ࡱ> -, ɀ\puser Ba==hL,8X@"1Arial1Arial1Arial1Arial1 Arial1$Arial1 Arial1 Arial1Arial1Arial1Arial1Arial1 Arial1 Arial1Arial1@Arial1Arial1@Arial "R$ "#,##0_);\("R$ "#,##0\)% "R$ "#,##0_);[Red]\("R$ "#,##0\)&!"R$ "#,##0.00_);\("R$ "#,##0.00\)+&"R$ "#,##0.00_);[Red]\("R$ "#,##0.00\)=*8_("R$ "* #,##0_);_("R$ "* \(#,##0\);_("R$ "* "-"_);_(@_).))_(* #,##0_);_(* \(#,##0\);_(* "-"_);_(@_)E,@_("R$ "* #,##0.00_);_("R$ "* \(#,##0.00\);_("R$ "* "-"??_);_(@_)6+1_(* #,##0.00_);_(* \(#,##0.00\);_(* "-"??_);_(@_)"R$"#,##0_);\("R$"#,##0\)#"R$"#,##0_);[Red]\("R$"#,##0\)$"R$"#,##0.00_);\("R$"#,##0.00\))$"R$"#,##0.00_);[Red]\("R$"#,##0.00\):5_("R$"* #,##0_);_("R$"* \(#,##0\);_("R$"* "-"_);_(@_)B=_("R$"* #,##0.00_);_("R$"* \(#,##0.00\);_("R$"* "-"??_);_(@_) 0.000000E+00 0.0000000E+00 0.000 0.0000000 0.000000000 0.00000000000 0.0000                  , *  + )         # #            #  #                         "  ` vPlan1 6#Va R5Plan2 Y6Plan377  ;`ihcc =T =Ho =f =Ho' = Dados FixosDados VariaveisDados CalculadosVa =T1 =T2 =D1 =D1' =D3 =D3' =c1 =f ' =HzZ = bilhes de anos luzbilhes de anos= c*( f - f ') / f%=raiz(( 1 + (Va/c))/(1 - (Va/c))) - 1= T - T2= Va / (c * Ho' ) = Va * T1 = c1 * T2= c * T2 = Va / Ho'= c - Vaunidade de velocidadeKm/s/Mpo= Ho/(300000*0,00326)f '=D1 '=D3 '==raiz((1+Va/c)/(1-(Va/c)))-1=((1+Z)^2-1)/((1+Z)^2+1)= f*(1-(Va/c))=T-T2 =Va/(c*Ho' )=Va*T1= c1*T2= c*T2 = Va/Ho'=c-VaZ =R ==c x T=Va*TD3''=Galxia:= =3e08*c1/=Va x T=Va x T2 = Va x T1Km/s/Mpc[ 1 ][ 2 ][ 3 ][ 4 ][ 5 ][ 6 ][ 7 ][ 8 ][ 9 ][ 10 ][ 11 ][ 12 ][ 13 ][ 14 ][ 15 ][ 16 ][ 17 ]Va = T2 = c1 = T1 = CDFh:[SAG99]GD10 Clculos:,Planilha do Universo Visvel entrando com Va+D =D1 = D3 = Velocidade da LuzIdade do UniversoFrequencia da luz na emisso5Velocidade de afastamento entre a galxia P e a Terra Redshift 0Distncia entre a Terra e a galxia P atualmente%Frequencia da luz ao chegar na terra Constante de Hubble?Tempo gasto pelo fton e pelo raio de luz para alcanar a Terra'Velocidade de chegada do fton na TerraDDistncia entre a Terra e a galxia P na poca da emisso dos ftonsRaio do Universo Visvel6Distncia percorrida pela galxia P da poso P1 at P2Idade do Universo na ocasio de emisso dos ftons= (Va/D) * (300000*0,00326)=D/cComprimento da onda da luzmjr Q }  t[]; G ɀ $"  dMbP?_*+%MHP DeskJet 690C Series v11.0:d,,HP DeskJet 690C Series v11.0LPT1 ,,"d,,~?~?U} } I} } m} } I} } }                         ~  ?  ~  @   hQ@  !k[hB  06J?DOAQ,j? !   " > B  ~  @    wFmx?        .`{x?DDD D   =?x?'D D  & /@;@*D DD DA % @z@*DDDDA  "-DA BDDD ' "-> BDD D '    !_N? DD   !Q? DD (  !*O? DD (    (i4)@DDD   (4)@DDD )  (P4)@D DD )    !|5h? DD   !͛h? DD *  !3h? D D *    ! h? DD  #!dϥh? DD + #!h? DD +   !i4)@ DD  !4)@ DD , !P4)@ DD ,   !i4)@ DD  $!4)@ DD - $!P4)@ D D -   !:@x? DD  !|? DD . 3! 4)@ D D 2   0!+@ DD 1 !+y? DD  .  . **..Px* >@7 ɀ ,'4  dMbP?_*+%M6\\gravidade\HP DeskJet 695CXC 4d,,A4DINU"4$H$$$$"P,,~?~?U} I} IM} } } } I} } I} } } } I  v@ ; ; ; ; ; ; ; ; ; ; w ; ; ; ; w w w w w ; ; w ; ; ; ; ; ; ; 5R55555# ##$ & #%###$##%# #; #V $~ '? #%#$'# #< #W $~ 'h@ #%#$'# #= #X $(C #%#$(# #> #f $5(ɿ > #g %###$##%# ##$ & #%# 44$ &4 #P %+ ##$&#%+ #? #Y $L ''s? # ## 6Q 66666# ##$,### #@ #Z $/@-ةoQ?#*D DD DA *% # #$1 #A #[ $S!)Kp @ D D *7 ## #B #^ $M!.Kp @ DD *e # #$2 * #C #_ $N!.^p? DD  *. # #$/  *# #D #` $T!/.[t @ DD *+ # #$/  *# #E #b $U!/C,v@ D D *8 # #$/  *# #F #c $O!/62@ DD *( # #$/  *# #G #\ $"-3d4BDD D *' # #$/  *# #H #a $0!/ffffff+@ DD *1 # #$/  *# #I #` $T!0.[t @ D D *9 # #$.  *# #J #\ $"+3oBADD *6 # #$/  *# #K #] $70UQ@!D DOAQ,j? *d #: #$/  *# ##$0*%#$.  *# ##$##%#$/  *# ##$)*%###$##%###$##%#B X$.ZZ^X.:Z&**">@ 7 ɀ  6  dMbP?_*+%" ~?~?U>@7 ɀ 7  dMbP?_*+%"~?~?U>@7 Oh+'0HP`l GERALDO.RAMicrosoft Excel@wOG@b[@0՜.+,0 PXh px SISTOPn Plan1VaPlan2Plan3  Planilhas  !"#%&'()*+Root Entry FɁ~Workbook`7SummaryInformation(DocumentSummaryInformation8$