De Platão à Kepler: um recorte sobre o movimento dos planetas no sistema solar
Autor(a) principal: | |
---|---|
Data de Publicação: | 2023 |
Tipo de documento: | Dissertação |
Idioma: | por |
Título da fonte: | Biblioteca Digital de Teses e Dissertações da UEFS |
Texto Completo: | http://tede2.uefs.br:8080/handle/tede/1605 |
Resumo: | The continuous observation of nature makes it possible to build assumptions based on what the senses tell us. Thus, for an observer located anywhere on Earth, the perception that the sky is rotating is quite natural. There is no immediate reason to assume that the Earth is moving. For ancient astronomers, the Earth was huge, stable, immobile and occupied the center of the majestic Universe. In the fourth century BC, the fertile thought of Greek philosophers began to foster a new perception of this Universe. Plato (c. 427-347 BC), considered one of the greatest thinkers of the time, sought an explanation for the cyclical variations observed in the sky, in such a way that he formulated the following problem to his disciples: the stars, eternal, divine and immutable stars , describe perfect, circular trajectories, with uniform speeds around the Earth. However, other celestial bodies, such as the Sun, the Moon and the planets, present complicated trajectories, even, in the case of the planets, describing retrograde movements. So how do you explain these peculiar movements in the sky? In the History of Astronomy, we can assure you that the problem presented by Plato was the starting point that triggered the search for understanding the Universe known until then, sowing theoretical models that were confronted with observational records subject to various errors, carried out until then without the aid of luxury of an optical instrument. What importance did the theories then developed, Geocentric and Heliocentric, have for the History of Science? How are these subjects dealt with in textbooks in the light of the Common National Curriculum Base? From the realization that there is still a great lack of information about ‘Plato’s Problem’ and the associated scientific developments, we propose the construction of the following Educational Technical Products (PTE): (1) Pedagogical Workshop, (2) Scientific Article and (3) Hands-on activity based on the application “Planetary Orbits Simulator from NAAP Labs”. |
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Poppe, Paulo César da Rocha926229257-00http://lattes.cnpq.br/3206145669430720056998654-12http://lattes.cnpq.br/0670669856936807Santos, Maria Amanda Guimarães2023-12-20T17:56:02Z2023-08-11SANTOS, Maria Amanda Guimarães. De Platão à Kepler: um recorte sobre o movimento dos planetas no sistema solar, 2023, 104 f., Dissertação (Mestrado Profissional) - Programa de Pós-Graduação em Astronomia, Universidade Estadual de Feira de Santana, Feira de Santana.http://tede2.uefs.br:8080/handle/tede/1605The continuous observation of nature makes it possible to build assumptions based on what the senses tell us. Thus, for an observer located anywhere on Earth, the perception that the sky is rotating is quite natural. There is no immediate reason to assume that the Earth is moving. For ancient astronomers, the Earth was huge, stable, immobile and occupied the center of the majestic Universe. In the fourth century BC, the fertile thought of Greek philosophers began to foster a new perception of this Universe. Plato (c. 427-347 BC), considered one of the greatest thinkers of the time, sought an explanation for the cyclical variations observed in the sky, in such a way that he formulated the following problem to his disciples: the stars, eternal, divine and immutable stars , describe perfect, circular trajectories, with uniform speeds around the Earth. However, other celestial bodies, such as the Sun, the Moon and the planets, present complicated trajectories, even, in the case of the planets, describing retrograde movements. So how do you explain these peculiar movements in the sky? In the History of Astronomy, we can assure you that the problem presented by Plato was the starting point that triggered the search for understanding the Universe known until then, sowing theoretical models that were confronted with observational records subject to various errors, carried out until then without the aid of luxury of an optical instrument. What importance did the theories then developed, Geocentric and Heliocentric, have for the History of Science? How are these subjects dealt with in textbooks in the light of the Common National Curriculum Base? From the realization that there is still a great lack of information about ‘Plato’s Problem’ and the associated scientific developments, we propose the construction of the following Educational Technical Products (PTE): (1) Pedagogical Workshop, (2) Scientific Article and (3) Hands-on activity based on the application “Planetary Orbits Simulator from NAAP Labs”.A observação contínua da natureza possibilita a construção de suposições a partir do que os sentidos nos dizem. Assim, para um observador situado em qual- quer lugar da Terra, a percepção de que o céu está girando é bastante natural. Não há uma imediata razão para supor que a Terra está se movendo. Para os astrônomos da Antiguidade, a Terra era enorme, estável, imóvel e ocupava o centro do majestoso Universo. No século IV a.C., o fértil pensamento dos filósofos gregos começa a fomentar uma nova percepção para este Universo. Platão (c. 427-347 a.C.), considerado um dos maiores pensadores da época, buscava uma explicação para as variações cíclicas observadas no céu, de tal modo que formulou o seguinte problema aos seus discípulos: as estrelas, astros eternos, divinos e imutáveis, descrevem trajetórias perfeitas, circulares, com velocidades uniformes em torno da Terra. No entanto, outros corpos celestes, como o Sol, a Lua e os planetas, apresentam traje- tórias complicadas, chegando mesmo, no caso dos planetas, a descrever movimentos retrógrados. Então, como explicar esses peculiares movimentos no céu? Na História da Astronomia, podemos assegurar que o problema apresentado por Platão foi o marco inicial que desencadeou a busca pela compreensão do Universo até então conhecido, semeando modelos teóricos que eram confrontados com os registros observacionais sujeitos a vários erros, realizados até então sem o auxílio luxuoso de um instrumento óptico. Que importância teve as teorias então desenvolvidas, Geocêntrica e Heliocêntrica, para a História da Ciência? Como estes assuntos são tratados nos livros didáticos à luz da Base Nacional Comum Curricular? A partir da constatação de que ainda existe uma grande carência de informações sobre o ‘Problema de Platão’ e os desdobramentos científicos associados, propomos a construção dos seguintes Produtos Técnicos Educacionais (PTE): (1) Oficina Pedagógica, (2) Artigo Científico e (3) Atividade Prática baseada no aplicativo “Simulador de Órbitas Planetárias do NAAP Labs”.Submitted by Daniela Costa (dmscosta@uefs.br) on 2023-12-20T17:56:02Z No. of bitstreams: 1 Maria Amanda Guimarães Santos - Dissertação.pdf: 4086258 bytes, checksum: b4c23d73e513e392dbc5c6b9e4803d93 (MD5)Made available in DSpace on 2023-12-20T17:56:02Z (GMT). No. of bitstreams: 1 Maria Amanda Guimarães Santos - Dissertação.pdf: 4086258 bytes, checksum: b4c23d73e513e392dbc5c6b9e4803d93 (MD5) Previous issue date: 2023-08-11application/pdfporUniversidade Estadual de Feira de SantanaMestrado Profissional em AstronomiaUEFSBrasilDEPARTAMENTO DE FÍSICAHistória da AstronomiaMovimento PlanetárioGeocentrismoHe- liocentrismoGeocentrismHeliocentrismPlanetary MotionASTRONOMIA::ASTROFISICA DO SISTEMA SOLARDe Platão à Kepler: um recorte sobre o movimento dos planetas no sistema solarinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/masterThesis-388142371651011665660060060031049134849372818771329586728058034802info:eu-repo/semantics/openAccessreponame:Biblioteca Digital de Teses e Dissertações da UEFSinstname:Universidade Estadual de Feira de Santana (UEFS)instacron:UEFSORIGINALMaria Amanda Guimarães Santos - Dissertação.pdfMaria Amanda Guimarães Santos - Dissertação.pdfapplication/pdf4086258http://tede2.uefs.br:8080/bitstream/tede/1605/2/Maria+Amanda+Guimar%C3%A3es+Santos+-+Disserta%C3%A7%C3%A3o.pdfb4c23d73e513e392dbc5c6b9e4803d93MD52LICENSElicense.txtlicense.txttext/plain; charset=utf-82165http://tede2.uefs.br:8080/bitstream/tede/1605/1/license.txtbd3efa91386c1718a7f26a329fdcb468MD51tede/16052023-12-20 14:56:02.124oai:tede2.uefs.br:8080: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Biblioteca Digital de Teses e Dissertaçõeshttp://tede2.uefs.br:8080/PUBhttp://tede2.uefs.br:8080/oai/requestbcuefs@uefs.br|| bcref@uefs.br||bcuefs@uefs.bropendoar:2023-12-20T17:56:02Biblioteca Digital de Teses e Dissertações da UEFS - Universidade Estadual de Feira de Santana (UEFS)false |
dc.title.por.fl_str_mv |
De Platão à Kepler: um recorte sobre o movimento dos planetas no sistema solar |
title |
De Platão à Kepler: um recorte sobre o movimento dos planetas no sistema solar |
spellingShingle |
De Platão à Kepler: um recorte sobre o movimento dos planetas no sistema solar Santos, Maria Amanda Guimarães História da Astronomia Movimento Planetário Geocentrismo He- liocentrismo Geocentrism Heliocentrism Planetary Motion ASTRONOMIA::ASTROFISICA DO SISTEMA SOLAR |
title_short |
De Platão à Kepler: um recorte sobre o movimento dos planetas no sistema solar |
title_full |
De Platão à Kepler: um recorte sobre o movimento dos planetas no sistema solar |
title_fullStr |
De Platão à Kepler: um recorte sobre o movimento dos planetas no sistema solar |
title_full_unstemmed |
De Platão à Kepler: um recorte sobre o movimento dos planetas no sistema solar |
title_sort |
De Platão à Kepler: um recorte sobre o movimento dos planetas no sistema solar |
author |
Santos, Maria Amanda Guimarães |
author_facet |
Santos, Maria Amanda Guimarães |
author_role |
author |
dc.contributor.advisor1.fl_str_mv |
Poppe, Paulo César da Rocha |
dc.contributor.advisor1ID.fl_str_mv |
926229257-00 |
dc.contributor.advisor1Lattes.fl_str_mv |
http://lattes.cnpq.br/3206145669430720 |
dc.contributor.authorID.fl_str_mv |
056998654-12 |
dc.contributor.authorLattes.fl_str_mv |
http://lattes.cnpq.br/0670669856936807 |
dc.contributor.author.fl_str_mv |
Santos, Maria Amanda Guimarães |
contributor_str_mv |
Poppe, Paulo César da Rocha |
dc.subject.por.fl_str_mv |
História da Astronomia Movimento Planetário Geocentrismo He- liocentrismo Geocentrism Heliocentrism |
topic |
História da Astronomia Movimento Planetário Geocentrismo He- liocentrismo Geocentrism Heliocentrism Planetary Motion ASTRONOMIA::ASTROFISICA DO SISTEMA SOLAR |
dc.subject.eng.fl_str_mv |
Planetary Motion |
dc.subject.cnpq.fl_str_mv |
ASTRONOMIA::ASTROFISICA DO SISTEMA SOLAR |
description |
The continuous observation of nature makes it possible to build assumptions based on what the senses tell us. Thus, for an observer located anywhere on Earth, the perception that the sky is rotating is quite natural. There is no immediate reason to assume that the Earth is moving. For ancient astronomers, the Earth was huge, stable, immobile and occupied the center of the majestic Universe. In the fourth century BC, the fertile thought of Greek philosophers began to foster a new perception of this Universe. Plato (c. 427-347 BC), considered one of the greatest thinkers of the time, sought an explanation for the cyclical variations observed in the sky, in such a way that he formulated the following problem to his disciples: the stars, eternal, divine and immutable stars , describe perfect, circular trajectories, with uniform speeds around the Earth. However, other celestial bodies, such as the Sun, the Moon and the planets, present complicated trajectories, even, in the case of the planets, describing retrograde movements. So how do you explain these peculiar movements in the sky? In the History of Astronomy, we can assure you that the problem presented by Plato was the starting point that triggered the search for understanding the Universe known until then, sowing theoretical models that were confronted with observational records subject to various errors, carried out until then without the aid of luxury of an optical instrument. What importance did the theories then developed, Geocentric and Heliocentric, have for the History of Science? How are these subjects dealt with in textbooks in the light of the Common National Curriculum Base? From the realization that there is still a great lack of information about ‘Plato’s Problem’ and the associated scientific developments, we propose the construction of the following Educational Technical Products (PTE): (1) Pedagogical Workshop, (2) Scientific Article and (3) Hands-on activity based on the application “Planetary Orbits Simulator from NAAP Labs”. |
publishDate |
2023 |
dc.date.accessioned.fl_str_mv |
2023-12-20T17:56:02Z |
dc.date.issued.fl_str_mv |
2023-08-11 |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/masterThesis |
format |
masterThesis |
status_str |
publishedVersion |
dc.identifier.citation.fl_str_mv |
SANTOS, Maria Amanda Guimarães. De Platão à Kepler: um recorte sobre o movimento dos planetas no sistema solar, 2023, 104 f., Dissertação (Mestrado Profissional) - Programa de Pós-Graduação em Astronomia, Universidade Estadual de Feira de Santana, Feira de Santana. |
dc.identifier.uri.fl_str_mv |
http://tede2.uefs.br:8080/handle/tede/1605 |
identifier_str_mv |
SANTOS, Maria Amanda Guimarães. De Platão à Kepler: um recorte sobre o movimento dos planetas no sistema solar, 2023, 104 f., Dissertação (Mestrado Profissional) - Programa de Pós-Graduação em Astronomia, Universidade Estadual de Feira de Santana, Feira de Santana. |
url |
http://tede2.uefs.br:8080/handle/tede/1605 |
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por |
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por |
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600 600 600 |
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1329586728058034802 |
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openAccess |
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Universidade Estadual de Feira de Santana |
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Mestrado Profissional em Astronomia |
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UEFS |
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Universidade Estadual de Feira de Santana |
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