De Plat?o ? Kepler: um recorte sobre o movimento dos planetas no sistema solar

Detalhes bibliográficos
Ano de defesa: 2023
Autor(a) principal: Santos, Maria Amanda Guimar?es lattes
Orientador(a): Poppe, Paulo C?sar da Rocha lattes
Banca de defesa: Não Informado pela instituição
Tipo de documento: Dissertação
Tipo de acesso: Acesso aberto
Idioma: por
Instituição de defesa: Universidade Estadual de Feira de Santana
Programa de Pós-Graduação: Mestrado Profissional em Astronomia
Departamento: DEPARTAMENTO DE F?SICA
País: Brasil
Palavras-chave em Português:
Palavras-chave em Inglês:
Área do conhecimento CNPq:
Link de acesso: 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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spelling Poppe, Paulo C?sar da Rocha926229257-00http://lattes.cnpq.br/3206145669430720056998654-12http://lattes.cnpq.br/0670669856936807Santos, Maria Amanda Guimar?es2023-12-20T17:56:02Z2023-08-11SANTOS, Maria Amanda Guimar?es. De Plat?o ? Kepler: um recorte sobre o movimento dos planetas no sistema solar, 2023, 104 f., Disserta??o (Mestrado Profissional) - Programa de P?s-Gradua??o 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 observa??o cont?nua da natureza possibilita a constru??o de suposi??es a partir do que os sentidos nos dizem. Assim, para um observador situado em qual- quer lugar da Terra, a percep??o de que o c?u est? girando ? bastante natural. N?o h? uma imediata raz?o para supor que a Terra est? se movendo. Para os astr?nomos da Antiguidade, a Terra era enorme, est?vel, im?vel e ocupava o centro do majestoso Universo. No s?culo IV a.C., o f?rtil pensamento dos fil?sofos gregos come?a a fomentar uma nova percep??o para este Universo. Plat?o (c. 427-347 a.C.), considerado um dos maiores pensadores da ?poca, buscava uma explica??o para as varia??es c?clicas observadas no c?u, de tal modo que formulou o seguinte problema aos seus disc?pulos: as estrelas, astros eternos, divinos e imut?veis, descrevem trajet?rias perfeitas, circulares, com velocidades uniformes em torno da Terra. No entanto, outros corpos celestes, como o Sol, a Lua e os planetas, apresentam traje- t?rias complicadas, chegando mesmo, no caso dos planetas, a descrever movimentos retr?grados. Ent?o, como explicar esses peculiares movimentos no c?u? Na Hist?ria da Astronomia, podemos assegurar que o problema apresentado por Plat?o foi o marco inicial que desencadeou a busca pela compreens?o do Universo at? ent?o conhecido, semeando modelos te?ricos que eram confrontados com os registros observacionais sujeitos a v?rios erros, realizados at? ent?o sem o aux?lio luxuoso de um instrumento ?ptico. Que import?ncia teve as teorias ent?o desenvolvidas, Geoc?ntrica e Helioc?ntrica, para a Hist?ria da Ci?ncia? Como estes assuntos s?o tratados nos livros did?ticos ? luz da Base Nacional Comum Curricular? A partir da constata??o de que ainda existe uma grande car?ncia de informa??es sobre o ?Problema de Plat?o? e os desdobramentos cient?ficos associados, propomos a constru??o dos seguintes Produtos T?cnicos Educacionais (PTE): (1) Oficina Pedag?gica, (2) Artigo Cient?fico e (3) Atividade Pr?tica baseada no aplicativo ?Simulador de ?rbitas Planet?rias do NAAP Labs?.Submitted by Daniela Costa (dmscosta@uefs.br) on 2023-12-20T17:56:02Z No. of bitstreams: 1 Maria Amanda Guimar?es Santos - Disserta??o.pdf: 4086258 bytes, checksum: b4c23d73e513e392dbc5c6b9e4803d93 (MD5)Made available in DSpace on 2023-12-20T17:56:02Z (GMT). No. of bitstreams: 1 Maria Amanda Guimar?es Santos - Disserta??o.pdf: 4086258 bytes, checksum: b4c23d73e513e392dbc5c6b9e4803d93 (MD5) Previous issue date: 2023-08-11application/pdfhttp://tede2.uefs.br:8080/retrieve/7511/Maria%20Amanda%20Guimar%c3%a3es%20Santos%20-%20Disserta%c3%a7%c3%a3o.pdf.jpgporUniversidade Estadual de Feira de SantanaMestrado Profissional em AstronomiaUEFSBrasilDEPARTAMENTO DE F?SICAHist?ria da AstronomiaMovimento Planet?rioGeocentrismoHe- liocentrismoGeocentrismHeliocentrismPlanetary MotionASTRONOMIA::ASTROFISICA DO SISTEMA SOLARDe Plat?o ? 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dc.title.por.fl_str_mv De Plat?o ? Kepler: um recorte sobre o movimento dos planetas no sistema solar
title De Plat?o ? Kepler: um recorte sobre o movimento dos planetas no sistema solar
spellingShingle De Plat?o ? Kepler: um recorte sobre o movimento dos planetas no sistema solar
Santos, Maria Amanda Guimar?es
Hist?ria da Astronomia
Movimento Planet?rio
Geocentrismo
He- liocentrismo
Geocentrism
Heliocentrism
Planetary Motion
ASTRONOMIA::ASTROFISICA DO SISTEMA SOLAR
title_short De Plat?o ? Kepler: um recorte sobre o movimento dos planetas no sistema solar
title_full De Plat?o ? Kepler: um recorte sobre o movimento dos planetas no sistema solar
title_fullStr De Plat?o ? Kepler: um recorte sobre o movimento dos planetas no sistema solar
title_full_unstemmed De Plat?o ? Kepler: um recorte sobre o movimento dos planetas no sistema solar
title_sort De Plat?o ? Kepler: um recorte sobre o movimento dos planetas no sistema solar
author Santos, Maria Amanda Guimar?es
author_facet Santos, Maria Amanda Guimar?es
author_role author
dc.contributor.advisor1.fl_str_mv Poppe, Paulo C?sar 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 Guimar?es
contributor_str_mv Poppe, Paulo C?sar da Rocha
dc.subject.por.fl_str_mv Hist?ria da Astronomia
Movimento Planet?rio
Geocentrismo
He- liocentrismo
Geocentrism
Heliocentrism
topic Hist?ria da Astronomia
Movimento Planet?rio
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
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dc.identifier.citation.fl_str_mv SANTOS, Maria Amanda Guimar?es. De Plat?o ? Kepler: um recorte sobre o movimento dos planetas no sistema solar, 2023, 104 f., Disserta??o (Mestrado Profissional) - Programa de P?s-Gradua??o 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 Guimar?es. De Plat?o ? Kepler: um recorte sobre o movimento dos planetas no sistema solar, 2023, 104 f., Disserta??o (Mestrado Profissional) - Programa de P?s-Gradua??o em Astronomia, Universidade Estadual de Feira de Santana, Feira de Santana.
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