Modelo estadístico para la distribución de materia en discos protoplanetarios
1 recurso en línea (xiii, 71 páginas) : ilustraciones, figuras, tablas.
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| Other Authors: | |
| Format: | Trabajo de grado - Maestría |
| Language: | spa |
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Universidad Pedagógica y Tecnológica de Colombia
2019
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| Online Access: | http://repositorio.uptc.edu.co/handle/001/2484 |
| _version_ | 1801705854483824640 |
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| author | Buitrago Carreño, Nidia Yiseth |
| author2 | Poveda Tejada, Nicanor |
| author_facet | Poveda Tejada, Nicanor Buitrago Carreño, Nidia Yiseth |
| author_sort | Buitrago Carreño, Nidia Yiseth |
| collection | DSpace |
| description | 1 recurso en línea (xiii, 71 páginas) : ilustraciones, figuras, tablas. |
| format | Trabajo de grado - Maestría |
| id | repositorio.uptc.edu.co-001-2484 |
| institution | Repositorio Institucional UPTC |
| language | spa |
| publishDate | 2019 |
| publisher | Universidad Pedagógica y Tecnológica de Colombia |
| record_format | dspace |
| spelling | repositorio.uptc.edu.co-001-24842023-04-10T16:25:04Z Modelo estadístico para la distribución de materia en discos protoplanetarios Buitrago Carreño, Nidia Yiseth Poveda Tejada, Nicanor Astrogeología Astrofísica Materia interestelar Polvo cósmico Maestría en Ciencias-Física - Tesis y disertaciones académicas 1 recurso en línea (xiii, 71 páginas) : ilustraciones, figuras, tablas. The planetary systems have their origin in the gravitational collapse of a cloud of gas and dust. Through an accretion process a massive star and a disk of planetesimals are formed orbiting the star. Through statistical considerations a model is obtained which allows to describe the distribution of matter of the star-planetesimal system. The parameters of the model for the solar system, satellites, exoplanets and the HL-Tauri system are determined. It is shown that the radius, eccentricity, energy, angular momentum and orbital inclination of the planetary objects formed take discrete values, depending only on the value of the mass of the star. Unlike other models, the formation of planetary objects is faster. Los sistemas planetarios tienen su origen en el colapso gravitacional de una nube de gas y polvo. Mediante un proceso de acreción se forma una estrella masiva y un disco de planetesimales orbitando la estrella. Mediante consideraciones estadísticas se obtiene un modelo el cual permite describir la distribución de materia del sistema estrella-planetesimales. Se determinan los parámetros del modelo para el Sistema Solar, satélites, exoplanetas y el sistema HL-Tauri. Se demuestra que el radio, excentricidad, energía, momentum angular e inclinación orbital, de los objetos planetarios formados toman valores discretos, dependiendo solamente del valor de la masa de la estrella. A diferencia de otros modelos, la formación de objetos planetarios es más rápida. Bibliografía y webgrafía: páginas 61-65. Maestría Magíster en Ciencias - Física 2019-03-20T19:51:42Z 2019-03-20T19:51:42Z 2018 Trabajo de grado - Maestría http://purl.org/coar/resource_type/c_bdcc info:eu-repo/semantics/masterThesis info:eu-repo/semantics/publishedVersion Text https://purl.org/redcol/resource_type/TM http://purl.org/coar/version/c_970fb48d4fbd8a85 Buitrago Carreño, N.Y. (2018) .Modelo estadístico para la distribución de materia en discos protoplanetarios. (Tesis de maestría). Universidad Pedagógica y Tecnológica de Colombia, Tunja. http://repositorio.uptc.edu.co/handle/001/2484 http://repositorio.uptc.edu.co/handle/001/2484 spa R. L. Akeson, X. Chen, D. Ciardi, M. Crane, J. Good, M. Harbut, E. Jackson, S. R. Kane, A. C. Laity, S. Leifer, M. Lynn, D. L. McElroy, M. Papin, P. Plavchan, S. V. Ramírez, R. Rey, K. von Braun, M. Wittman, M. Abajian, B. Ali, C. Beichman, A. Beekley, G. B. 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Copyright (c) 2018 Universidad Pedagógica y Tecnológica de Colombia https://creativecommons.org/licenses/by-nc-sa/4.0/ info:eu-repo/semantics/openAccess Atribución-NoComercial-CompartirIgual 4.0 Internacional (CC BY-NC-SA 4.0) http://purl.org/coar/access_right/c_abf2 application/pdf application/pdf application/pdf Universidad Pedagógica y Tecnológica de Colombia Facultad de Ciencias. Maestría en Ciencias - Física |
| spellingShingle | Astrogeología Astrofísica Materia interestelar Polvo cósmico Maestría en Ciencias-Física - Tesis y disertaciones académicas Buitrago Carreño, Nidia Yiseth Modelo estadístico para la distribución de materia en discos protoplanetarios |
| title | Modelo estadístico para la distribución de materia en discos protoplanetarios |
| title_full | Modelo estadístico para la distribución de materia en discos protoplanetarios |
| title_fullStr | Modelo estadístico para la distribución de materia en discos protoplanetarios |
| title_full_unstemmed | Modelo estadístico para la distribución de materia en discos protoplanetarios |
| title_short | Modelo estadístico para la distribución de materia en discos protoplanetarios |
| title_sort | modelo estadistico para la distribucion de materia en discos protoplanetarios |
| topic | Astrogeología Astrofísica Materia interestelar Polvo cósmico Maestría en Ciencias-Física - Tesis y disertaciones académicas |
| url | http://repositorio.uptc.edu.co/handle/001/2484 |
| work_keys_str_mv | AT buitragocarrenonidiayiseth modeloestadisticoparaladistribuciondemateriaendiscosprotoplanetarios |
