Relevant bibliographies by topics / Edgeworth Kuiper belt

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  2. Dissertations / Theses
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  4. Book chapters

Academic literature on the topic 'Edgeworth Kuiper belt'

Author: Grafiati
Published: 4 June 2021
Last updated: 13 February 2022

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Journal articles on the topic "Edgeworth Kuiper belt"

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Ipatov, S. I. "Evolution of the Edgeworth-Kuiper Belt." Highlights of Astronomy 12 (2002): 247–48. http://dx.doi.org/10.1017/s153929960001340x.

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AbstractDue to gravitational interactions with large trans-neptunian objects (TNOs) several percent of TNOs can change their semimajor axes by more that 1 AU during last 4 Gyr. Now about 30000 1-km former TNOs can be Jupiter crossers and about 20% of Earth-crossing objects can be former TNOs which now move in Jupiter-crossing orbits.
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Yamamoto, T. "Are Edgeworth-Kuiper Belt Objects Pristine?" Science 273, no. 5277 (August 16, 1996): 921–0. http://dx.doi.org/10.1126/science.273.5277.921.

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Hughes, David W. "Quaoar and the Edgeworth-Kuiper belt." Astronomy and Geophysics 44, no. 3 (June 2003): 3.21–3.22. http://dx.doi.org/10.1046/j.1468-4004.2003.44321.x.

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Collander-Brown, S. "The plane of the Edgeworth–Kuiper belt." Icarus 162, no. 1 (March 2003): 22–26. http://dx.doi.org/10.1016/s0019-1035(02)00061-1.

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DAVIS, D., and P. FARINELLA. "Collisional Evolution of Edgeworth–Kuiper Belt Objects☆." Icarus 125, no. 1 (January 1997): 50–60. http://dx.doi.org/10.1006/icar.1996.5595.

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Barucci, M. "Spectrophotometric Observations of Edgeworth–Kuiper Belt Objects." Icarus 142, no. 2 (December 1999): 476–81. http://dx.doi.org/10.1006/icar.1999.6212.

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Doressoundiram, A., N. Peixinho, C. de Bergh, S. Fornasier, P. Thébault, M. A. Barucci, and C. Veillet. "The Color Distribution in the Edgeworth-Kuiper Belt." Astronomical Journal 124, no. 4 (October 2002): 2279–96. http://dx.doi.org/10.1086/342447.

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Fulchignoni, Marcello, and Audrey C. Delsanti. "A statistical insight into the Edgeworth-Kuiper belt." Comptes Rendus Physique 4, no. 7 (September 2003): 767–74. http://dx.doi.org/10.1016/j.crhy.2003.09.013.

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Taidakova, Tanya, Leonid M. Ozernoy, and Nick N. Gorkavyi. "Resonant Gaps in the Scattered Cometary Population of the Trans-Neptunian Region." Highlights of Astronomy 12 (2002): 251–52. http://dx.doi.org/10.1017/s1539299600013423.

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AbstractOur numerical simulations of the Edgeworth-Kuiper Belt objects gravitationally scattered by the four giant planets accounting for mean motion resonances reveal numerous resonant gaps in the distribution of the scattered population.
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Davis, Donald R., and Paolo Farinella. "Collisional Evolution of the Edgeworth-Kuiper Belt: Implications for the Origin and Evolution of Small Body Populations." Highlights of Astronomy 12 (2002): 219–22. http://dx.doi.org/10.1017/s1539299600013307.

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AbstractCollisions have been a major process that shaped the Kuiper Belt that we see today. Collisional grinding likely played a significant role in removing mass from the trans-neptunian region and collisions are a mechanism for injecting fragments into resonances to start their journey to become short period comets. The Kuiper Belt preserves the accretional size distribution in bodies ≳ 100 km while the size distribution of smaller bodies is the result of collisional evolution. Observational confirmation of the transition size between these different regimes will constrain our understanding of the origin and evolution of the Kuiper Belt.
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Dissertations / Theses on the topic "Edgeworth Kuiper belt"

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Fletcher, Edel. "Optical observations of Edgeworth-Kuiper belt objects." Thesis, Queen's University Belfast, 2000. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.322857.

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Maran, Michael David. "Dynamics of bodies on heliocentric orbits in the outer solar system." Thesis, Queen Mary, University of London, 2001. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.251849.

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Gerlach, Enrico. "Stabilitätsuntersuchungen an Asteroidenbahnen in ausgewählten Bahnresonanzen des Edgeworth-Kuiper-Gürtels." Doctoral thesis, Saechsische Landesbibliothek- Staats- und Universitaetsbibliothek Dresden, 2008. http://nbn-resolving.de/urn:nbn:de:bsz:14-ds-1225227803732-58854.

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Gegenstand dieser Dissertation ist eine umfassende Analyse der Stabilität von Asteroidenbahnen im Edgeworth-Kuiper-Gürtel am Beispiel der 3:5-, 4:7- und der 1:2-Bahnresonanz mit Neptun. Einen weiteren Schwerpunkt der Arbeit bildet die Untersuchung der numerischen Berechenbarkeit der Lyapunov-Zeit von Asteroidenbahnen. Ausgehend von einer allgemeinen Beschreibung der bei numerischen Berechnungen auftretenden Rundungs- und Diskretisierungsfehler wird deren Wachstum bei numerischen Integrationen ermittelt. Diese, teilweise maschinenabhängigen, Fehler beeinflussen die berechnete Trajektorie des Asteroiden ebenso wie die daraus abgeleitete Lyapunov-Zeit. Durch Beispielrechnungen mit unterschiedlichen Rechnerarchitekturen und Integrationsmethoden wird der Einfluss auf die erhaltenen Lyapunov-Zeiten eingehend untersucht. Als Maß zur Beschreibung dieser Abhängigkeit wird ein Berechenbarkeitsindex $\kappa$ definiert. Weiterhin wird gezeigt, dass die allgemeine Struktur des Phasenraumes robust gegenüber diesen Änderungen ist. Unter Nutzung dieser Erkenntnis werden anschließend ausgewählte Bahnresonanzen im Edgeworth-Kuiper-Gürtel untersucht. Grundlegende Charakteristika, wie die Resonanzbreiten, werden dabei aus einfachen Modellen abgeleitet. Eine möglichst realitätsnahe Beschreibung der Stabilität wird durch numerische Integration einer Vielzahl von Testkörpern zusammen mit den Planeten Jupiter bis Neptun erreicht. Die erhaltenen Ergebnisse werden dabei mit der beobachteten Verteilung der Asteroiden im Edgeworth-Kuiper-Gürtel verglichen. ---- Hinweis: Beim Betrachten der pdf-Version dieses Dokumentes mit dem Acrobat Reader mit einer Version kleiner 8.0 kann es unter Windows zu Problemen in der Darstellung der Abbildungen auf den Seiten 46, 72, 74, 79 und 86 kommen. Um die Datenpunkte zu sehen ist eine Vergrößerung von mehr als 800% notwendig. Alternativ kann in den Grundeinstellungen der Haken für das Glätten von Vektorgraphiken entfernt werden
This dissertation presents a comprehensive description of the stability of asteroid orbits in the Edgeworth-Kuiper belt taking the 3:5, 4:7 and 1:2 mean motion resonance with Neptune as example. Further emphasis is given to the numerical computability of the Lyapunov time of asteroids. Starting with a general description of rounding and approximation errors in numerical computations, the growth of these errors within numerical integrations is estimated. These, partly machine-dependent errors influence the calculated trajectory of the asteroid as well as the derived Lyapunov time. Different hardware architectures and integration methods were used to investigate the influence on the computed Lyapunov time. As a measure of this dependence a computability index $\kappa$ is defined. Furthermore it is shown, that the general structure of phase space is robust against these changes. Subsequently, several selected mean motion resonances in the Edgeworth-Kuiper belt are investigated using these findings. Basic properties, like the resonance width, are deduced from simple models. To get a realistic description of the stability, a huge number of test particles was numerically integrated together with the planets Jupiter to Neptune. The obtained results are compared to the observed distribution of asteroids in the Edgeworth-Kuiper belt. ---- Additional information: If the pdf-file of this document is viewed using Acrobat Reader with a version less 8.0 under Windows the figures on page 46, 72, 74, 79 and 86 are shown incomplete. To see the data points a zoom factor larger than 800% is necessary. Alternatively the smoothing of vector graphics should be disabled in the settings of the reader
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Vitense, Christian [Verfasser], Alexander V. [Akademischer Betreuer] Krivov, Sebastian [Akademischer Betreuer] Wolf, and Marc [Akademischer Betreuer] Kuchner. "The edgeworth-kuiper belt as a debris disk / Christian Vitense. Gutachter: Alexander V. Krivov ; Sebastian Wolf ; Marc Kuchner." Jena : Thüringer Universitäts- und Landesbibliothek Jena, 2013. http://d-nb.info/1030521808/34.

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Books on the topic "Edgeworth Kuiper belt"

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Davies, John K., and Luis H. Barrera, eds. The First Decadal Review of the Edgeworth-Kuiper Belt. Dordrecht: Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-94-017-3321-2.

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(Editor), John K. Davies, and Luis H. Barrera (Editor), eds. The First Decadal Review of the Edgeworth-Kuiper Belt. Springer, 2004.

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The first decadal review of the Edgeworth-Kuiper Belt. Dordrecht: Kluwer Academic Publishers, 2004.

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Book chapters on the topic "Edgeworth Kuiper belt"

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Davis, Donald R., and Paolo F. Farinella. "Collisional Effects in the Edgeworth-Kuiper Belt." In Collisional Processes in the Solar System, 277–86. Dordrecht: Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-010-0712-2_17.

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Wyatt, Mark C., Wayne S. Holland, Jane S. Greaves, and William R. F. Dent. "Extrasolar Analogues to the Kuiper Belt." In The First Decadal Review of the Edgeworth-Kuiper Belt, 423–34. Dordrecht: Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-94-017-3321-2_36.

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Morbidelli, A., M. E. Brown, and H. F. Levison. "The Kuiper Belt and Its Primordial Sculpting." In The First Decadal Review of the Edgeworth-Kuiper Belt, 1–27. Dordrecht: Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-94-017-3321-2_1.

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Sheppard, Scott S., and David C. Jewitt. "Hawaii Kuiper Belt Variability Project: An Update." In The First Decadal Review of the Edgeworth-Kuiper Belt, 207–19. Dordrecht: Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-94-017-3321-2_19.

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Luu, Jane, and Pedro Lacerda. "The Shape Distribution of Kuiper Belt Objects." In The First Decadal Review of the Edgeworth-Kuiper Belt, 221–32. Dordrecht: Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-94-017-3321-2_20.

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Belskaya, Irina N., Antonella M. Barucci, and Yurij G. Shkuratov. "Opposition Effect of Kuiper Belt Objects: Preliminary Estimations." In The First Decadal Review of the Edgeworth-Kuiper Belt, 201–6. Dordrecht: Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-94-017-3321-2_18.

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Cruikshank, Dale P., and Cristina M. Dalle Ore. "Spectral Models of Kuiper Belt Objects and Centaurs." In The First Decadal Review of the Edgeworth-Kuiper Belt, 315–30. Dordrecht: Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-94-017-3321-2_28.

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Chiang, E. I., J. R. Lovering, R. L. Millis, M. W. Buie, L. H. Wasserman, and K. J. Meech. "Resonant and Secular Families of the Kuiper Belt." In The First Decadal Review of the Edgeworth-Kuiper Belt, 49–62. Dordrecht: Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-94-017-3321-2_4.

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Moody, Rachel, Brian Schmidt, Charles Alcock, Jeffrey Goldader, Tim Axelrod, Kem H. Cook, and Stuart Marshall. "Initial Results from the Southern Edgeworth-Kuiper Belt Survey." In The First Decadal Review of the Edgeworth-Kuiper Belt, 125–30. Dordrecht: Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-94-017-3321-2_11.

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Roques, Françoise. "Research of Small Kuiper Belt Objects by Stellar Occultations." In The First Decadal Review of the Edgeworth-Kuiper Belt, 453–57. Dordrecht: Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-94-017-3321-2_39.

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You might also be interested in the extended bibliographies on the topic 'Edgeworth Kuiper belt' for particular source types:
Journal articles
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