{"id":1437,"date":"2015-10-13T03:35:54","date_gmt":"2015-10-13T03:35:54","guid":{"rendered":"http:\/\/fisicaevestibular.com.br\/novo\/?page_id=1437"},"modified":"2024-08-23T14:21:09","modified_gmt":"2024-08-23T14:21:09","slug":"resolucoes-comentadas-dos-exercicios-de-vestibulares-sobre-a-lei-da-gravitacao-universal","status":"publish","type":"page","link":"https:\/\/fisicaevestibular.com.br\/novo\/mecanica\/gravitacao\/lei-da-gravitacao-universal-de-newton\/resolucoes-comentadas-dos-exercicios-de-vestibulares-sobre-a-lei-da-gravitacao-universal\/","title":{"rendered":"Lei da Gravita\u00e7\u00e3o Universal – Resolu\u00e7\u00e3o"},"content":{"rendered":"

Resolu\u00e7\u00f5es comentadas dos exerc\u00edcios de vestibulares sobre a<\/b><\/span><\/span><\/span><\/p>\n

Lei da \u00a0Gravita\u00e7\u00e3o Universal<\/b><\/span><\/span><\/span><\/p>\n

 <\/p>\n

0<\/b><\/span><\/span><\/span>1-<\/b><\/span><\/span><\/span> GM=K (constante)\u00a0 —\u00a0 F=GMm\/R<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 F<\/b><\/span><\/span>1<\/b><\/span><\/span><\/sub>=Km\/R<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 F<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sub>=K2m\/R<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 F<\/b><\/span><\/span>3<\/b><\/span><\/span><\/sub>=K8m\/R<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 R- C<\/b><\/span><\/span><\/p>\n

02-<\/b><\/span><\/span><\/span> F=GMm\/R<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 F\u2019=G2M2m\/R<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>\/4\u00a0 —\u00a0 16F=F\u2019\u00a0 —\u00a0 R- A<\/b><\/span><\/span><\/p>\n

03-<\/b><\/span><\/span><\/span> m<\/b><\/span><\/span>s<\/b><\/span><\/span><\/sub>100m<\/b><\/span><\/span>t\u00a0 —\u00a0\u00a0<\/b><\/span><\/span><\/sub>\u00a0\u00a0F<\/b><\/span><\/span>s<\/b><\/span><\/span><\/sub>=GMm<\/b><\/span><\/span>s<\/b><\/span><\/span><\/sub>\/R<\/b><\/span><\/span>s<\/b><\/span><\/span><\/sub>2<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 F<\/b><\/span><\/span>t<\/b><\/span><\/span><\/sub>=GMm<\/b><\/span><\/span>t<\/b><\/span><\/span><\/sub>\/R<\/b><\/span><\/span>t<\/b><\/span><\/span><\/sub>2<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 F<\/b><\/span><\/span>s<\/b><\/span><\/span><\/sub>\/F<\/b><\/span><\/span>t<\/b><\/span><\/span><\/sub>=GMm<\/b><\/span><\/span>s<\/b><\/span><\/span><\/sub>\/R<\/b><\/span><\/span>s<\/b><\/span><\/span><\/sub>2<\/b><\/span><\/span><\/sup>x R<\/b><\/span><\/span>t<\/b><\/span><\/span><\/sub>2<\/b><\/span><\/span><\/sup>\/GMm<\/b><\/span><\/span>t<\/b><\/span><\/span><\/sub>\u00a0 —\u00a0 F<\/b><\/span><\/span>s<\/b><\/span><\/span><\/sub>\/F<\/b><\/span><\/span>t<\/b><\/span><\/span><\/sub>=100m<\/b><\/span><\/span>t<\/b><\/span><\/span><\/sub>.R<\/b><\/span><\/span>t<\/b><\/span><\/span><\/sub>2<\/b><\/span><\/span><\/sup>\/100R<\/b><\/span><\/span>t<\/b><\/span><\/span><\/sub>2<\/b><\/span><\/span><\/sup>.m<\/b><\/span><\/span>t<\/b><\/span><\/span><\/sub>\u00a0 — F<\/b><\/span><\/span>s<\/b><\/span><\/span><\/sub>\/F<\/b><\/span><\/span>t<\/b><\/span><\/span><\/sub>=1 — R- C<\/b><\/span><\/span><\/p>\n

04-<\/b><\/span><\/span><\/span> m<\/b><\/span><\/span>p<\/b><\/span><\/span><\/sub>\/m<\/b><\/span><\/span>s<\/b><\/span><\/span><\/sub>=81\u00a0 —\u00a0 F<\/b><\/span><\/span>p<\/b><\/span><\/span><\/sub>=GMm<\/b><\/span><\/span>p<\/b><\/span><\/span><\/sub>\/R<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 Fs=GMm<\/b><\/span><\/span>s<\/b><\/span><\/span><\/sub>\/r<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 F<\/b><\/span><\/span>p<\/b><\/span><\/span><\/sub>=F<\/b><\/span><\/span>s<\/b><\/span><\/span><\/sub>\u00a0 —\u00a0 \u00a0\u00a0GMm<\/b><\/span><\/span>p<\/b><\/span><\/span><\/sub>\/R<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>= GMm<\/b><\/span><\/span>s<\/b><\/span><\/span><\/sub>\/r<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 R<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>\/r<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>=m<\/b><\/span><\/span>p<\/b><\/span><\/span><\/sub>\/m<\/b><\/span><\/span>s<\/b><\/span><\/span><\/sub>=81\u00a0 — R\/r=9\u00a0<\/b><\/span><\/span><\/p>\n

\"\"<\/p>\n

R- C<\/b><\/span><\/span><\/p>\n

05- a)<\/b><\/span><\/span><\/span><\/p>\n

\"\"<\/p>\n

b) <\/b><\/span><\/span><\/span>Massas, tanto do Sol quanto do planeta s\u00e3o iguais, independe do meio ou da posi\u00e7\u00e3o. F=GMm\/R<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 M=(1,4.10<\/b><\/span><\/span>23<\/b><\/span><\/span><\/sup>).(0,9.10<\/b><\/span><\/span>11<\/b><\/span><\/span><\/sup>)<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>\/10<\/b><\/span><\/span>-11<\/b><\/span><\/span><\/sup>.7.8,1.10<\/b><\/span><\/span>24<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 M=2,0.10<\/b><\/span><\/span>30<\/b><\/span><\/span><\/sup>kg<\/b><\/span><\/span><\/p>\n

c)<\/b><\/span><\/span><\/span> F<\/b><\/span><\/span>a<\/b><\/span><\/span><\/sub>=GMm\/R<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 F<\/b><\/span><\/span>a<\/b><\/span><\/span><\/sub>=7.10<\/b><\/span><\/span>11<\/b><\/span><\/span><\/sup>.2.10<\/b><\/span><\/span>30<\/b><\/span><\/span><\/sup>.8,1.10<\/b><\/span><\/span>24<\/b><\/span><\/span><\/sup>\/10<\/b><\/span><\/span>22<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 F<\/b><\/span><\/span>a<\/b><\/span><\/span><\/sub>=1,134.10<\/b><\/span><\/span>23<\/b><\/span><\/span><\/sup>N<\/b><\/span><\/span><\/p>\n

06-<\/b><\/span><\/span><\/span> Pelo gr\u00e1fico, quando F=4,0.10<\/b><\/span><\/span>19<\/b><\/span><\/span><\/sup>N, o r ser\u00e1 igual a 1,6.10<\/b><\/span><\/span>20<\/b><\/span><\/span><\/sup>m\u00a0 —\u00a0 4.10<\/b><\/span><\/span>19<\/b><\/span><\/span><\/sup>=6,7.10<\/b><\/span><\/span>-11<\/b><\/span><\/span><\/sup>.M.10<\/b><\/span><\/span>30<\/b><\/span><\/span><\/sup>\/6,7.10<\/b><\/span><\/span>-11<\/b><\/span><\/span><\/sup>.10<\/b><\/span><\/span>30<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 M=10,24.10<\/b><\/span><\/span>59<\/b><\/span><\/span><\/sup>\/6,7.10<\/b><\/span><\/span>19<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 M\u00bb1,6.10<\/b><\/span><\/span>40<\/b><\/span><\/span><\/sup>kg<\/b><\/span><\/span><\/p>\n

07-<\/b><\/span><\/span><\/span> E (vide teoria)<\/b><\/span><\/span><\/p>\n

08-<\/b><\/span><\/span><\/span>\u00a0<\/b><\/span><\/span>A atra\u00e7\u00e3o gravitacional entre massas n\u00e3o depende de nenhuma rota\u00e7\u00e3o\u00a0 —\u00a0<\/b><\/span><\/span>\u00a0R- D<\/b><\/span><\/span><\/p>\n

09-<\/b><\/span><\/span><\/span>\u00a0<\/b><\/span><\/span>Pelo princ\u00edpio da a\u00e7\u00e3o-rea\u00e7\u00e3o (3\u00aa lei da Newton) o m\u00f3dulo da for\u00e7a de atra\u00e7\u00e3o do Sol sobre a Terra \u00e9 igual ao m\u00f3dulo da for\u00e7a de atra\u00e7\u00e3o da Terra sobre o Sol\u00a0 —\u00a0\u00a0<\/b><\/span><\/span>R- A<\/b><\/span><\/span><\/p>\n

10-<\/b><\/span><\/span><\/span>\u00a0<\/b><\/span><\/span>R<\/b><\/span><\/span>T<\/b><\/span><\/span><\/sub>=10<\/b><\/span><\/span>6<\/b><\/span><\/span><\/sup>R<\/b><\/span><\/span>P<\/b><\/span><\/span><\/sub>\u00a0 — a intensidade da acelera\u00e7\u00e3o da gravidade na superf\u00edcie de um planeta homog\u00eaneo e esf\u00e9rico de raio R vale\u00a0 —\u00a0\u00a0 g=GM\/R<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 \u03c1=M\/V\u00a0 —\u00a0 M=\u03c1V\u00a0 —\u00a0 volume do planeta\u00a0 —\u00a0 V=4\u03c0R<\/b><\/span><\/span>3<\/b><\/span><\/span><\/sup>\/3\u00a0 —\u00a0 M=\u03c14\u03c0R<\/b><\/span><\/span>3<\/b><\/span><\/span><\/sup>\/3\u00a0 —\u00a0 g=G \u03c14\u03c0R<\/b><\/span><\/span>3<\/b><\/span><\/span><\/sup>\/3R<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 g= G\u03c14\u03c0R\/3 \u00a0—\u00a0 do enunciado\u00a0 —\u00a0 g<\/b><\/span><\/span>P<\/b><\/span><\/span><\/sub>=g<\/b><\/span><\/span>T<\/b><\/span><\/span><\/sub>\u00a0 —\u00a0 G\u03c1<\/b><\/span><\/span>P<\/b><\/span><\/span><\/sub>4\u03c0R<\/b><\/span><\/span>P<\/b><\/span><\/span><\/sub>\/3= G\u03c1<\/b><\/span><\/span>T<\/b><\/span><\/span><\/sub>4\u03c0R<\/b><\/span><\/span>T<\/b><\/span><\/span><\/sub>\/3\u00a0 —\u00a0 \u03c1<\/b><\/span><\/span>P<\/b><\/span><\/span><\/sub>\/\u03c1<\/b><\/span><\/span>T<\/b><\/span><\/span><\/sub>=R<\/b><\/span><\/span>T<\/b><\/span><\/span><\/sub>\/R<\/b><\/span><\/span>P<\/b><\/span><\/span><\/sub>\u00a0 —\u00a0 \u03c1<\/b><\/span><\/span>P<\/b><\/span><\/span><\/sub>\/\u03c1<\/b><\/span><\/span>T<\/b><\/span><\/span><\/sub>=10<\/b><\/span><\/span>6<\/b><\/span><\/span><\/sup>R<\/b><\/span><\/span>P<\/b><\/span><\/span><\/sub>\/R<\/b><\/span><\/span>P<\/b><\/span><\/span><\/sub>\u00a0 —\u00a0 \u03c1<\/b><\/span><\/span>P<\/b><\/span><\/span><\/sub>\/\u03c1<\/b><\/span><\/span>T<\/b><\/span><\/span><\/sub>=10<\/b><\/span><\/span>6<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0<\/b><\/span><\/span>\u00a0R- B<\/b><\/span><\/span><\/p>\n

11<\/b><\/span><\/span><\/span>–<\/b><\/span><\/span><\/span> Observe que, como o movimento do cometa \u00e9 peri\u00f3dico, sua \u00f3rbita \u00e9 el\u00edptica\u00a0 —\u00a0 assim, a dist\u00e2ncia do Sol ao cometa \u00e9 vari\u00e1vel \u00a0—\u00a0 \u00a0for\u00e7a gravitacional sobre o cometa \u00e9 dada pela lei de Newton da gravita\u00e7\u00e3o\u00a0 —\u00a0 F=GM<\/b><\/span><\/span>Sol<\/b><\/span><\/span><\/sub>m<\/b><\/span><\/span>cometa<\/b><\/span><\/span><\/sub>\/d<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 como a dist\u00e2ncia entre eles varia, a for\u00e7a gravitacional tamb\u00e9m variar\u00e1 e ter\u00e1 intensidade m\u00ednima quando o cometa passa pelo seu af\u00e9lio e intensidade<\/b><\/span><\/span><\/p>\n

\"\"<\/p>\n

\u00a0m\u00e1xima quando passa pelo seu peri\u00e9lio conforme voc\u00ea pode observar na figura acima.<\/b><\/span><\/span><\/p>\n

R- A<\/b><\/span><\/span><\/p>\n

12-\u00a0<\/b><\/span><\/span><\/span>a)<\/b><\/span><\/span><\/span> Falsa\u00a0 —\u00a0 de acordo com a Lei de Newton da Gravita\u00e7\u00e3o, as for\u00e7as gravitacionais trocadas entre duas massas M e m, distantes r entre si, \u00e9\u00a0 —\u00a0 F=GMm\/r<\/b><\/span><\/span>2\u00a0\u00a0<\/b><\/span><\/span><\/sup>—\u00a0 onde G \u00e9 a constante de gravita\u00e7\u00e3o universal. \u00a0\u00a0—\u00a0 aplicando essa express\u00e3o para as duas situa\u00e7\u00f5es<\/b><\/span><\/span><\/p>\n

\"\"<\/p>\n

b)<\/b><\/span><\/span><\/span> Falsa\u00a0 —\u00a0 pela terceira lei de Kepler (lei dos per\u00edodos), o per\u00edodo orbital (T) s\u00f3 depende do raio (r) da \u00f3rbita\u00a0 —\u00a0 T<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>\u00a0= k r<\/b><\/span><\/span>3<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 \u00a0independe da massa do sat\u00e9lite.<\/b><\/span><\/span><\/p>\n

c)<\/b><\/span><\/span><\/span> Falsa\u00a0 —\u00a0 basta comparar os valores mostrados na tabela.<\/b><\/span><\/span><\/p>\n

d)<\/b><\/span><\/span><\/span> Falsa\u00a0 —\u00a0 \u00a0velocidade angular (W) \u00e9 inversamente proporcional ao per\u00edodo\u00a0 —\u00a0 W=2 \u03c0\/T.<\/b><\/span><\/span><\/p>\n

\"\"<\/p>\n

R- E<\/b><\/span><\/span><\/p>\n

 <\/p>\n

13-<\/b><\/span><\/span><\/span>\u00a0I. Correta\u00a0 —\u00a0 como a ma\u00e7\u00e3 est\u00e1 em equil\u00edbrio (repouso) presa ao galho a for\u00e7a resultante\u00a0\"\"\u00a0sobre ela deve ser nula e, para<\/b><\/span><\/span><\/p>\n

\"\"<\/p>\n

que isso ocorra seu peso\u00a0\"\"\u00a0(vertical e para baixo) dever ser anulado pela for\u00e7a de tra\u00e7\u00e3o\u00a0\"\"\u00a0no cabinho.<\/b><\/span><\/span><\/p>\n

II.<\/b><\/span><\/span><\/span> Falsa\u00a0 —\u00a0 sem atrito a ma\u00e7\u00e3 cai sujeita \u00e0 acelera\u00e7\u00e3o da gravidade g, independente de sua massa (P=m.g \u2013 g \u00e9 a mesma)\u00a0 —\u00a0 assim,\u00a0 desprezando-se os atritos,todos os corpos chegam com a mesma velocidade e ao mesmo tempo ao solo, independe de sua massa\u00a0 —\u00a0\u00a0 com atrito, a intensidade da for\u00e7a resultante sobre ela F<\/b><\/span><\/span>R<\/b><\/span><\/span><\/sub>=P \u2013 F<\/b><\/span><\/span>at<\/b><\/span><\/span><\/sub>=m.a.<\/b><\/span><\/span><\/p>\n

III.<\/b><\/span><\/span><\/span> Correta\u00a0 —\u00a0 trata-se do princ\u00edpio da a\u00e7\u00e3o e rea\u00e7\u00e3o (for\u00e7as trocadas entre o centro da Terra e a ma\u00e7\u00e3).<\/b><\/span><\/span><\/p>\n

R- C<\/b><\/span><\/span><\/p>\n

14-<\/b><\/span><\/span><\/span>Trata-se da lei da atra\u00e7\u00e3o universal de Newton de defini\u00e7\u00e3o \u201c Mat\u00e9ria atrai mat\u00e9ria na raz\u00e3o direta das massas e inversa ao quadrado da dist\u00e2ncia entre elas\u201d\u00a0 —\u00a0 sua express\u00e3o matem\u00e1tica \u00e9 F=GMm\/d2, onde G \u00e9 denominada constante de gravita\u00e7\u00e3o universal de Newton de valor aproximado G\u22486,7.10-11N.m2\/kg2\u00a0 —\u00a0 como G \u00e9 uma constante universal ela tem sempre esse mesmo valor independentemente dos corpos que est\u00e3o se atraindo e, \u00e9 claro que a raz\u00e3o pedida \u00e9 1.<\/b><\/span><\/span><\/p>\n

 <\/p>\n

15-<\/b><\/span><\/span><\/span>For\u00e7a gravitacional entre J\u00fapiter e Terra\u00a0 —\u00a0 F<\/b><\/span><\/span>G<\/b><\/span><\/span><\/sub>=G.m<\/b><\/span><\/span>J<\/b><\/span><\/span><\/sub>.m<\/b><\/span><\/span>T<\/b><\/span><\/span><\/sub>\/r<\/b><\/span><\/span>2<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 r=R<\/b><\/span><\/span>J<\/b><\/span><\/span><\/sub>\u00a0– R<\/b><\/span><\/span>T<\/b><\/span><\/span><\/sub>\u00a0= 7,5.10<\/b><\/span><\/span>11<\/b><\/span><\/span><\/sup>m \u2013 1,5.10<\/b><\/span><\/span>11<\/b><\/span><\/span><\/sup>m\u00a0 —\u00a0<\/b><\/span><\/span><\/p>\n

\"\"<\/p>\n

r=6,0.10<\/b><\/span><\/span>11<\/b><\/span><\/span><\/sup>m\u00a0 —F<\/b><\/span><\/span>G<\/b><\/span><\/span><\/sub>=6,7.10<\/b><\/span><\/span>-11<\/b><\/span><\/span><\/sup>.2,0.10<\/b><\/span><\/span>27<\/b><\/span><\/span><\/sup>.6,0.10<\/b><\/span><\/span>24<\/b><\/span><\/span><\/sup>\/6,0.10<\/b><\/span><\/span>11<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 F<\/b><\/span><\/span>G<\/b><\/span><\/span><\/sub>=80,4.10<\/b><\/span><\/span>40<\/b><\/span><\/span><\/sup>\/6,0.10<\/b><\/span><\/span>11<\/b><\/span><\/span><\/sup>\u00a0 —\u00a0 F<\/b><\/span><\/span>G<\/b><\/span><\/span><\/sub>=13,4.10<\/b><\/span><\/span>29<\/b><\/span><\/span><\/sup>\u00a0N\u00a0 —\u00a0 F<\/b><\/span><\/span>G<\/b><\/span><\/span><\/sub>=1,34.10<\/b><\/span><\/span>30<\/b><\/span><\/span><\/sup>\u00a0N\u00a0 —\u00a0\u00a0<\/b><\/span><\/span>R- D\u00a0<\/b><\/span><\/span>\u00a0\u00a0\u00a0<\/b><\/span><\/span><\/p>\n

 <\/p>\n

Voltar para os exerc\u00edcios<\/span><\/a><\/h3>\n","protected":false},"excerpt":{"rendered":"

Resolu\u00e7\u00f5es comentadas dos exerc\u00edcios de vestibulares sobre a Lei da \u00a0Gravita\u00e7\u00e3o Universal   01- GM=K (constante)\u00a0 —\u00a0 F=GMm\/R2\u00a0 —\u00a0 F1=Km\/R2\u00a0 —\u00a0 F2=K2m\/R2\u00a0 —\u00a0 F3=K8m\/R2\u00a0 —\u00a0 R- C 02- F=GMm\/R2\u00a0 —\u00a0 F\u2019=G2M2m\/R2\/4\u00a0 —\u00a0 16F=F\u2019\u00a0 —\u00a0 R- A 03- ms100mt\u00a0 —\u00a0\u00a0\u00a0\u00a0Fs=GMms\/Rs2\u00a0 —\u00a0 Ft=GMmt\/Rt2\u00a0 —\u00a0 Fs\/Ft=GMms\/Rs2x Rt2\/GMmt\u00a0 —\u00a0 Fs\/Ft=100mt.Rt2\/100Rt2.mt\u00a0 — Fs\/Ft=1 — R- C 04- mp\/ms=81\u00a0 —\u00a0 Fp=GMmp\/R2\u00a0 —\u00a0 Fs=GMms\/r2\u00a0 —\u00a0 Fp=Fs\u00a0 —\u00a0<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":1433,"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-1437","page","type-page","status-publish","hentry"],"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/fisicaevestibular.com.br\/novo\/wp-json\/wp\/v2\/pages\/1437","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=1437"}],"version-history":[{"count":4,"href":"https:\/\/fisicaevestibular.com.br\/novo\/wp-json\/wp\/v2\/pages\/1437\/revisions"}],"predecessor-version":[{"id":10879,"href":"https:\/\/fisicaevestibular.com.br\/novo\/wp-json\/wp\/v2\/pages\/1437\/revisions\/10879"}],"up":[{"embeddable":true,"href":"https:\/\/fisicaevestibular.com.br\/novo\/wp-json\/wp\/v2\/pages\/1433"}],"wp:attachment":[{"href":"https:\/\/fisicaevestibular.com.br\/novo\/wp-json\/wp\/v2\/media?parent=1437"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}