ETDs @PUC-Rio
| Título: | TENSIONS GENERATED BY SELF-INDUCED GRAVITATIONAL ACTION ON A SOLID SPHERE: APPLICATIONS TO STUDY THE DISTRIBUTION OF DENSITY AND ELASTICITY OF THE PLANETS | ||||||||||||
| Autor: |
CARLOS FERNANDO MARTINS PAMPLONA |
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| Colaborador(es): |
SIDNEY STUCKENBRUCK - Orientador |
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| Catalogação: | 27/MAR/2019 | Língua(s): | PORTUGUESE - BRAZIL |
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| Tipo: | TEXT | Subtipo: | THESIS | ||||||||||
| Notas: |
[pt] Todos os dados constantes dos documentos são de inteira responsabilidade de seus autores. Os dados utilizados nas descrições dos documentos estão em conformidade com os sistemas da administração da PUC-Rio. [en] All data contained in the documents are the sole responsibility of the authors. The data used in the descriptions of the documents are in conformity with the systems of the administration of PUC-Rio. |
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| Referência(s): |
[pt] https://www.maxwell.vrac.puc-rio.br/projetosEspeciais/ETDs/consultas/conteudo.php?strSecao=resultado&nrSeq=37501&idi=1 [en] https://www.maxwell.vrac.puc-rio.br/projetosEspeciais/ETDs/consultas/conteudo.php?strSecao=resultado&nrSeq=37501&idi=2 |
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| DOI: | https://doi.org/10.17771/PUCRio.acad.37501 | ||||||||||||
| Resumo: | |||||||||||||
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In the present work an analysis of the density distribution in large spherical bodies is made based on the stresses generated by gravitational action. Is is found that an eliptical expression for the radial density distribution in the form of the equation p=po[1-a(r/R)(2)](1/2) give reasonable results for the mechanical properties of earth interior. Starting with this assumption, several models for density distribution for terrestrial planets and earth s moon are analysed and proposed, based on the assumption of similiarity of core materials of these bodies. The value of moment of inertia as well as the diameter of the core of the inner planets of the solar system are estimated from those analyses.
The models were developed admiting variable mechanical properties with pressure, as well as discontinuity on the density distribution, and the results compared with seismic data from geodesy and selenodesy. Extension of those results for other terrestrial planets were made in an attempt to obtain new informations about these planets, for wich little is know about its interior.
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