Questões TBG 2023 para Analista Júnior – Ênfase: Gestão, Meio Ambiente

Q2281240

Q2281240 Inglês

Texto associado

Text CB1A2-I

Oppenheimer’s brief advance into astrophysics began with a 1938 paper about neutron stars, which continued in a 1939 installment that further incorporated the principles of Einstein’s general theory of relativity. He then published a third paper on black holes on September 1st, 1939—but at the time, it was scarcely noticed because this was the very day Germany invaded Poland, launching World War II. Oppenheimer never wrote on the topic again.

Even if it hadn’t been overshadowed by war, Oppenheimer’s work on neutron stars and black holes “was not understood to be terribly significant at the time,” says Cathryn Carson, a historian of science at the University of California, Berkeley.

Each paper was written with a different member of the swarm of graduate students that Oppenheimer carefully cultivated. These protégés facilitated his ability to jump between research topics—and ultimately, helped him develop some of his most important contributions to physics.

Oppenheimer’s climactic third paper, written with his student Hartland Snyder, explores the implications of general relativity on the universe’s most massive stars. Although the physicists needed to include some assumptions to simplify the question, they determined that a large enough star would gravitationally collapse indefinitely—and within a finite amount of time, meaning that the objects we now know as black holes could exist.

Internet: <scientificamerican.com> (adapted)

Based on text CB1A2-I, judge the following item.

Oppenheimer’s paper on black holes received little attention at the time it was published.

Certo

Errado

Você errou! Resposta:

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Q2281241

Q2281241 Inglês

Texto associado

Text CB1A2-I

Oppenheimer’s brief advance into astrophysics began with a 1938 paper about neutron stars, which continued in a 1939 installment that further incorporated the principles of Einstein’s general theory of relativity. He then published a third paper on black holes on September 1st, 1939—but at the time, it was scarcely noticed because this was the very day Germany invaded Poland, launching World War II. Oppenheimer never wrote on the topic again.

Even if it hadn’t been overshadowed by war, Oppenheimer’s work on neutron stars and black holes “was not understood to be terribly significant at the time,” says Cathryn Carson, a historian of science at the University of California, Berkeley.

Each paper was written with a different member of the swarm of graduate students that Oppenheimer carefully cultivated. These protégés facilitated his ability to jump between research topics—and ultimately, helped him develop some of his most important contributions to physics.

Oppenheimer’s climactic third paper, written with his student Hartland Snyder, explores the implications of general relativity on the universe’s most massive stars. Although the physicists needed to include some assumptions to simplify the question, they determined that a large enough star would gravitationally collapse indefinitely—and within a finite amount of time, meaning that the objects we now know as black holes could exist.

Internet: <scientificamerican.com> (adapted)

Based on text CB1A2-I, judge the following item.

According to Cathryn Carson, Oppenheimer’s work on neutron stars and black holes was meaningless at the time it was developed.

Certo

Errado

Você errou! Resposta:

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Q2281242

Q2281242 Inglês

Texto associado

Text CB1A2-I

Oppenheimer’s brief advance into astrophysics began with a 1938 paper about neutron stars, which continued in a 1939 installment that further incorporated the principles of Einstein’s general theory of relativity. He then published a third paper on black holes on September 1st, 1939—but at the time, it was scarcely noticed because this was the very day Germany invaded Poland, launching World War II. Oppenheimer never wrote on the topic again.

Even if it hadn’t been overshadowed by war, Oppenheimer’s work on neutron stars and black holes “was not understood to be terribly significant at the time,” says Cathryn Carson, a historian of science at the University of California, Berkeley.

Each paper was written with a different member of the swarm of graduate students that Oppenheimer carefully cultivated. These protégés facilitated his ability to jump between research topics—and ultimately, helped him develop some of his most important contributions to physics.

Oppenheimer’s climactic third paper, written with his student Hartland Snyder, explores the implications of general relativity on the universe’s most massive stars. Although the physicists needed to include some assumptions to simplify the question, they determined that a large enough star would gravitationally collapse indefinitely—and within a finite amount of time, meaning that the objects we now know as black holes could exist.

Internet: <scientificamerican.com> (adapted)

Based on text CB1A2-I, judge the following item.

With the help of his students, Oppenheimer could easily shift from one research topic to another.

Certo

Errado

Você errou! Resposta:

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Q2281243

Q2281243 Inglês

Texto associado

Text CB1A2-I

Oppenheimer’s brief advance into astrophysics began with a 1938 paper about neutron stars, which continued in a 1939 installment that further incorporated the principles of Einstein’s general theory of relativity. He then published a third paper on black holes on September 1st, 1939—but at the time, it was scarcely noticed because this was the very day Germany invaded Poland, launching World War II. Oppenheimer never wrote on the topic again.

Even if it hadn’t been overshadowed by war, Oppenheimer’s work on neutron stars and black holes “was not understood to be terribly significant at the time,” says Cathryn Carson, a historian of science at the University of California, Berkeley.

Each paper was written with a different member of the swarm of graduate students that Oppenheimer carefully cultivated. These protégés facilitated his ability to jump between research topics—and ultimately, helped him develop some of his most important contributions to physics.

Oppenheimer’s climactic third paper, written with his student Hartland Snyder, explores the implications of general relativity on the universe’s most massive stars. Although the physicists needed to include some assumptions to simplify the question, they determined that a large enough star would gravitationally collapse indefinitely—and within a finite amount of time, meaning that the objects we now know as black holes could exist.

Internet: <scientificamerican.com> (adapted)

Based on text CB1A2-I, judge the following item.

The word “war” (first sentence of the second paragraph) refers to any war.

Certo

Errado

Você errou! Resposta:

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Q2281244

Q2281244 Inglês

Texto associado

Text CB1A2-I

Oppenheimer’s brief advance into astrophysics began with a 1938 paper about neutron stars, which continued in a 1939 installment that further incorporated the principles of Einstein’s general theory of relativity. He then published a third paper on black holes on September 1st, 1939—but at the time, it was scarcely noticed because this was the very day Germany invaded Poland, launching World War II. Oppenheimer never wrote on the topic again.

Even if it hadn’t been overshadowed by war, Oppenheimer’s work on neutron stars and black holes “was not understood to be terribly significant at the time,” says Cathryn Carson, a historian of science at the University of California, Berkeley.

Each paper was written with a different member of the swarm of graduate students that Oppenheimer carefully cultivated. These protégés facilitated his ability to jump between research topics—and ultimately, helped him develop some of his most important contributions to physics.

Oppenheimer’s climactic third paper, written with his student Hartland Snyder, explores the implications of general relativity on the universe’s most massive stars. Although the physicists needed to include some assumptions to simplify the question, they determined that a large enough star would gravitationally collapse indefinitely—and within a finite amount of time, meaning that the objects we now know as black holes could exist.

Internet: <scientificamerican.com> (adapted)

Based on text CB1A2-I, judge the following item.

Hartland Snyder helped Oppenheimer write his least relevant paper in physics.

Certo

Errado

Você errou! Resposta:

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Q2281245

Q2281245 Inglês

Texto associado

Text CB1A2-I

Oppenheimer’s brief advance into astrophysics began with a 1938 paper about neutron stars, which continued in a 1939 installment that further incorporated the principles of Einstein’s general theory of relativity. He then published a third paper on black holes on September 1st, 1939—but at the time, it was scarcely noticed because this was the very day Germany invaded Poland, launching World War II. Oppenheimer never wrote on the topic again.

Even if it hadn’t been overshadowed by war, Oppenheimer’s work on neutron stars and black holes “was not understood to be terribly significant at the time,” says Cathryn Carson, a historian of science at the University of California, Berkeley.

Each paper was written with a different member of the swarm of graduate students that Oppenheimer carefully cultivated. These protégés facilitated his ability to jump between research topics—and ultimately, helped him develop some of his most important contributions to physics.

Oppenheimer’s climactic third paper, written with his student Hartland Snyder, explores the implications of general relativity on the universe’s most massive stars. Although the physicists needed to include some assumptions to simplify the question, they determined that a large enough star would gravitationally collapse indefinitely—and within a finite amount of time, meaning that the objects we now know as black holes could exist.

Internet: <scientificamerican.com> (adapted)

Based on the vocabulary and linguistic aspects of text CB1A2-I, judge the following item.
The pronoun “they” (last sentence of the last paragraph) refers to the word “assumptions”.

Certo

Errado

Você errou! Resposta:

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Q2281246

Q2281246 Inglês

Texto associado

Text CB1A2-I

Oppenheimer’s brief advance into astrophysics began with a 1938 paper about neutron stars, which continued in a 1939 installment that further incorporated the principles of Einstein’s general theory of relativity. He then published a third paper on black holes on September 1st, 1939—but at the time, it was scarcely noticed because this was the very day Germany invaded Poland, launching World War II. Oppenheimer never wrote on the topic again.

Even if it hadn’t been overshadowed by war, Oppenheimer’s work on neutron stars and black holes “was not understood to be terribly significant at the time,” says Cathryn Carson, a historian of science at the University of California, Berkeley.

Each paper was written with a different member of the swarm of graduate students that Oppenheimer carefully cultivated. These protégés facilitated his ability to jump between research topics—and ultimately, helped him develop some of his most important contributions to physics.

Oppenheimer’s climactic third paper, written with his student Hartland Snyder, explores the implications of general relativity on the universe’s most massive stars. Although the physicists needed to include some assumptions to simplify the question, they determined that a large enough star would gravitationally collapse indefinitely—and within a finite amount of time, meaning that the objects we now know as black holes could exist.

Internet: <scientificamerican.com> (adapted)

Based on the vocabulary and linguistic aspects of text CB1A2-I, judge the following item.

The word “overshadowed” (first sentence of the second paragraph) means, in the context of text CB1A2-I, “made less noticeable”.

Certo

Errado

Você errou! Resposta:

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Q2281247

Q2281247 Inglês

Texto associado

Text CB1A2-I

Oppenheimer’s brief advance into astrophysics began with a 1938 paper about neutron stars, which continued in a 1939 installment that further incorporated the principles of Einstein’s general theory of relativity. He then published a third paper on black holes on September 1st, 1939—but at the time, it was scarcely noticed because this was the very day Germany invaded Poland, launching World War II. Oppenheimer never wrote on the topic again.

Even if it hadn’t been overshadowed by war, Oppenheimer’s work on neutron stars and black holes “was not understood to be terribly significant at the time,” says Cathryn Carson, a historian of science at the University of California, Berkeley.

Each paper was written with a different member of the swarm of graduate students that Oppenheimer carefully cultivated. These protégés facilitated his ability to jump between research topics—and ultimately, helped him develop some of his most important contributions to physics.

Oppenheimer’s climactic third paper, written with his student Hartland Snyder, explores the implications of general relativity on the universe’s most massive stars. Although the physicists needed to include some assumptions to simplify the question, they determined that a large enough star would gravitationally collapse indefinitely—and within a finite amount of time, meaning that the objects we now know as black holes could exist.

Internet: <scientificamerican.com> (adapted)

Based on the vocabulary and linguistic aspects of text CB1A2-I, judge the following item.

The word “installment” (first sentence of the first paragraph) means, in the context of text CB1A2-I, “to make it ready to use”.

Certo

Errado

Você errou! Resposta:

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Q2281248

Q2281248 Inglês

Texto associado

Text CB1A2-I

Oppenheimer’s brief advance into astrophysics began with a 1938 paper about neutron stars, which continued in a 1939 installment that further incorporated the principles of Einstein’s general theory of relativity. He then published a third paper on black holes on September 1st, 1939—but at the time, it was scarcely noticed because this was the very day Germany invaded Poland, launching World War II. Oppenheimer never wrote on the topic again.

Even if it hadn’t been overshadowed by war, Oppenheimer’s work on neutron stars and black holes “was not understood to be terribly significant at the time,” says Cathryn Carson, a historian of science at the University of California, Berkeley.

Each paper was written with a different member of the swarm of graduate students that Oppenheimer carefully cultivated. These protégés facilitated his ability to jump between research topics—and ultimately, helped him develop some of his most important contributions to physics.

Oppenheimer’s climactic third paper, written with his student Hartland Snyder, explores the implications of general relativity on the universe’s most massive stars. Although the physicists needed to include some assumptions to simplify the question, they determined that a large enough star would gravitationally collapse indefinitely—and within a finite amount of time, meaning that the objects we now know as black holes could exist.

Internet: <scientificamerican.com> (adapted)

Based on the vocabulary and linguistic aspects of text CB1A2-I, judge the following item.

The word “physicists” means “medical doctors”.

Certo

Errado

Você errou! Resposta:

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Q2281249

Q2281249 Inglês

Texto associado

Text CB1A2-I

Oppenheimer’s brief advance into astrophysics began with a 1938 paper about neutron stars, which continued in a 1939 installment that further incorporated the principles of Einstein’s general theory of relativity. He then published a third paper on black holes on September 1st, 1939—but at the time, it was scarcely noticed because this was the very day Germany invaded Poland, launching World War II. Oppenheimer never wrote on the topic again.

Even if it hadn’t been overshadowed by war, Oppenheimer’s work on neutron stars and black holes “was not understood to be terribly significant at the time,” says Cathryn Carson, a historian of science at the University of California, Berkeley.

Each paper was written with a different member of the swarm of graduate students that Oppenheimer carefully cultivated. These protégés facilitated his ability to jump between research topics—and ultimately, helped him develop some of his most important contributions to physics.

Oppenheimer’s climactic third paper, written with his student Hartland Snyder, explores the implications of general relativity on the universe’s most massive stars. Although the physicists needed to include some assumptions to simplify the question, they determined that a large enough star would gravitationally collapse indefinitely—and within a finite amount of time, meaning that the objects we now know as black holes could exist.

Internet: <scientificamerican.com> (adapted)

Based on the vocabulary and linguistic aspects of text CB1A2-I, judge the following item.

Graduate students are people studying for a master’s degree or doctorate.

Certo

Errado

Você errou! Resposta:

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Q2286055

Ano: 2023 Banca: CESPE / CEBRASPE Órgão: TBG Prova: CESPE / CEBRASPE - 2023 - TBG - Analista Júnior – Ênfase: Gestão, Meio Ambiente |

Q2286055 Engenharia Ambiental e Sanitária

Texto associado

A fonte e a quantidade de energia disponível determinam, a um grau maior ou menor, os tipos e a abundância dos organismos, o padrão dos processos funcionais e de desenvolvimento e o estilo de vida dos seres humanos. Já que a energia é um denominador comum e a função motriz final em todos os ecossistemas, seja antropogênico, seja natural, ela fornece uma base lógica para uma classificação de “primeira ordem”.

Eugene P. Odum. Ecologia. Rio de Janeiro: Guanabara, 1988

Considerando a classificação de ecossistemas citada no texto precedente, julgue o item a seguir.

A produtividade dos ecossistemas de energia solar com subsídios naturais é bem maior que a dos ecossistemas com subsídios antropogênicos.

Certo

Errado

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Q2286056

Ano: 2023 Banca: CESPE / CEBRASPE Órgão: TBG Prova: CESPE / CEBRASPE - 2023 - TBG - Analista Júnior – Ênfase: Gestão, Meio Ambiente |

Q2286056 Engenharia Ambiental e Sanitária

Texto associado

A fonte e a quantidade de energia disponível determinam, a um grau maior ou menor, os tipos e a abundância dos organismos, o padrão dos processos funcionais e de desenvolvimento e o estilo de vida dos seres humanos. Já que a energia é um denominador comum e a função motriz final em todos os ecossistemas, seja antropogênico, seja natural, ela fornece uma base lógica para uma classificação de “primeira ordem”.

Eugene P. Odum. Ecologia. Rio de Janeiro: Guanabara, 1988

Considerando a classificação de ecossistemas citada no texto precedente, julgue o item a seguir.

A referida classificação baseia-se na estrutura interna dos ecossistemas.

Certo

Errado

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Q2286057

Ano: 2023 Banca: CESPE / CEBRASPE Órgão: TBG Prova: CESPE / CEBRASPE - 2023 - TBG - Analista Júnior – Ênfase: Gestão, Meio Ambiente |

Q2286057 Engenharia Ambiental e Sanitária

Texto associado

A fonte e a quantidade de energia disponível determinam, a um grau maior ou menor, os tipos e a abundância dos organismos, o padrão dos processos funcionais e de desenvolvimento e o estilo de vida dos seres humanos. Já que a energia é um denominador comum e a função motriz final em todos os ecossistemas, seja antropogênico, seja natural, ela fornece uma base lógica para uma classificação de “primeira ordem”.

Eugene P. Odum. Ecologia. Rio de Janeiro: Guanabara, 1988

Considerando a classificação de ecossistemas citada no texto precedente, julgue o item a seguir.

As grandes áreas de florestas de altitude são exemplos da classe de ecossistemas de energia solar cujas fontes auxiliares de energia são dispensáveis.

Certo

Errado

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Q2286058

Ano: 2023 Banca: CESPE / CEBRASPE Órgão: TBG Prova: CESPE / CEBRASPE - 2023 - TBG - Analista Júnior – Ênfase: Gestão, Meio Ambiente |

Q2286058 Engenharia Ambiental e Sanitária

Texto associado

A fonte e a quantidade de energia disponível determinam, a um grau maior ou menor, os tipos e a abundância dos organismos, o padrão dos processos funcionais e de desenvolvimento e o estilo de vida dos seres humanos. Já que a energia é um denominador comum e a função motriz final em todos os ecossistemas, seja antropogênico, seja natural, ela fornece uma base lógica para uma classificação de “primeira ordem”.

Eugene P. Odum. Ecologia. Rio de Janeiro: Guanabara, 1988

Considerando a classificação de ecossistemas citada no texto precedente, julgue o item a seguir.

Um estuário costeiro tem na energia das marés um subsídio natural de energia que reduz o custo unitário da automanutenção do ecossistema.

Certo

Errado

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Q2286059

Ano: 2023 Banca: CESPE / CEBRASPE Órgão: TBG Prova: CESPE / CEBRASPE - 2023 - TBG - Analista Júnior – Ênfase: Gestão, Meio Ambiente |

Q2286059 Meteorologia

No que diz respeito aos ciclones extratropicais, responsáveis pelas tempestades que ocorrem entre as costas sul e sudeste do Brasil, julgue os seguinte item.

A nebulosidade presente em um ciclone extratropical cujo formato é de uma vírgula invertida se deve ao ramo frio do sistema frontal associado ao ciclone.

Certo

Errado

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Q2286060

Ano: 2023 Banca: CESPE / CEBRASPE Órgão: TBG Prova: CESPE / CEBRASPE - 2023 - TBG - Analista Júnior – Ênfase: Gestão, Meio Ambiente |

Q2286060 Meteorologia

No que diz respeito aos ciclones extratropicais, responsáveis pelas tempestades que ocorrem entre as costas sul e sudeste do Brasil, julgue os seguinte item.

No hemisfério sul, o escoamento atmosférico em um ciclone extratropical tem giro anti-horário devido à força de Coriolis.

Certo

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Q2286061

Ano: 2023 Banca: CESPE / CEBRASPE Órgão: TBG Prova: CESPE / CEBRASPE - 2023 - TBG - Analista Júnior – Ênfase: Gestão, Meio Ambiente |

Q2286061 Meteorologia

No que diz respeito aos ciclones extratropicais, responsáveis pelas tempestades que ocorrem entre as costas sul e sudeste do Brasil, julgue os seguinte item.

Os ciclones extratropicais, bastante frequentes na região Sul do Brasil, são sistemas atmosféricos que afetam e modulam as condições do tempo atmosférico.

Certo

Errado

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Q2286062

Ano: 2023 Banca: CESPE / CEBRASPE Órgão: TBG Prova: CESPE / CEBRASPE - 2023 - TBG - Analista Júnior – Ênfase: Gestão, Meio Ambiente |

Q2286062 Meteorologia

No que diz respeito aos ciclones extratropicais, responsáveis pelas tempestades que ocorrem entre as costas sul e sudeste do Brasil, julgue os seguinte item.

O ciclone extratropical caracteriza-se como um sistema meteorológico que apresenta maior pressão atmosférica que o ambiente ao seu redor.

Certo

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Q2286063

Ano: 2023 Banca: CESPE / CEBRASPE Órgão: TBG Prova: CESPE / CEBRASPE - 2023 - TBG - Analista Júnior – Ênfase: Gestão, Meio Ambiente |

Q2286063 Engenharia Ambiental e Sanitária

Em relação às propriedades dos solos, julgue o item subsequente.

Nos solos de estrutura massiva, a presença de agregados grandes e estáveis condiciona a ocorrência de poros grandes, por meio dos quais a água e o ar podem se mover livremente e as raízes de plantas encontram caminhos fáceis para crescer.

Certo

Errado

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Q2286064

Ano: 2023 Banca: CESPE / CEBRASPE Órgão: TBG Prova: CESPE / CEBRASPE - 2023 - TBG - Analista Júnior – Ênfase: Gestão, Meio Ambiente |

Q2286064 Engenharia Ambiental e Sanitária

Em relação às propriedades dos solos, julgue o item subsequente.

A análise da estrutura do solo permite que se diferenciem as manifestações das forças de adesão e coesão de partículas do solo, que podem variar conforme a textura do solo e a presença de matéria orgânica e minerais.

Certo

Errado

Quer um estudo ilimitado?

Quer um estudo ilimitado?

Questões de Concurso Público TBG 2023 para Analista Júnior – Ênfase: Gestão, Meio Ambiente

Foram encontradas 100 questões