{"id":3674,"date":"2018-02-13T14:10:20","date_gmt":"2018-02-13T14:10:20","guid":{"rendered":"http:\/\/fisicaevestibular.com.br\/novo\/?page_id=3674"},"modified":"2024-06-26T15:18:04","modified_gmt":"2024-06-26T15:18:04","slug":"gravitacao-universal-lei-da-gravitacao-universal-e-satelites-em-orbitas","status":"publish","type":"page","link":"https:\/\/fisicaevestibular.com.br\/novo\/enem\/gravitacao-universal-lei-da-gravitacao-universal-e-satelites-em-orbitas\/","title":{"rendered":"Lei da Gravita\u00e7\u00e3o Universal e Sat\u00e9lites em \u00d3rbitas"},"content":{"rendered":"

Gravita\u00e7\u00e3o Universal<\/b><\/span><\/span><\/span><\/p>\n

Lei da Gravita\u00e7\u00e3o Universal e Sat\u00e9lites em \u00d3rbitas<\/b><\/span><\/span><\/span><\/p>\n

Exerc\u00edcios com caracter\u00edsticas de ENEM<\/b><\/span><\/span><\/span><\/p>\n

01-(UDESC-SC-010)\u00a0<\/b><\/span><\/span><\/span><\/p>\n

\"Gravita\u00e7\u00e3o\"<\/p>\n

A mar\u00e9 \u00e9 o fen\u00f4meno natural de subida e descida do n\u00edvel das \u00e1guas, percebido principalmente nos oceanos, causado pela atra\u00e7\u00e3o gravitacional do Sol e da Lua. A ilustra\u00e7\u00e3o a seguir esquematiza a <\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

varia\u00e7\u00e3o do n\u00edvel das \u00e1guas ao longo de uma rota\u00e7\u00e3o completa da Terra. Considere as seguintes proposi\u00e7\u00f5es sobre mar\u00e9, e assinale a alternativa incorreta.<\/b><\/span><\/span><\/span><\/p>\n

a) As mar\u00e9s de maior amplitude ocorrem pr\u00f3ximo das situa\u00e7\u00f5es de Lua Nova ou Lua Cheia, quando as for\u00e7as atrativas, devido ao Sol e \u00e0 Lua, se refor\u00e7am mutuamente.\u00a0<\/b><\/span><\/span><\/span><\/p>\n

b) A influ\u00eancia da Lua \u00e9 maior do que a do Sol, pois, embora a sua massa seja muito menor do que a do Sol, esse fato \u00e9 compensado pela menor dist\u00e2ncia \u00e0 Terra.\u00a0<\/b><\/span><\/span><\/span><\/p>\n

c) A mar\u00e9 cheia \u00e9 vista por um observador quando a Lua passa por cima dele, ou quando a Lua passa por baixo dele.\u00a0<\/b><\/span><\/span><\/span><\/p>\n

d) As massas de \u00e1gua que est\u00e3o mais pr\u00f3ximas da Lua ou do Sol sofrem atra\u00e7\u00e3o maior do que as massas de \u00e1gua que est\u00e3o mais afastadas, devido \u00e0 rota\u00e7\u00e3o da Terra.\u00a0<\/b><\/span><\/span><\/span><\/p>\n

e) As mar\u00e9s alta e baixa sucedem-se em intervalos de aproximadamente 6 horas.\u00a0<\/b><\/span><\/span><\/span><\/p>\n

\u00a0<\/span><\/p>\n

\u00a0<\/span>02-(ITA-SP)<\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

Sabe-se que a atra\u00e7\u00e3o gravitacional da Lua sobre a camada de \u00e1gua \u00e9 a principal respons\u00e1vel pelo <\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

aparecimento das mar\u00e9s oce\u00e2nicas na Terra.\u00a0 Considere as seguintes afirmativas:<\/b><\/span><\/span><\/span><\/p>\n

I. As massa de \u00e1gua pr\u00f3ximas das regi\u00f5es A e B experimentam mar\u00e9s altas simultaneamente.<\/b><\/span><\/span><\/span><\/p>\n

II. As massas de \u00e1gua pr\u00f3ximas das regi\u00f5es A e B experimentam mar\u00e9s opostas, isto \u00e9, quando A tem mar\u00e9 alta, B tem mar\u00e9 baixa e vice-versa.<\/b><\/span><\/span><\/span><\/p>\n

III. Durante o intervalo de tempo de um dia ocorrem duas mar\u00e9s altas e duas mar\u00e9s baixas.<\/b><\/span><\/span><\/span><\/p>\n

Ent\u00e3o, est\u00e1(r\u00e3o) correta(s), apenas:<\/b><\/span><\/span><\/span><\/p>\n

a) a afirmativa I\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0 <\/b><\/span><\/span><\/span><\/p>\n

b) a afirmativa II\u00a0\u00a0\u00a0\u00a0 \u00a0\u00a0\u00a0\u00a0\u00a0<\/b><\/span><\/span><\/span><\/p>\n

c) a afirmativa III\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0 <\/b><\/span><\/span><\/span><\/p>\n

d) as afirmativas I e II\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0 <\/b><\/span><\/span><\/span><\/p>\n

e) as afirmativas I e III<\/b><\/span><\/span><\/span><\/p>\n

\u00a0<\/span><\/p>\n

03-(UFV-MG)\u00a0<\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

\u00a0Seja F o m\u00f3dulo da for\u00e7a da gravidade que o Sol faz sobre um cometa, de massa constante, cujo per\u00edodo orbital \u00e9 T (em anos).<\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

Dos gr\u00e1ficos adiante, aquele que representa CORRETAMENTE a varia\u00e7\u00e3o de F com o tempo t \u00e9:<\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

\u00a0<\/span><\/p>\n

04-(UNICAMP-SP)\u00a0<\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

Observa\u00e7\u00f5es astron\u00f4micas indicam que as velocidades de rota\u00e7\u00e3o das estrelas em torno de <\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

gal\u00e1xias s\u00e3o incompat\u00edveis com a distribui\u00e7\u00e3o de massa vis\u00edvel das gal\u00e1xias, sugerindo que grande parte da mat\u00e9ria do Universo \u00e9 escura, isto \u00e9, mat\u00e9ria que n\u00e3o interage com a luz. O movimento de rota\u00e7\u00e3o das estrelas resulta da for\u00e7a de atra\u00e7\u00e3o gravitacional que as gal\u00e1xias exercem sobre elas.<\/b><\/span><\/span><\/span><\/p>\n

A curva no gr\u00e1fico abaixo mostra como a for\u00e7a gravitacional\u00a0F=GMm\/r<\/b><\/span><\/span><\/span>2<\/b><\/span><\/span><\/sup><\/span>\u00a0que uma gal\u00e1xia de massa\u00a0M\u00a0exerce sobre uma estrela externa \u00e0 gal\u00e1xia, deve variar em fun\u00e7\u00e3o da dist\u00e2ncia\u00a0r da estrela em rela\u00e7\u00e3o ao centro da gal\u00e1xia, considerando-se m=1,0.10<\/b><\/span><\/span><\/span>30\u00a0<\/b><\/span><\/span><\/sup><\/span>kg<\/b><\/span><\/span><\/span><\/p>\n

para a massa da estrela. A constante de gravita\u00e7\u00e3o\u00a0G\u00a0vale 6,7.10<\/b><\/span><\/span><\/span>-11<\/b><\/span><\/span><\/sup><\/span>\u00a0N.m<\/b><\/span><\/span><\/span>2<\/b><\/span><\/span><\/sup><\/span>.kg<\/b><\/span><\/span><\/span>-2<\/b><\/span><\/span><\/sup><\/span>.<\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

A massa M da gal\u00e1xia vale, aproximadamente, em kg:<\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

05-(FUVEST-SP)<\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

Sat\u00e9lites utilizados para telecomunica\u00e7\u00f5es s\u00e3o colocados em \u00f3rbitas geo-estacion\u00e1rias ao redor da <\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

Terra, ou seja,\u00a0 de tal forma que permane\u00e7am sempre acima de um mesmo ponto da superf\u00edcie da Terra. Considere algumas condi\u00e7\u00f5es que deveriam corresponder a esses sat\u00e9lites:<\/b><\/span><\/span><\/span><\/p>\n

I.\u00a0\u00a0\u00a0 Ter o mesmo per\u00edodo, de cerca de 24 horas.<\/b><\/span><\/span><\/span><\/p>\n

II.\u00a0\u00a0 Ter aproximadamente a mesma massa.<\/b><\/span><\/span><\/span><\/p>\n

III.\u00a0 Estar aproximadamente \u00e0 mesma altitude.<\/b><\/span><\/span><\/span><\/p>\n

IV.\u00a0 Manter-se num plano que contenha o c\u00edrculo do equador terrestre.<\/b><\/span><\/span><\/span><\/p>\n

O conjunto de todas as condi\u00e7\u00f5es que sat\u00e9lites em \u00f3rbitas geo-estacion\u00e1rias devem necessariamente obedecer corresponde a:<\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

\u00a0<\/span><\/p>\n

06-(FGV-RJ)<\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

Muitos sat\u00e9lites utilizados em telefonia, transmiss\u00f5es de r\u00e1dio e TV, internet e outros servi\u00e7os de telecomunica\u00e7\u00f5es ocupam a \u00f3rbita geoestacion\u00e1ria. Nesta \u00f3rbita, situada no plano da linha do <\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

equador, os sat\u00e9lites permanecem sempre acima de um mesmo ponto da superf\u00edcie terrestre, parecendo parados para um observador no equador. A altura de um sat\u00e9lite geoc\u00eantrico, em rela\u00e7\u00e3o \u00e0 superf\u00edcie da Terra, em \u00f3rbita circular, \u00e9 aproximadamente igual a<\/b><\/span><\/span><\/span><\/p>\n

Dados: G = constante de gravita\u00e7\u00e3o universal; M = massa da Terra; R = raio da Terra = 6, 4.10<\/b><\/span><\/span><\/span>6<\/b><\/span><\/span><\/sup><\/span>\u00a0m; (G M\/4 \u03c0<\/b><\/span><\/span><\/span>2<\/b><\/span><\/span><\/sup><\/span>)\/3\u00a0=2,2.10<\/b><\/span><\/span><\/span>4<\/b><\/span><\/span><\/sup><\/span>ms<\/b><\/span><\/span><\/span>-2\/3<\/b><\/span><\/span><\/sup><\/span><\/p>\n

; (24 horas)<\/b><\/span><\/span><\/span>2\/3<\/b><\/span><\/span><\/sup><\/span>\u00a0= 2,0.10<\/b><\/span><\/span><\/span>3<\/b><\/span><\/span><\/sup><\/span>\u00a0s<\/b><\/span><\/span><\/span>2\/3<\/b><\/span><\/span><\/sup><\/span><\/p>\n

a) 37.600 km.\u00a0 \u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0<\/b><\/span><\/span><\/span><\/p>\n

b) 50.000 km.\u00a0 \u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0<\/b><\/span><\/span><\/span><\/p>\n

c) 64.000 km.\u00a0 \u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0<\/b><\/span><\/span><\/span><\/p>\n

d) 12.800 km.\u00a0 \u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0<\/b><\/span><\/span><\/span><\/p>\n

e) 25.000 km.\u00a0<\/b><\/span><\/span><\/span><\/p>\n

\u00a0<\/span><\/p>\n

07-(UFES-ES)<\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

Dois sat\u00e9lites descrevem \u00f3rbitas circulares em torno da Terra.<\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

O raio da \u00f3rbita do sat\u00e9lite mais afastado da Terra \u00e9 o dobro do raio da \u00f3rbita do sat\u00e9lite mais pr\u00f3ximo. Considere que V<\/b><\/span><\/span><\/span>a<\/b><\/span><\/span><\/sub><\/span>\u00a0e V<\/b><\/span><\/span><\/span>f\u00a0<\/b><\/span><\/span><\/sub><\/span>s\u00e3o, respectivamente, os m\u00f3dulos das velocidades do sat\u00e9lite afastado e do sat\u00e9lite pr\u00f3ximo. A rela\u00e7\u00e3o entre esses m\u00f3dulos \u00e9:<\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

08-(UFMG-MG)<\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

Dois sat\u00e9lites artificiais, R e S, est\u00e3o em \u00f3rbitas circulares de mesmo raio, em torno da Terra.<\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

A massa do sat\u00e9lite R \u00e9 maior que a do sat\u00e9lite S. Com rela\u00e7\u00e3o ao m\u00f3dulo das velocidades, V<\/b><\/span><\/span><\/span>R<\/b><\/span><\/span><\/sub><\/span>\u00a0e V<\/b><\/span><\/span><\/span>S<\/b><\/span><\/span><\/sub><\/span>, e dos per\u00edodos\u00a0 de transla\u00e7\u00e3o, T<\/b><\/span><\/span><\/span>R<\/b><\/span><\/span><\/sub><\/span>\u00a0e T<\/b><\/span><\/span><\/span>S<\/b><\/span><\/span><\/sub><\/span>, pode-se afirmar que:<\/b><\/span><\/span><\/span><\/p>\n

a) V<\/b><\/span><\/span><\/span>R<\/b><\/span><\/span><\/sub><\/span>\u00a0<\u00a0 V<\/b><\/span><\/span><\/span>S<\/b><\/span><\/span><\/sub><\/span>\u00a0\u00a0e T<\/b><\/span><\/span><\/span>R<\/b><\/span><\/span><\/sub><\/span>\u00a0\u00a0=\u00a0T<\/b><\/span><\/span><\/span>S<\/b><\/span><\/span><\/sub><\/span>\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0 <\/b><\/span><\/span><\/span><\/p>\n

b) V<\/b><\/span><\/span><\/span>R<\/b><\/span><\/span><\/sub><\/span>\u00a0\u00a0<\u00a0V<\/b><\/span><\/span><\/span>S<\/b><\/span><\/span><\/sub><\/span>\u00a0\u00a0e T<\/b><\/span><\/span><\/span>R<\/b><\/span><\/span><\/sub><\/span>\u00a0\u00a0>\u00a0\u00a0T<\/b><\/span><\/span><\/span>S<\/b><\/span><\/span><\/sub><\/span>\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0 <\/b><\/span><\/span><\/span><\/p>\n

c) V<\/b><\/span><\/span><\/span>R<\/b><\/span><\/span><\/sub><\/span>\u00a0=\u00a0 V<\/b><\/span><\/span><\/span>S<\/b><\/span><\/span><\/sub><\/span>\u00a0\u00a0e T<\/b><\/span><\/span><\/span>R<\/b><\/span><\/span><\/sub><\/span>\u00a0\u00a0=T<\/b><\/span><\/span><\/span>S<\/b><\/span><\/span><\/sub><\/span>\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0 <\/b><\/span><\/span><\/span><\/p>\n

d) V<\/b><\/span><\/span><\/span>R<\/b><\/span><\/span><\/sub><\/span>\u00a0=\u00a0 V<\/b><\/span><\/span><\/span>S<\/b><\/span><\/span><\/sub><\/span>\u00a0\u00a0e T<\/b><\/span><\/span><\/span>R<\/b><\/span><\/span><\/sub><\/span>\u00a0\u00a0>\u00a0\u00a0T<\/b><\/span><\/span><\/span>S<\/b><\/span><\/span><\/sub><\/span>\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0<\/b><\/span><\/span><\/span><\/p>\n

e) V<\/b><\/span><\/span><\/span>R\u00a0<\/b><\/span><\/span><\/sub><\/span>\u00a0>\u00a0 V<\/b><\/span><\/span><\/span>S<\/b><\/span><\/span><\/sub><\/span>\u00a0\u00a0e T<\/b><\/span><\/span><\/span>R<\/b><\/span><\/span><\/sub><\/span>\u00a0\u00a0>\u00a0\u00a0T<\/b><\/span><\/span><\/span>S<\/b><\/span><\/span><\/sub><\/span><\/p>\n

\u00a0<\/span><\/p>\n

09-(UNICAMP-SP)<\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

Observa\u00e7\u00f5es astron\u00f4micas indicam que as velocidades de rota\u00e7\u00e3o das estrelas em torno de gal\u00e1xias s\u00e3o incompat\u00edveis com a distribui\u00e7\u00e3o de massa vis\u00edvel das gal\u00e1xias, sugerindo que grande <\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

parte da mat\u00e9ria do Universo \u00e9 escura, isto \u00e9, mat\u00e9ria que n\u00e3o<\/b><\/span><\/span><\/span><\/p>\n

interage com a luz. O movimento de rota\u00e7\u00e3o das estrelas resulta da for\u00e7a de atra\u00e7\u00e3o gravitacional que as gal\u00e1xias exercem sobre elas.<\/b><\/span><\/span><\/span><\/p>\n

A curva no gr\u00e1fico abaixo mostra como a for\u00e7a gravitacional\u00a0F=GMm\/r<\/b><\/span><\/span><\/span>2\u00a0<\/b><\/span><\/span><\/sup><\/span>que uma gal\u00e1xia de massa\u00a0M\u00a0exerce sobre uma estrela externa \u00e0 gal\u00e1xia, deve variar em fun\u00e7\u00e3o da dist\u00e2ncia\u00a0r\u00a0da estrela em rela\u00e7\u00e3o ao centro da gal\u00e1xia, considerando-se m=1,0.10<\/b><\/span><\/span><\/span>30<\/b><\/span><\/span><\/sup><\/span>kg<\/b><\/span><\/span><\/span><\/p>\n

para a massa da estrela. A constante de gravita\u00e7\u00e3o\u00a0G\u00a0vale \u00a06,7.10<\/b><\/span><\/span><\/span>-11<\/b><\/span><\/span><\/sup><\/span>\u00a0Nm<\/b><\/span><\/span><\/span>2<\/b><\/span><\/span><\/sup><\/span>.kg<\/b><\/span><\/span><\/span>-2<\/b><\/span><\/span><\/sup><\/span>.<\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

\u00a0A velocidade de uma estrela em \u00f3rbita circular a uma dist\u00e2ncia\u00a0r=1,6.10<\/b><\/span><\/span><\/span>20<\/b><\/span><\/span><\/sup><\/span>\u00a0m do centro da gal\u00e1xia vale:<\/b><\/span><\/span><\/span><\/p>\n

a) V=8,0.10<\/b><\/span><\/span><\/span>4<\/b><\/span><\/span><\/sup><\/span>m\/s\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0 <\/b><\/span><\/span><\/span><\/p>\n

b) V=2,0.10<\/b><\/span><\/span><\/span>4<\/b><\/span><\/span><\/sup><\/span>m\/s\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0 <\/b><\/span><\/span><\/span><\/p>\n

c) V=3,0.10<\/b><\/span><\/span><\/span>5<\/b><\/span><\/span><\/sup><\/span>m\/s\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0 <\/b><\/span><\/span><\/span><\/p>\n

d) V=8,0.10<\/b><\/span><\/span><\/span>6<\/b><\/span><\/span><\/sup><\/span>m\/s\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0 <\/b><\/span><\/span><\/span><\/p>\n

e) V=3,0.10<\/b><\/span><\/span><\/span>6<\/b><\/span><\/span><\/sup><\/span>m\/s<\/b><\/span><\/span><\/span><\/p>\n

\u00a0<\/span><\/p>\n

Confira a resolu\u00e7\u00e3o comentada<\/span><\/a><\/h3>\n

 <\/p>\n

Clique aqui para ver sobre o tema!<\/a><\/p>\n

Confira as v\u00eddeo aulas!<\/a>\u00a0<\/span><\/p>\n","protected":false},"excerpt":{"rendered":"

Gravita\u00e7\u00e3o Universal Lei da Gravita\u00e7\u00e3o Universal e Sat\u00e9lites em \u00d3rbitas Exerc\u00edcios com caracter\u00edsticas de ENEM 01-(UDESC-SC-010)\u00a0 A mar\u00e9 \u00e9 o fen\u00f4meno natural de subida e descida do n\u00edvel das \u00e1guas, percebido principalmente nos oceanos, causado pela atra\u00e7\u00e3o gravitacional do Sol e da Lua. A ilustra\u00e7\u00e3o a seguir esquematiza a varia\u00e7\u00e3o do n\u00edvel das \u00e1guas ao longo de uma rota\u00e7\u00e3o completa<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":3575,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"om_disable_all_campaigns":false,"_monsterinsights_skip_tracking":false,"_monsterinsights_sitenote_active":false,"_monsterinsights_sitenote_note":"","_monsterinsights_sitenote_category":0,"footnotes":""},"class_list":["post-3674","page","type-page","status-publish","hentry"],"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/fisicaevestibular.com.br\/novo\/wp-json\/wp\/v2\/pages\/3674","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/fisicaevestibular.com.br\/novo\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/fisicaevestibular.com.br\/novo\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/fisicaevestibular.com.br\/novo\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/fisicaevestibular.com.br\/novo\/wp-json\/wp\/v2\/comments?post=3674"}],"version-history":[{"count":4,"href":"https:\/\/fisicaevestibular.com.br\/novo\/wp-json\/wp\/v2\/pages\/3674\/revisions"}],"predecessor-version":[{"id":9795,"href":"https:\/\/fisicaevestibular.com.br\/novo\/wp-json\/wp\/v2\/pages\/3674\/revisions\/9795"}],"up":[{"embeddable":true,"href":"https:\/\/fisicaevestibular.com.br\/novo\/wp-json\/wp\/v2\/pages\/3575"}],"wp:attachment":[{"href":"https:\/\/fisicaevestibular.com.br\/novo\/wp-json\/wp\/v2\/media?parent=3674"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}