes recent advancements in observational and theoretical studies to explore the rich diversity of circumstellar and circumbinary discs within multiple stellar systems. We examine how stellar companions shape
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Marzari, Francesco, and Philippe Thebault. "Planets in Binaries: Formation and Dynamical Evolution." Galaxies 7, no. 4 (2019): 84. http://dx.doi.org/10.3390/galaxies7040084.

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Binary systems are very common among field stars, yet the vast majority of known exoplanets have been detected around single stars. While this relatively small number of planets in binaries is probably partly due to strong observational biases, there is, however, statistical evidence that planets are indeed less frequent in binaries with separations smaller than 100 au, strongly suggesting that the presence of a close-in companion star has an adverse effect on planet formation. It is indeed possible for the gravitational pull of the second star to affect all the different stages of planet form
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Kawai, Toshio. "Pattern Formation by Inelastic Collisions, Especially in Planetary Systems." International Journal of Modern Physics B 12, no. 03 (1998): 309–60. http://dx.doi.org/10.1142/s0217979298000247.

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The Titius–Bode law governs the planet distribution in our Solar system. In this paper a possible explanation is proposed based on inelastic collision effects among planetessimals during the evolution of the Solar system. The main purpose of this paper is, however, to introduce a strategy to study phenomena driven by rare but drastic events such as colllisions in the planetary problem. Many complex systems evolve through rare but violent events, so that an efficient strategy to simulate such systems is desirable. An event-driven strategy is proposed in this article, and is used to produce many
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Дисертації з теми "Formation and evolution of planetary systems"

1

Inamdar, Niraj K. "The formation and evolution of planetary systems." Thesis, Massachusetts Institute of Technology, 2016. http://hdl.handle.net/1721.1/107104.

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Thesis: Ph. D. in Planetary Science, Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences, 2016.<br>Cataloged from PDF version of thesis.<br>Includes bibliographical references (pages 299-311).<br>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
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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.

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Hands, 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.

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Of the myriad of insights into exoplanetary systems provided by the Kepler mission, one of the most intriguing new discoveries is that of a class of compact planetary systems which include Kepler-11, Kepler-32 and Kepler-90. In such systems, ensembles of several planets are found in very closely packed orbits (often within a few percent of an astronomical unit of one another). These systems present a challenge for traditional formation and migration scenarios, since these planets presumably formed at larger orbital radii before migrating inwards. In particular, it is difficult to understand ho
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Davies, 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.

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Stars form via the gravitational collapse of molecular clouds during which time the protostellar object contracts by over seven orders of magnitude. If all the angular momentum present in the natal cloud was conserved during collapse, stars would approach rotational velocities rapid enough to tear themselves apart within just a few Myr. In contrast to this, observations of pre-main sequence rotation rates are relatively slow (∼ 1 − 15 days) indicating that significant quantities of angular momentum must be removed from the star. I use observations of fully convective pre-main sequence stars in
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5

Meng, Huan Y. A., George H. Rieke, Kate Y. L. Su, and 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.

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We characterize the first 40 Myr of evolution of circumstellar disks through a unified study of the infrared properties of members of young clusters and associations with ages from 2 Myr up to similar to 40 Myr: NGC 1333, NGC 1960, NGC 2232, NGC 2244, NGC 2362, NGC 2547, IC 348, IC 2395, IC 4665, Chamaeleon I, Orion OB1a and OB1b, Taurus, the beta Pictoris Moving Group,. Ophiuchi, and the associations of Argus, Carina, Columba, Scorpius-Centaurus, and Tucana-Horologium. Our work features: (1) a filtering technique to flag noisy backgrounds; (2) a method based on the probability distribution of
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Trilling, 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.

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The recent discoveries of extrasolar giant planets (planets like Jupiter orbiting other stars like our Sun) at small distances from their central stars have revitalized the fields of planet and planetary system formation. The discoveries have overturned the former paradigm for planetary system formation which suggested that all planetary systems would look like our Solar System: these decidedly do not. The new view is that the early solar system was not nearly the quiescent place previously thought, but rather a dynamic environment in which planets are both easily created and easily destroyed.
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Ngo, Henry, Heather A. Knutson, Sasha Hinkley, 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.

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Stellar companions can influence the formation and evolution of planetary systems, but there are currently few observational constraints on the properties of planet-hosting binary star systems. We search for stellar companions around 77 transiting hot Jupiter systems to explore the statistical properties of this population of companions as compared to field stars of similar spectral type. After correcting for survey incompleteness, we find that 47% +/- 7% of hot Jupiter systems have stellar companions with semimajor axes between 50 and 2000 au. This is 2.9 times larger than the field star comp
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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.

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La détection des premières exoplanètes dans les années 1990 a ouvert une nouvelle ère dans l'étude des planètes. Aujourd'hui, grâce aux instruments toujours plus performants, plusieurs centaines d'exoplanètes (Jupiters chauds, Super-Terre, systèmes multiples...) sont découvertes chaque année. Grâce à cette grande variété d'exoplanètes, il est possible d'étudier la distribution (distance, masse, excentricité...) de ces objets afin de mieux contraindre les modèles de formation et d'évolution des systèmes planétaires. Néanmoins, chaque méthode de détection a ses limites et ses biais de détection.
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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.

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Bonsor, 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.

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Книги з теми "Formation and evolution of planetary systems"

1

Burke, Bernard F., Jürgen H. Rahe, and Elizabeth E. Roettger, eds. Planetary Systems: Formation, Evolution, and Detection. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6.

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1953-, Weaver Harold A., Danly L, and 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 University Press, 1989.

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3

N, Kylafis, and Lada Charles J, eds. The Origin of stars and planetary systems. Kluwer Academic, 1999.

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4

J, Lada Charles, Kylafis N, and 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. Kluwer Academic Publishers, 1999.

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5

United 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. National Aeronautics and Space Administration, 1997.

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6

1928-, Burke Bernard F., Rahe Jürgen H. Rahe, and 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. Kluwer Academic, 1994.

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7

Alessandro, Sozzetti, Lattanzi Mario G, Boss Alan 1951-, and 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 University Press, 2011.

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8

Packevich, Alla. Architecture of Evolution. INFRA-M Academic Publishing LLC., 2021. http://dx.doi.org/10.12737/1079356.

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The monograph, on the one hand, examines the period of development of the descending cycle of evolution and the associated progressive changes that show the irreversibility of the processes of formation of the planetary system. The end of one cycle and the beginning of another leads to the transformation of the system of life and the expansion of consciousness at a new energy level. On the other hand, the questions of potential opportunities for the development of the ascending phase of evolution, which goes both along the path of complexity of the organization and along the path of diversity,
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Alan, 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. Published on behalf of the IAU by Astronomical Society of the Pacific, 2004.

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10

Dvorak, R., and J. Henrard, eds. Long Term Evolution of Planetary Systems. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2285-3.

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Частини книг з теми "Formation and evolution of planetary systems"

1

Bonsor, Amy, and Siyi Xu. "White Dwarf Planetary Systems: Insights Regarding the Fate of Planetary Systems." In Formation, Evolution, and Dynamics of Young Solar Systems. Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-60609-5_8.

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Safronov, V. S., and E. L. Ruskol. "Formation and Evolution of Planets." In Planetary Systems: Formation, Evolution, and Detection. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6_2.

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Fierro, J. "Interaction of Planetary Nebulae with Prenebulae Debris." In Planetary Systems: Formation, Evolution, and Detection. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6_8.

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4

Cruikshank, D. P., M. W. Werner, and D. E. Backman. "SIRTF: Capabilities for the Study of Planetary Systems." In Planetary Systems: Formation, Evolution, and Detection. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6_42.

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Donn, Bertram, and J. Mark Duva. "Formation and Properties of Fluffy Planetesimals." In Planetary Systems: Formation, Evolution, and Detection. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6_5.

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Wetherill, George W. "Possible Consequences of Absence of “Jupiters“ in Planetary Systems." In Planetary Systems: Formation, Evolution, and Detection. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6_3.

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Sargent, A. I., and S. V. W. Beckwith. "The Detection and Study of Pre-Planetary Disks." In Planetary Systems: Formation, Evolution, and Detection. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6_20.

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Owen, T. "The Search for Other Planets: Clues from the Solar System." In Planetary Systems: Formation, Evolution, and Detection. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6_1.

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Peale, S. J. "On the Detection of Mutual Perturbations as Proof of Planets Around PSR1257+12." In Planetary Systems: Formation, Evolution, and Detection. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6_10.

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Phillips, J. A., and S. E. Thorsett. "Planets Around Pulsars: A Review." In Planetary Systems: Formation, Evolution, and Detection. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6_11.

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Тези доповідей конференцій з теми "Formation and evolution of planetary systems"

1

Jiao, Hongying, Miaohua Liu, and Lei Ao. "Azimuth-only Passive Location of UAV Formation Based on Differential Evolution Algorithm." In 2024 International Conference on Interactive Intelligent Systems and Techniques (IIST). IEEE, 2024. http://dx.doi.org/10.1109/iist62526.2024.00103.

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Grady, C. A., Michael E. Van Steenberg, George Sonneborn, H. Warren Moos, and 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.

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Marov, M. Ya, and 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.

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The modern view of planets goes far beyond the usual concept of the planets as bodies of the Solar system. The discovery ofexoplanets has immeasurably expanded the understanding of the architecture and properties of planetary systems. Majoradvances have been made in the study of the planets and minor bodies of the Solar system. However, no answers havebeen received to fundamental questions about the causes of various paths of evolution and formation of planetary naturalcomplexes. To give answers to these questions, research on exoplanets is called upon, of which more than 5000 have beendiscove
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Otsuka, M., H. Izumiura, A. Tajitsu, 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.

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Abdulmyanov, 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.

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The mechanisms of fragmentation of the equatorial dust disk around young stars and the formation of planetary systemsare considered. Using the model of librational motions of co-orbital asteroids of Jupiter, a model of viscous motion of gas,dust particles and small bodies in dust disks is constructed. The dynamic viscosity is obtained from the Navier-Stokesequation for three cases of characteristic flow orbits.It is shown that the librational orbits of Trojans at the early stages ofthe evolution of planetary systems could be transit orbits for dust particles during the formation of celestial bo
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Nath, Arushi. "Algorithms to Determine Asteroid’s Physical Properties using Sparse and Dense Photometry, Robotic Telescopes and Open Data." In Python in Science Conference. SciPy, 2024. http://dx.doi.org/10.25080/twcf2755.

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The rapid pace of discovering asteroids due to advancements in detection techniques outpaces current abilities to analyze them comprehensively. Understanding an asteroid’s physical properties is crucial for effective deflection strategies and improves our understanding of the solar system’s formation and evolution. Dense photometry provides continuous time-series measurements valuable for determining an asteroid’s rotation period, yet is limited to a singular phase angle. Conversely, sparse photometry offers non-continuous measurements across multiple phase angles, essential for determining an
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Athanassoula, 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.

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Chiappini, 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.

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Savage, Paul, and Frédéric Moynier. "Planetary formation and evolution through the lens of zinc and copper isotopes." In Goldschmidt2023. European Association of Geochemistry, 2023. http://dx.doi.org/10.7185/gold2023.20371.

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Rein, Hanno, John C. B. Papaloizou, Tomonori Usuda, Motohide Tamura, and 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.

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Звіти організацій з теми "Formation and evolution of planetary systems"

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O’Dea, Annika, and Katherine Brodie. Analysis of beach cusp formation and evolution using high‐frequency 3D lidar scans. Engineer Research and Development Center (U.S.), 2024. http://dx.doi.org/10.21079/11681/48781.

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Анотація:
Beach cusp characteristics were explored using 15 months of 3D lidar scans collected hourly at the Duck, NC, Field Research Facility. Fourier analyses performed on lidar-derived beach elevation contours generated spatial cusp spectra. Active cusp events identified from the location and magnitude of each spectrum’s peak were used to evaluate conditions during cusp formation and evolution. Cusps primarily developed during normally-incident, long-period, low-energy wave conditions with low frequency spread and reflective beach conditions. Often, however, persistent upper-beach cusps lasted days t
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