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	<title>Words&#039; of Physic</title>
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		<title>Energia Cin&#233;tica!</title>
		<link>http://wordsofphysic.wordpress.com/2010/02/16/energia-cintica/</link>
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		<pubDate>Tue, 16 Feb 2010 17:07:55 +0000</pubDate>
		<dc:creator>Tiago Portela</dc:creator>
				<category><![CDATA[Newton]]></category>
		<category><![CDATA[dedução]]></category>
		<category><![CDATA[energia cinetica]]></category>

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		<description><![CDATA[Bem hoje não estou com muita vontade de escrever por isso vou os apresentar uma dedução simples da formula para calcular a energia cinética Newtoniana. Sabemos que o trabalho de uma força é dado por: Diferenciando a expressão: &#160;&#160; Como Integrando:<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=wordsofphysic.wordpress.com&amp;blog=10243983&amp;post=455&amp;subd=wordsofphysic&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<p>Bem hoje não estou com muita vontade de escrever por isso vou os apresentar uma dedução simples da formula para calcular a energia cinética Newtoniana.</p>
<p>Sabemos que o trabalho de uma força é dado por:</p>
<p><img src='http://s0.wp.com/latex.php?latex=W%3D%5Cint_%7BA%7D%5E%7BB%7DFdx&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='W=&#92;int_{A}^{B}Fdx' title='W=&#92;int_{A}^{B}Fdx' class='latex' /></p>
<p>Diferenciando a expressão:</p>
<p><img src='http://s0.wp.com/latex.php?latex=dW%3Dd%28%5Cint_%7BA%7D%5E%7BB%7DFdx%29&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='dW=d(&#92;int_{A}^{B}Fdx)' title='dW=d(&#92;int_{A}^{B}Fdx)' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=dW%3DFdx&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='dW=Fdx' title='dW=Fdx' class='latex' />&#160;&#160; Como <img src='http://s0.wp.com/latex.php?latex=%5Cfrac%7Bdx%7D%7Bdt%7D%3Dv&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;frac{dx}{dt}=v' title='&#92;frac{dx}{dt}=v' class='latex' /> <img src='http://s0.wp.com/latex.php?latex=%5CLeftrightarrow+d%7Bx%7D%3Dv+d%7Bt%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;Leftrightarrow d{x}=v d{t}' title='&#92;Leftrightarrow d{x}=v d{t}' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=dW%3DFvdt&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='dW=Fvdt' title='dW=Fvdt' class='latex' /> <img src='http://s0.wp.com/latex.php?latex=F%3Dma%3Dm%5Cfrac%7Bdv%7D%7Bdt%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='F=ma=m&#92;frac{dv}{dt}' title='F=ma=m&#92;frac{dv}{dt}' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=dW%3Dm%5Cfrac%7Bdv%7D%7Bdt%7Dvdt&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='dW=m&#92;frac{dv}{dt}vdt' title='dW=m&#92;frac{dv}{dt}vdt' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=dW%3Dmvdv&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='dW=mvdv' title='dW=mvdv' class='latex' /> Integrando:</p>
<p><img src='http://s0.wp.com/latex.php?latex=%5Cint+dW%3D%5Cint+mvdv&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;int dW=&#92;int mvdv' title='&#92;int dW=&#92;int mvdv' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=E_c%3D%5Cfrac%7B1%7D%7B2%7Dmv%5E2&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='E_c=&#92;frac{1}{2}mv^2' title='E_c=&#92;frac{1}{2}mv^2' class='latex' /></p>
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		<title>Marca Words&#8217; of Physic</title>
		<link>http://wordsofphysic.wordpress.com/2010/02/11/marca-words-of-physic/</link>
		<comments>http://wordsofphysic.wordpress.com/2010/02/11/marca-words-of-physic/#comments</comments>
		<pubDate>Thu, 11 Feb 2010 18:20:20 +0000</pubDate>
		<dc:creator>Tiago Portela</dc:creator>
				<category><![CDATA[Outros]]></category>
		<category><![CDATA[blog de fisica]]></category>
		<category><![CDATA[fisica]]></category>
		<category><![CDATA[logotipo]]></category>
		<category><![CDATA[marca]]></category>
		<category><![CDATA[words of physic]]></category>

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		<description><![CDATA[Hoje apresento-vos o logótipo do Esta imagem passará a representar a marca&#160; em todas as suas actividades.<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=wordsofphysic.wordpress.com&amp;blog=10243983&amp;post=449&amp;subd=wordsofphysic&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<p>Hoje apresento-vos o logótipo do <img src='http://s0.wp.com/latex.php?latex=Words%60%5C%2Cof%5C%2CPhysic&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='Words`&#92;,of&#92;,Physic' title='Words`&#92;,of&#92;,Physic' class='latex' /> </p>
<p><a href="http://wordsofphysic.files.wordpress.com/2010/02/logoblog1.jpg"><img title="logoblog" style="border-right:0;border-top:0;display:block;float:none;margin-left:auto;border-left:0;margin-right:auto;border-bottom:0;" height="345" alt="logoblog" src="http://wordsofphysic.files.wordpress.com/2010/02/logoblog_thumb.jpg?w=345&#038;h=345" width="345" border="0" /></a>Esta imagem passará a representar a marca&#160; <img src='http://s0.wp.com/latex.php?latex=Words%60%5C%2Cof%5C%2CPhysic&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='Words`&#92;,of&#92;,Physic' title='Words`&#92;,of&#92;,Physic' class='latex' /> em todas as suas actividades.</p>
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		<title>Einstein disse &#8220;E=mc^2&#8221;!</title>
		<link>http://wordsofphysic.wordpress.com/2010/02/08/einstein-disse-emc2/</link>
		<comments>http://wordsofphysic.wordpress.com/2010/02/08/einstein-disse-emc2/#comments</comments>
		<pubDate>Mon, 08 Feb 2010 21:10:16 +0000</pubDate>
		<dc:creator>Tiago Portela</dc:creator>
				<category><![CDATA[relatividade]]></category>
		<category><![CDATA[dedução]]></category>
		<category><![CDATA[deução e=mc^2]]></category>
		<category><![CDATA[E=mc^2]]></category>
		<category><![CDATA[einstein]]></category>

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		<description><![CDATA[Olá hoje irei apresentar uma dedução da equação . &#160; A força e dada por: [1] Como segundo a relatividade: Aplicando em [1] Como W=E E assim chegamos a mais famosa equação da física.<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=wordsofphysic.wordpress.com&amp;blog=10243983&amp;post=433&amp;subd=wordsofphysic&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<p>Olá hoje irei apresentar uma dedução da equação <img src='http://s0.wp.com/latex.php?latex=E%3Dmc%5E2&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='E=mc^2' title='E=mc^2' class='latex' />.</p>
<p>&#160;</p>
<p>A força e dada por:</p>
<p><img src='http://s0.wp.com/latex.php?latex=F%3D%5Cfrac%7Bdp%7D%7Bdt%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='F=&#92;frac{dp}{dt}' title='F=&#92;frac{dp}{dt}' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=F+%3D+%5Cfrac%7Bd%28mv%29%7D%7Bdt%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='F = &#92;frac{d(mv)}{dt}' title='F = &#92;frac{d(mv)}{dt}' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=F+%3D+%5Cfrac%7Bd%28m%29%7D%7Bdt%7Dv%2B%5Cfrac%7Bdv%7D%7Bdt%7Dm&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='F = &#92;frac{d(m)}{dt}v+&#92;frac{dv}{dt}m' title='F = &#92;frac{d(m)}{dt}v+&#92;frac{dv}{dt}m' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=F%3D%5Cfrac%7Bdmv%2Bdvm%7D%7Bdt%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='F=&#92;frac{dmv+dvm}{dt}' title='F=&#92;frac{dmv+dvm}{dt}' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=W%3D%5Cint+%28Fdx%29%5C%2C%5C%2C%5C%2C%5C%2C%5C%2C%5C%2C%5C%2C%5C%2C%5C%2C%5C%2C%5C%2CComo%5C%2C%5Cfrac%7Bdx%7D%7Bdt%7D%3Dv+%5CLeftrightarrow+dx%3Dvdt&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='W=&#92;int (Fdx)&#92;,&#92;,&#92;,&#92;,&#92;,&#92;,&#92;,&#92;,&#92;,&#92;,&#92;,Como&#92;,&#92;frac{dx}{dt}=v &#92;Leftrightarrow dx=vdt' title='W=&#92;int (Fdx)&#92;,&#92;,&#92;,&#92;,&#92;,&#92;,&#92;,&#92;,&#92;,&#92;,&#92;,Como&#92;,&#92;frac{dx}{dt}=v &#92;Leftrightarrow dx=vdt' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=W%3D%5Cint%28%5Cfrac%7Bdmv%2Bdvm%7D%7Bdt%7D+vdt%29&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='W=&#92;int(&#92;frac{dmv+dvm}{dt} vdt)' title='W=&#92;int(&#92;frac{dmv+dvm}{dt} vdt)' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=W%3D%5Cint%28dmv%2Bdvm%29v&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='W=&#92;int(dmv+dvm)v' title='W=&#92;int(dmv+dvm)v' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=W%3D%5Cint%28dmv%5E2%2Bdvmv%29&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='W=&#92;int(dmv^2+dvmv)' title='W=&#92;int(dmv^2+dvmv)' class='latex' /> [1]</p>
<p>Como segundo a relatividade:</p>
<p><img src='http://s0.wp.com/latex.php?latex=m%3D%5Cdisplaystyle+%5Cfrac%7Bm_0%7D%7B%5Csqrt%7B1-%28v%2Fc%29%5E2%7D%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='m=&#92;displaystyle &#92;frac{m_0}{&#92;sqrt{1-(v/c)^2}}' title='m=&#92;displaystyle &#92;frac{m_0}{&#92;sqrt{1-(v/c)^2}}' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=%5Csqrt%7B1-%28v%2Fc%29%5E2%7Dm%3Dm_0&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;sqrt{1-(v/c)^2}m=m_0' title='&#92;sqrt{1-(v/c)^2}m=m_0' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=m%5E2%281-%28v%2Fc%29%5E2%29%3Dm_0%5E2&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='m^2(1-(v/c)^2)=m_0^2' title='m^2(1-(v/c)^2)=m_0^2' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=c%5E2m%5E2-m%5E2v%5E2%3Dm_0%5E2c%5E2&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='c^2m^2-m^2v^2=m_0^2c^2' title='c^2m^2-m^2v^2=m_0^2c^2' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=d%28c%5E2m%5E2-m%5E2v%5E2%29%3Dd%28m_0%5E2c%5E2%29&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='d(c^2m^2-m^2v^2)=d(m_0^2c^2)' title='d(c^2m^2-m^2v^2)=d(m_0^2c^2)' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=c%5E22mdm-2mv%5E2dm-2vm%5E2dv%3D0&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='c^22mdm-2mv^2dm-2vm^2dv=0' title='c^22mdm-2mv^2dm-2vm^2dv=0' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=c%5E2dm-v%5E2dm-vmdv%3D0&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='c^2dm-v^2dm-vmdv=0' title='c^2dm-v^2dm-vmdv=0' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=c%5E2dm%3Dv%5E2dm%2Bvmdv&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='c^2dm=v^2dm+vmdv' title='c^2dm=v^2dm+vmdv' class='latex' /></p>
<p>Aplicando em [1]</p>
<p><img src='http://s0.wp.com/latex.php?latex=W%3D%5Cint%28c%5E2dm%29&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='W=&#92;int(c^2dm)' title='W=&#92;int(c^2dm)' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=W%3Dc%5E2m&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='W=c^2m' title='W=c^2m' class='latex' /> Como W=E</p>
<p><img src='http://s0.wp.com/latex.php?latex=E%3Dmc%5E2&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='E=mc^2' title='E=mc^2' class='latex' /></p>
<p>E assim chegamos a mais famosa equação da física.</p>
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		<title>Porque n&#227;o se pode alcan&#231;ar a velocidade da luz?</title>
		<link>http://wordsofphysic.wordpress.com/2010/01/29/porque-no-se-pode-alcanar-a-velocidade-da-luz/</link>
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		<pubDate>Fri, 29 Jan 2010 14:23:37 +0000</pubDate>
		<dc:creator>Tiago Portela</dc:creator>
				<category><![CDATA[relatividade]]></category>
		<category><![CDATA[E=mc^2]]></category>
		<category><![CDATA[einstein]]></category>
		<category><![CDATA[energia infinita]]></category>
		<category><![CDATA[física moderna]]></category>
		<category><![CDATA[velocidade da luz]]></category>

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		<description><![CDATA[Como este ano(para o ) é dedicado a Albert Einstein, deixo-vos aqui mais um post sobre relatividade. Porque não se pode alcançar a velocidade da luz? &#160; Segundo a relatividade restrita a massa varia em função da velocidade segundo a função: Estudando a função e fazendo a velocidade tender para a velocidade da luz(c). [1] [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=wordsofphysic.wordpress.com&amp;blog=10243983&amp;post=425&amp;subd=wordsofphysic&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<p>Como este ano(para o <img src='http://s0.wp.com/latex.php?latex=Words%27%5C%3Aof%5C%3APhysic&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='Words&#039;&#92;:of&#92;:Physic' title='Words&#039;&#92;:of&#92;:Physic' class='latex' />) é dedicado a Albert Einstein, deixo-vos aqui mais um post sobre relatividade.</p>
<p><strong><em>Porque não se pode alcançar a velocidade da luz?</em></strong></p>
<p><a href="http://wordsofphysic.files.wordpress.com/2010/01/image5.png"><img title="image" style="border-right:0;border-top:0;display:inline;border-left:0;border-bottom:0;" height="335" alt="image" src="http://wordsofphysic.files.wordpress.com/2010/01/image_thumb5.png?w=252&#038;h=335" width="252" border="0" /></a>&#160; </p>
<p>Segundo a relatividade restrita a massa varia em função da velocidade segundo a função:</p>
<p><img src='http://s0.wp.com/latex.php?latex=m%28v%29%3Dm_0%5Cfrac%7B1%7D%7B%5Csqrt%7B1-v%5E2%2Fc%5E2%7D%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='m(v)=m_0&#92;frac{1}{&#92;sqrt{1-v^2/c^2}}' title='m(v)=m_0&#92;frac{1}{&#92;sqrt{1-v^2/c^2}}' class='latex' /></p>
<p>Estudando a função e fazendo a velocidade tender para a velocidade da luz(c).</p>
<p><img src='http://s0.wp.com/latex.php?latex=%5Cdisplaystyle+%5Clim_%7Bv+%5Cto+c%7Dm%28v%29%3D%5Clim_%7Bv+%5Cto+c%7D%28m_0%5Cfrac%7B1%7D%7B%5Csqrt%7B1-v%5E2%2Fc%5E2%7D%7D%29&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;displaystyle &#92;lim_{v &#92;to c}m(v)=&#92;lim_{v &#92;to c}(m_0&#92;frac{1}{&#92;sqrt{1-v^2/c^2}})' title='&#92;displaystyle &#92;lim_{v &#92;to c}m(v)=&#92;lim_{v &#92;to c}(m_0&#92;frac{1}{&#92;sqrt{1-v^2/c^2}})' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=%5CRightarrow+m_0%5Cfrac%7B1%7D%7B%5Csqrt%7B1-c%5E2%2Fc%5E2%7D%7D%29%3D%5Cfrac%7Bm_0%7D%7B0%7D%3D%5Cinfty&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;Rightarrow m_0&#92;frac{1}{&#92;sqrt{1-c^2/c^2}})=&#92;frac{m_0}{0}=&#92;infty' title='&#92;Rightarrow m_0&#92;frac{1}{&#92;sqrt{1-c^2/c^2}})=&#92;frac{m_0}{0}=&#92;infty' class='latex' /> [1]</p>
<p>Segundo a equivalência de massa energia.</p>
<p><img src='http://s0.wp.com/latex.php?latex=E%3Dmc%5E2&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='E=mc^2' title='E=mc^2' class='latex' />; substituindo [1]</p>
<p><img src='http://s0.wp.com/latex.php?latex=E%3D%5Cinfty+%5Ctimes+c%5E2&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='E=&#92;infty &#92;times c^2' title='E=&#92;infty &#92;times c^2' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=%5CLeftrightarrow+E%3D%5Cinfty+&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;Leftrightarrow E=&#92;infty ' title='&#92;Leftrightarrow E=&#92;infty ' class='latex' /></p>
<p>Como não existe energia infinita no Universo inteiro concluímos que nada pode atingir a velocidade da luz. </p>
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		<title>Ser&#225; que o Pai Natal existe?</title>
		<link>http://wordsofphysic.wordpress.com/2010/01/27/ser-que-o-pai-natal-existe/</link>
		<comments>http://wordsofphysic.wordpress.com/2010/01/27/ser-que-o-pai-natal-existe/#comments</comments>
		<pubDate>Wed, 27 Jan 2010 23:37:55 +0000</pubDate>
		<dc:creator>Tiago Portela</dc:creator>
				<category><![CDATA[Lei dos movimentos.]]></category>
		<category><![CDATA[Outros]]></category>
		<category><![CDATA[fisica do pai natal]]></category>
		<category><![CDATA[o pai natal existe]]></category>
		<category><![CDATA[pai natal]]></category>
		<category><![CDATA[viagem]]></category>

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		<description><![CDATA[Olá hoje irei analisar “fisicamente” o Pai Natal! 1 – As crianças. Existem aproximadamente 2 biliões de crianças (pessoas com menos de 18 anos). Como o Pai Natal é católico e não visita crianças de outras religiões restam-nos 378 milhões de crianças. Segundo os censos existem cerca de 4 crianças em cada lar logo: de [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=wordsofphysic.wordpress.com&amp;blog=10243983&amp;post=417&amp;subd=wordsofphysic&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<p>Olá hoje irei analisar “fisicamente” o Pai Natal!</p>
<p><a href="http://wordsofphysic.files.wordpress.com/2010/01/image4.png"><img title="image" style="border-right:0;border-top:0;display:inline;border-left:0;border-bottom:0;" height="330" alt="image" src="http://wordsofphysic.files.wordpress.com/2010/01/image_thumb4.png?w=314&#038;h=330" width="314" border="0" /></a></p>
<p>1 – <em>As crianças.</em></p>
<p>Existem aproximadamente 2 biliões de crianças (pessoas com menos de 18 anos).</p>
<p>Como o Pai Natal é católico e não visita crianças de outras religiões restam-nos 378 milhões de crianças. </p>
<p>Segundo os censos existem cerca de 4 crianças em cada lar logo:</p>
<p><img src='http://s0.wp.com/latex.php?latex=%5Cfrac%7B378000000%7D%7B4%7D%3D94500000&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;frac{378000000}{4}=94500000' title='&#92;frac{378000000}{4}=94500000' class='latex' /> de lares.</p>
<p>2- <em>Tempo.</em></p>
<p>Devido ao fuso-horário e á rotação da Terra o Pai Natal têm cerca de 31 horas para entregar todos os presentes.</p>
<p><img src='http://s0.wp.com/latex.php?latex=31%5C%3Ah%3D31%5Ctimes+60%5Ctimes+60%5C%3As%3D111600%5C%3As&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='31&#92;:h=31&#92;times 60&#92;times 60&#92;:s=111600&#92;:s' title='31&#92;:h=31&#92;times 60&#92;times 60&#92;:s=111600&#92;:s' class='latex' /></p>
<p>Assim se dividirmos o numero de lares pelo tempo que ele têm para entregar os presentes teremos o número de visitas por segundo.</p>
<p><img src='http://s0.wp.com/latex.php?latex=%5Cfrac%7B94500000%7D%7B111600%7D%3D847%5C%3Avisitas%2Fsegundo&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;frac{94500000}{111600}=847&#92;:visitas/segundo' title='&#92;frac{94500000}{111600}=847&#92;:visitas/segundo' class='latex' /></p>
<p>E também que ele só poderá dispender 0.001 segundos para sair do trenó, descer pela chaminé, colocar o presente e voltar ao trenó</p>
<p>3- <em>Velocidade </em></p>
<p>Admitindo que as casas se encontram uniformemente distribuídas(o que é falso mas é aceitável para a simplificação dos cálculos) e que o Pai Natal só entrega os presentes nos continentes europeu e americano, podemos calcular a distancia entre cada lar.</p>
<p>Área da Europa + Área da América = Área total</p>
<p><img src='http://s0.wp.com/latex.php?latex=10498000%2B42189120%3D+52687120%5Cquad+Km&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='10498000+42189120= 52687120&#92;quad Km' title='10498000+42189120= 52687120&#92;quad Km' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=%5Cfrac%7B94500000%7D%7B52687120%7D%3D1.8%5C%3Acasas%2FKm&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;frac{94500000}{52687120}=1.8&#92;:casas/Km' title='&#92;frac{94500000}{52687120}=1.8&#92;:casas/Km' class='latex' /></p>
<p>Assim </p>
<p><img src='http://s0.wp.com/latex.php?latex=distancia%5C%3Apercorrida%3D1.8%5Ctimes+94500000%3D1.8%5Ctimes10%5E8%5Cquad+km&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='distancia&#92;:percorrida=1.8&#92;times 94500000=1.8&#92;times10^8&#92;quad km' title='distancia&#92;:percorrida=1.8&#92;times 94500000=1.8&#92;times10^8&#92;quad km' class='latex' /></p>
<p>Como <img src='http://s0.wp.com/latex.php?latex=R_m%3D%5Cfrac%7Bd%7D%7B%5CDelta%7Bt%7D%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='R_m=&#92;frac{d}{&#92;Delta{t}}' title='R_m=&#92;frac{d}{&#92;Delta{t}}' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=%5CRightarrow+%5Cfrac%7B1.8%5Ctimes10%5E8%7D%7B111600%7D%3D1524.2%5Cquad+km%2Fs&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;Rightarrow &#92;frac{1.8&#92;times10^8}{111600}=1524.2&#92;quad km/s' title='&#92;Rightarrow &#92;frac{1.8&#92;times10^8}{111600}=1524.2&#92;quad km/s' class='latex' /></p>
<p>Como num movimento uniforme onde não existe inversão do sentido a rapidez media é igual a velocidade:</p>
<p><img src='http://s0.wp.com/latex.php?latex=v%3D1524200%5Cquad+m%2Fs&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='v=1524200&#92;quad m/s' title='v=1524200&#92;quad m/s' class='latex' /> Assim ele teria de viajar a uma velocidade muito superior ao veiculo mais rápido construído pelo Homem, a sonda espacial Ulisses,   <br />move-se a acanhados 44100 m/s, e uma rena “normal” anda no máximo a 24km/h.</p>
<p>4- <em>Força</em></p>
<p>Ele viaja a uma velocidade de 1524200 m/s e para ele parar será aplicada uma aceleração contraria ao movimento logo</p>
<p><img src='http://s0.wp.com/latex.php?latex=v%3Dv_0-at&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='v=v_0-at' title='v=v_0-at' class='latex' /> Como pára para v=0</p>
<p><img src='http://s0.wp.com/latex.php?latex=v_0%3Dat&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='v_0=at' title='v_0=at' class='latex' />;&#160; <img src='http://s0.wp.com/latex.php?latex=v_0%3D1.5%5Ctimes+10%5E6&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='v_0=1.5&#92;times 10^6' title='v_0=1.5&#92;times 10^6' class='latex' /> e <img src='http://s0.wp.com/latex.php?latex=t%3D0.001%5C%3A+segundos&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='t=0.001&#92;: segundos' title='t=0.001&#92;: segundos' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=a%3D1.5%5Ctimes+10%5E9%5Cquad+m%2Fs%5E2+&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='a=1.5&#92;times 10^9&#92;quad m/s^2 ' title='a=1.5&#92;times 10^9&#92;quad m/s^2 ' class='latex' /></p>
<p>Admitindo que o Pai Natal tem uma massa de 150 Kg</p>
<p><img src='http://s0.wp.com/latex.php?latex=F_r%3Dma%3D1.5%5Ctimes+10%5E9+%5Ctimes+150%3D228630000000%5Cquad+N+&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='F_r=ma=1.5&#92;times 10^9 &#92;times 150=228630000000&#92;quad N ' title='F_r=ma=1.5&#92;times 10^9 &#92;times 150=228630000000&#92;quad N ' class='latex' /></p>
<p>Com uma força destas o Pai Natal seria esmagado completamente.</p>
<p>4-<em>Conclusão.</em></p>
<p>Se o Pai Natal existiu está morto.</p>
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		<title>A ma&#231;&#227; de Newton!</title>
		<link>http://wordsofphysic.wordpress.com/2010/01/24/a-ma-de-newton/</link>
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		<pubDate>Sun, 24 Jan 2010 01:35:07 +0000</pubDate>
		<dc:creator>Tiago Portela</dc:creator>
				<category><![CDATA[gravitação]]></category>
		<category><![CDATA[dedução]]></category>
		<category><![CDATA[dedução da equação da gravidade]]></category>
		<category><![CDATA[força centripta]]></category>
		<category><![CDATA[lei universal da gravidade]]></category>
		<category><![CDATA[Newton]]></category>

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		<description><![CDATA[Olá hoje irei publicar um artigo com a dedução da famosa equação da gravidade elaborada por Issac Newton. Uma maneira prática de o fazer e estudar o movimento dos planetas. Vermelho Estrela A Verde Planeta B ; Usando a 3º Lei de Kepler: substituindo: [1] Como Assim concluísse que é constante para quaisquer corpos em [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=wordsofphysic.wordpress.com&amp;blog=10243983&amp;post=403&amp;subd=wordsofphysic&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<p>Olá hoje irei publicar um artigo com a dedução da famosa equação da gravidade elaborada por Issac Newton.</p>
<p><a href="http://wordsofphysic.files.wordpress.com/2010/01/image3.png"><img style="display:inline;border:0;" title="image" src="http://wordsofphysic.files.wordpress.com/2010/01/image_thumb3.png?w=365&#038;h=245" border="0" alt="image" width="365" height="245" /></a></p>
<p>Uma maneira prática de o fazer e estudar o movimento dos planetas.</p>
<p><a href="http://wordsofphysic.files.wordpress.com/2010/01/tr.png"><img class="alignnone" style="border:0 none;display:inline;margin-left:0;margin-right:0;" title="tr" src="http://wordsofphysic.files.wordpress.com/2010/01/tr_thumb.png?w=328&#038;h=253" border="0" alt="tr" width="328" height="253" align="left" /></a></p>
<p>Vermelho Estrela A</p>
<p>Verde Planeta B</p>
<p><img src='http://s0.wp.com/latex.php?latex=F_%7BresultanteA%2FB%7D%3DFc&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='F_{resultanteA/B}=Fc' title='F_{resultanteA/B}=Fc' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=%5CRightarrow+F_%7BresultanteA%2FB%7D%3D%3Dm_B%5Cfrac%7Bv%5E2%7D%7Br%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;Rightarrow F_{resultanteA/B}==m_B&#92;frac{v^2}{r}' title='&#92;Rightarrow F_{resultanteA/B}==m_B&#92;frac{v^2}{r}' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=%5CLeftrightarrow+F_%7BresultanteA%2FB%7D%3Dm_B%5Cfrac%7B4%5Cpi%5E2r%7D%7BT%5E2%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;Leftrightarrow F_{resultanteA/B}=m_B&#92;frac{4&#92;pi^2r}{T^2}' title='&#92;Leftrightarrow F_{resultanteA/B}=m_B&#92;frac{4&#92;pi^2r}{T^2}' class='latex' />; <img src='http://s0.wp.com/latex.php?latex=v%5E2%3D%5Comega%5E2r%5E2&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='v^2=&#92;omega^2r^2' title='v^2=&#92;omega^2r^2' class='latex' /></p>
<p>Usando a 3º Lei de Kepler:</p>
<p><img src='http://s0.wp.com/latex.php?latex=%5Cfrac%7Br%5E3%7D%7BT%5E2%7D%3DK&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;frac{r^3}{T^2}=K' title='&#92;frac{r^3}{T^2}=K' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=%5CLeftrightarrow+T%5E2%3D%5Cfrac%7Br%5E3%7D%7BK%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;Leftrightarrow T^2=&#92;frac{r^3}{K}' title='&#92;Leftrightarrow T^2=&#92;frac{r^3}{K}' class='latex' /> substituindo:</p>
<p><img src='http://s0.wp.com/latex.php?latex=F_%7BresultanteA%2FB%7D%3D%5Cfrac%7B4%5Cpi%5E2rK_A%7D%7Br%5E3%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='F_{resultanteA/B}=&#92;frac{4&#92;pi^2rK_A}{r^3}' title='F_{resultanteA/B}=&#92;frac{4&#92;pi^2rK_A}{r^3}' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=%5CLeftrightarrow+F_%7BresultanteA%2FB%7D%3D%5Cfrac%7B4%5Cpi%5E2K_A%7D%7Br%5E2%7Dm_B&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;Leftrightarrow F_{resultanteA/B}=&#92;frac{4&#92;pi^2K_A}{r^2}m_B' title='&#92;Leftrightarrow F_{resultanteA/B}=&#92;frac{4&#92;pi^2K_A}{r^2}m_B' class='latex' /> [1]</p>
<p>Como <img src='http://s0.wp.com/latex.php?latex=%7CF_%7BresultanteA%2FB%7D%7C%3D%7CF_%7BresultanteB%2FA%7D%7C&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='|F_{resultanteA/B}|=|F_{resultanteB/A}|' title='|F_{resultanteA/B}|=|F_{resultanteB/A}|' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=%5CLeftrightarrow+%5Cfrac%7B4%5Cpi%5E2K%7D%7Br%5E2%7Dm_B%3D%5Cfrac%7B4%5Cpi%5E2K%7D%7Br%5E2%7Dm_A&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;Leftrightarrow &#92;frac{4&#92;pi^2K}{r^2}m_B=&#92;frac{4&#92;pi^2K}{r^2}m_A' title='&#92;Leftrightarrow &#92;frac{4&#92;pi^2K}{r^2}m_B=&#92;frac{4&#92;pi^2K}{r^2}m_A' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=%5CLeftrightarrow+%5Cfrac%7B4%5Cpi%5E2K_A%7D%7Bm_A%7D%3D%5Cfrac%7B4%5Cpi%5E2K_B%7D%7Bm_B%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;Leftrightarrow &#92;frac{4&#92;pi^2K_A}{m_A}=&#92;frac{4&#92;pi^2K_B}{m_B}' title='&#92;Leftrightarrow &#92;frac{4&#92;pi^2K_A}{m_A}=&#92;frac{4&#92;pi^2K_B}{m_B}' class='latex' /></p>
<p>Assim concluísse que <img src='http://s0.wp.com/latex.php?latex=%5Cfrac%7B4%5Cpi%5E2K_A%7D%7Bm_A%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;frac{4&#92;pi^2K_A}{m_A}' title='&#92;frac{4&#92;pi^2K_A}{m_A}' class='latex' /> é constante para quaisquer corpos em interacção gravitacional sendo esta constante <img src='http://s0.wp.com/latex.php?latex=G&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='G' title='G' class='latex' /></p>
<p>Logo:</p>
<p><img src='http://s0.wp.com/latex.php?latex=%5Cfrac%7B4%5Cpi%5E2K_A%7D%7Bm_A%7D%3DG&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;frac{4&#92;pi^2K_A}{m_A}=G' title='&#92;frac{4&#92;pi^2K_A}{m_A}=G' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=4%5Cpi%5E2K_A%3DGm_A&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='4&#92;pi^2K_A=Gm_A' title='4&#92;pi^2K_A=Gm_A' class='latex' /> Substituindo em [1]:</p>
<p><img src='http://s0.wp.com/latex.php?latex=%5CLeftrightarrow+F_%7BresultanteA%2FB%7D%3DG%5Cfrac%7Bm_A+m_B%7D%7Br%5E2%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;Leftrightarrow F_{resultanteA/B}=G&#92;frac{m_A m_B}{r^2}' title='&#92;Leftrightarrow F_{resultanteA/B}=G&#92;frac{m_A m_B}{r^2}' class='latex' /></p>
<p>E assim chegamos a Lei Universal da Gravitação…</p>
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		<title>Um pouco de matem&#225;tica.</title>
		<link>http://wordsofphysic.wordpress.com/2010/01/23/um-pouco-de-matemtica/</link>
		<comments>http://wordsofphysic.wordpress.com/2010/01/23/um-pouco-de-matemtica/#comments</comments>
		<pubDate>Sat, 23 Jan 2010 21:07:52 +0000</pubDate>
		<dc:creator>Tiago Portela</dc:creator>
				<category><![CDATA[matematica]]></category>
		<category><![CDATA[calculo diferencial limites]]></category>
		<category><![CDATA[declive]]></category>
		<category><![CDATA[derivadas]]></category>
		<category><![CDATA[funçoes]]></category>

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		<description><![CDATA[Olá depois de algumas recomendações decidi escrever um conjunto de artigos sobre matemática que irão vos ajudar a compreender melhor os outros artigos. Hoje irei explicarei um pouco cálculo diferencial. Derivadas Imaginemos a função: Que tem como gráfico: Como poderíamos calcular a equação da reca tangente a este gráfico no ponto () O declive dessa [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=wordsofphysic.wordpress.com&amp;blog=10243983&amp;post=388&amp;subd=wordsofphysic&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<p>Olá depois de algumas recomendações decidi escrever um conjunto de artigos sobre matemática que irão vos ajudar a compreender melhor os outros artigos. </p>
<p>Hoje irei explicarei um pouco cálculo diferencial.</p>
<p><strong><font size="5">Derivadas</font></strong></p>
<p>Imaginemos a função:</p>
<p><img src='http://s0.wp.com/latex.php?latex=f%28x%29%3Dx%5E2%2B2x%2B1&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='f(x)=x^2+2x+1' title='f(x)=x^2+2x+1' class='latex' /></p>
<p>Que tem como gráfico:</p>
<p><a href="http://wordsofphysic.files.wordpress.com/2010/01/graph.png"><img title="graph" style="border-right:0;border-top:0;display:inline;border-left:0;border-bottom:0;" height="252" alt="graph" src="http://wordsofphysic.files.wordpress.com/2010/01/graph_thumb.png?w=379&#038;h=252" width="379" border="0" /></a></p>
<p>Como poderíamos calcular a equação da reca tangente a este gráfico no ponto (<img src='http://s0.wp.com/latex.php?latex=x_0%2Cf%28x_0%29&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='x_0,f(x_0)' title='x_0,f(x_0)' class='latex' />)</p>
<p><a href="http://wordsofphysic.files.wordpress.com/2010/01/graph2.png"><img title="graph2" style="border-right:0;border-top:0;display:inline;border-left:0;border-bottom:0;" height="255" alt="graph2" src="http://wordsofphysic.files.wordpress.com/2010/01/graph2_thumb.png?w=383&#038;h=255" width="383" border="0" /></a> </p>
<p>O declive dessa recta é dado por:</p>
<p> <img src='http://s0.wp.com/latex.php?latex=%5Cdisplaystyle%7B%5Clim_%7Bh+%5Cto+0%7D%5Cfrac%7Bf%28x_0%2Bh%29-f%28x_0%29%7D%7Bh%7D%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;displaystyle{&#92;lim_{h &#92;to 0}&#92;frac{f(x_0+h)-f(x_0)}{h}}' title='&#92;displaystyle{&#92;lim_{h &#92;to 0}&#92;frac{f(x_0+h)-f(x_0)}{h}}' class='latex' /></p>
<p><strong><font size="4">Definição de derivada de uma função num ponto:</font></strong></p>
<blockquote><p><strong><font size="3">Significado geométrico.</font></strong></p>
</blockquote>
<p><font size="2">Chama-se derivada da função <img src='http://s0.wp.com/latex.php?latex=f&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='f' title='f' class='latex' /> no ponto <img src='http://s0.wp.com/latex.php?latex=x_0&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='x_0' title='x_0' class='latex' /> ao limite, quando existir, da razão <img src='http://s0.wp.com/latex.php?latex=%5Cfrac%7Bf%28x_0%2Bh%29-f%28x_0%29%7D%7Bh%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;frac{f(x_0+h)-f(x_0)}{h}' title='&#92;frac{f(x_0+h)-f(x_0)}{h}' class='latex' /> quando <img src='http://s0.wp.com/latex.php?latex=h&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='h' title='h' class='latex' /> tende para zero.</font></p>
<p><font size="2">Esta derivada representasse por: <img src='http://s0.wp.com/latex.php?latex=f%27%28x_0%29&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='f&#039;(x_0)' title='f&#039;(x_0)' class='latex' />, <img src='http://s0.wp.com/latex.php?latex=%28%5Cfrac%7Bdf%7D%7Bdx%7D%29&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='(&#92;frac{df}{dx})' title='(&#92;frac{df}{dx})' class='latex' /> ou <img src='http://s0.wp.com/latex.php?latex=Df_x%3Dx_0&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='Df_x=x_0' title='Df_x=x_0' class='latex' /></font></p>
<p><font size="2"><u>Geometricamente</u>, tem-se que:</font></p>
<p><font size="2">A derivada de uma função num ponto <img src='http://s0.wp.com/latex.php?latex=x_0&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='x_0' title='x_0' class='latex' /> é o declive, <img src='http://s0.wp.com/latex.php?latex=m&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='m' title='m' class='latex' />, da recta tangente ao gráfico da função no ponto de abcissa, <img src='http://s0.wp.com/latex.php?latex=x_0&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='x_0' title='x_0' class='latex' /></font></p>
</p>
</p>
<blockquote><p><font size="3"><strong>Taxa de variação</strong></font></p>
</blockquote>
<p><font size="3"><strong>&#160;</strong></font><font size="2">A taxa média de variação de uma função <img src='http://s0.wp.com/latex.php?latex=f&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='f' title='f' class='latex' /> num intervalo <img src='http://s0.wp.com/latex.php?latex=%5Ba%2Cb%5D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='[a,b]' title='[a,b]' class='latex' /> é dado por:</font></p>
<p><font size="2"><img src='http://s0.wp.com/latex.php?latex=t.m.v_%5Ba%2Cb%5D%3D%5Cfrac%7Bf%28b%29-f%28a%29%7D%7Bb-a%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='t.m.v_[a,b]=&#92;frac{f(b)-f(a)}{b-a}' title='t.m.v_[a,b]=&#92;frac{f(b)-f(a)}{b-a}' class='latex' /></font></p>
<p><font size="2">A taxa de variação instantânea ou taxa de variação de uma função no ponto <img src='http://s0.wp.com/latex.php?latex=x%3Da&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='x=a' title='x=a' class='latex' /> é dada por:</font></p>
<p> <img src='http://s0.wp.com/latex.php?latex=%5Cdisplaystyle%7B%5Clim_%7Bh+%5Cto+0%7D%5Cfrac%7Bf%28a%2Bh%29-f%28a%29%7D%7Bh%7D%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;displaystyle{&#92;lim_{h &#92;to 0}&#92;frac{f(a+h)-f(a)}{h}}' title='&#92;displaystyle{&#92;lim_{h &#92;to 0}&#92;frac{f(a+h)-f(a)}{h}}' class='latex' />; ou seja a derivada da função no ponto <img src='http://s0.wp.com/latex.php?latex=a&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='a' title='a' class='latex' />.</p>
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		<title>Porque a Lua n&#227;o t&#234;m atmosfera?</title>
		<link>http://wordsofphysic.wordpress.com/2010/01/22/porque-a-lua-no-tm-atmosfera/</link>
		<comments>http://wordsofphysic.wordpress.com/2010/01/22/porque-a-lua-no-tm-atmosfera/#comments</comments>
		<pubDate>Fri, 22 Jan 2010 14:12:06 +0000</pubDate>
		<dc:creator>Tiago Portela</dc:creator>
				<category><![CDATA[Atmosfera]]></category>
		<category><![CDATA[energia cineticas gases]]></category>
		<category><![CDATA[gás]]></category>
		<category><![CDATA[lua]]></category>
		<category><![CDATA[velocidade de escape]]></category>

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		<description><![CDATA[Bem, de certeza que já ouviram dizer que a lua não possui atmosfera. Mas a que se deverá este facto?! Deixo-vos aqui uma pequena explicação…equ &#160; Para que algo escape da superfície terá de ter uma certa velocidade (ver). Esquecendo o movimento de rotação da lua. Onde v é a velocidade da atmosfera e r [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=wordsofphysic.wordpress.com&amp;blog=10243983&amp;post=381&amp;subd=wordsofphysic&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<p>Bem, de certeza que já ouviram dizer que a lua não possui atmosfera. Mas a que se deverá este facto?! Deixo-vos aqui uma pequena explicação…equ</p>
<p>&#160;<a href="http://wordsofphysic.files.wordpress.com/2010/01/image2.png"><img title="image" style="border-right:0;border-top:0;display:inline;border-left:0;border-bottom:0;" height="293" alt="image" src="http://wordsofphysic.files.wordpress.com/2010/01/image_thumb2.png?w=278&#038;h=293" width="278" border="0" /></a> </p>
<p>Para que algo escape da superfície terá de ter uma certa velocidade (<a href="http://wordsofphysic.wordpress.com/2009/12/26/viagens-para-fora-da-terra/">ver</a>). Esquecendo o movimento de rotação da lua.</p>
<p><img src='http://s0.wp.com/latex.php?latex=%5Cfrac%7B1%7D%7B2%7Dm_%7Batmosfera%7Dv%5E2%3D%5Cfrac%7BGm_%7BLua%7Dm_%7Batmosfera%7D%7D%7Br%5E2%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;frac{1}{2}m_{atmosfera}v^2=&#92;frac{Gm_{Lua}m_{atmosfera}}{r^2}' title='&#92;frac{1}{2}m_{atmosfera}v^2=&#92;frac{Gm_{Lua}m_{atmosfera}}{r^2}' class='latex' /> Onde v é a velocidade da atmosfera e r o raio da Lua</p>
<p><img src='http://s0.wp.com/latex.php?latex=v%3D%5Csqrt%7B%5Cfrac%7B2Gm_%7BLua%7D%7D%7Br%5E2%7D%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='v=&#92;sqrt{&#92;frac{2Gm_{Lua}}{r^2}}' title='v=&#92;sqrt{&#92;frac{2Gm_{Lua}}{r^2}}' class='latex' />[1]</p>
</p>
<p>Como a atmosfera e composta por gás podemos utilizar a equação da energia cinética de um gás.</p>
<p><img src='http://s0.wp.com/latex.php?latex=Ec%3D%5Cfrac%7B3%7D%7B2%7DkT&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='Ec=&#92;frac{3}{2}kT' title='Ec=&#92;frac{3}{2}kT' class='latex' /> Onde k é a constante de Boltzman e T a temperatura.</p>
<p><img src='http://s0.wp.com/latex.php?latex=%5Cfrac%7B1%7D%7B2%7Dm_%7Batmosfera%7D%7Bv_%7B1%7D%7D%5E2%3D%5Cfrac%7B3%7D%7B2%7DkT&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;frac{1}{2}m_{atmosfera}{v_{1}}^2=&#92;frac{3}{2}kT' title='&#92;frac{1}{2}m_{atmosfera}{v_{1}}^2=&#92;frac{3}{2}kT' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=%7Bv_%7B1%7D%7D%3D%5Csqrt%7B%5Cfrac%7B3kT%7D%7Bm_%7Batmosfera%7D%7D%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='{v_{1}}=&#92;sqrt{&#92;frac{3kT}{m_{atmosfera}}}' title='{v_{1}}=&#92;sqrt{&#92;frac{3kT}{m_{atmosfera}}}' class='latex' />[2]</p>
<p>Assim podemos calcular a massa maxima de atmosfera que a lua pode ter.</p>
<p>Aplicando os valores em [1]:</p>
<p><img src='http://s0.wp.com/latex.php?latex=v%3D%5Csqrt%7B%5Cfrac%7B2%5Ctimes6%2C67+%5Ctimes+10%5E%7B-11%7D+%5Ctimes+7%2C349%5Ctimes+10%5E%7B22%7D%7D%7B%7B1737400%7D%5E2%7D%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='v=&#92;sqrt{&#92;frac{2&#92;times6,67 &#92;times 10^{-11} &#92;times 7,349&#92;times 10^{22}}{{1737400}^2}}' title='v=&#92;sqrt{&#92;frac{2&#92;times6,67 &#92;times 10^{-11} &#92;times 7,349&#92;times 10^{22}}{{1737400}^2}}' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=v%3D3.2%5Cquad+m%2Fs&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='v=3.2&#92;quad m/s' title='v=3.2&#92;quad m/s' class='latex' /></p>
<p>Substituindo em [2]</p>
<p><img src='http://s0.wp.com/latex.php?latex=3.2%3D%5Csqrt%7B%5Cfrac%7B3kT%7D%7Bm_%7Batmosfera%7D%7D%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='3.2=&#92;sqrt{&#92;frac{3kT}{m_{atmosfera}}}' title='3.2=&#92;sqrt{&#92;frac{3kT}{m_{atmosfera}}}' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=%7B3.2%7D%5E2m_%7Batmosfera%7D%3D3%5Ctimes+1.38%5Ctimes10%5E%7B-23%7D%5Ctimes+380.15&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='{3.2}^2m_{atmosfera}=3&#92;times 1.38&#92;times10^{-23}&#92;times 380.15' title='{3.2}^2m_{atmosfera}=3&#92;times 1.38&#92;times10^{-23}&#92;times 380.15' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=m_%7Batmosfera%7D%3D1.54%5Ctimes10%5E%7B-21%7D%5Cquad+kg+&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='m_{atmosfera}=1.54&#92;times10^{-21}&#92;quad kg ' title='m_{atmosfera}=1.54&#92;times10^{-21}&#92;quad kg ' class='latex' /></p>
<p>Como a massa é muito pequena que a Lua apenas poderá ter uma quantidade <strong>muito muito muito</strong> pequena de gás não podem ter atmosfera.</p>
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		<title>Grande Defesa!</title>
		<link>http://wordsofphysic.wordpress.com/2010/01/13/grande-defesa/</link>
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		<pubDate>Wed, 13 Jan 2010 21:37:20 +0000</pubDate>
		<dc:creator>Tiago Portela</dc:creator>
				<category><![CDATA[Colisões]]></category>
		<category><![CDATA[Momentum]]></category>
		<category><![CDATA[braga]]></category>
		<category><![CDATA[defesa]]></category>
		<category><![CDATA[futebol]]></category>
		<category><![CDATA[guarda-redes]]></category>

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		<description><![CDATA[Olá mais uma vez, agora vou vós apresentar um post muito simples sobre momentum e defesas no futebol. Imaginemos que um jogador de futebol remata a bola com um velocidade () qual seria está velocidade da bola para que o guarda-redes entrasse dentro da baliza. Uma das mais importantes lei da física e que a [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=wordsofphysic.wordpress.com&amp;blog=10243983&amp;post=376&amp;subd=wordsofphysic&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<p>Olá mais uma vez, agora vou vós apresentar um post muito simples sobre <a href="http://pt.wikipedia.org/wiki/Quantidade_de_movimento_linear">momentum</a> e defesas no futebol. </p>
<p><a href="http://wordsofphysic.files.wordpress.com/2010/01/image1.png"><img title="image" style="border-right:0;border-top:0;display:inline;border-left:0;border-bottom:0;" height="193" alt="image" src="http://wordsofphysic.files.wordpress.com/2010/01/image_thumb1.png?w=288&#038;h=193" width="288" border="0" /></a> </p>
<p>Imaginemos que um jogador de futebol remata a bola com um velocidade (<img src='http://s0.wp.com/latex.php?latex=%5Cvec%7Bv%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;vec{v}' title='&#92;vec{v}' class='latex' />) qual seria está velocidade da bola para que o guarda-redes entrasse dentro da baliza.</p>
<p>Uma das mais importantes lei da física e que a conservação do momentum ou seja:</p>
<p><img src='http://s0.wp.com/latex.php?latex=%5CDelta%7Bp%7D%3D0+%5CLeftrightarrow+p%60-p%3D0+%5CLeftrightarrow+p%60%3Dp&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;Delta{p}=0 &#92;Leftrightarrow p`-p=0 &#92;Leftrightarrow p`=p' title='&#92;Delta{p}=0 &#92;Leftrightarrow p`-p=0 &#92;Leftrightarrow p`=p' class='latex' /> Sendo p o momentum antes da colisão e p’ O momentum após a colusão.</p>
<p>Como o guarde-redes se encontra parado <img src='http://s0.wp.com/latex.php?latex=v_%7Bguarda-resdes%7D%3D0&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='v_{guarda-resdes}=0' title='v_{guarda-resdes}=0' class='latex' /> Logo <img src='http://s0.wp.com/latex.php?latex=p_%7Bguarda-redes%7D%3D0&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='p_{guarda-redes}=0' title='p_{guarda-redes}=0' class='latex' /></p>
<p>E admitindo que depois da colisão o guarda-redes e a bola saem à mesma velocidade.</p>
<p><img src='http://s0.wp.com/latex.php?latex=m_%7Bbola%7Dv_%7Bbola%7D%3D%28m_%7Bbola%7D%2Bm_%7Bguarda-redes%7D%29v%60&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='m_{bola}v_{bola}=(m_{bola}+m_{guarda-redes})v`' title='m_{bola}v_{bola}=(m_{bola}+m_{guarda-redes})v`' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=v_%7Bbola%7D%3D%5Cfrac%7Bm_%7Bbola%7D%2Bm_%7Bguarda-redes%7D%7D%7Bm_%7Bbola%7D%7Dv%60&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='v_{bola}=&#92;frac{m_{bola}+m_{guarda-redes}}{m_{bola}}v`' title='v_{bola}=&#92;frac{m_{bola}+m_{guarda-redes}}{m_{bola}}v`' class='latex' /> Admitindo que o guarde-redes tem uma massa de 75 kg e que ele e a bola saem a uma velocidade,após a colusão, de 3 m/s</p>
<p><img src='http://s0.wp.com/latex.php?latex=v_%7Bbola%7D%3D3%5Cfrac%7B75%2Bm_%7Bbola%7D%7D%7Bm_%7Bbola%7D%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='v_{bola}=3&#92;frac{75+m_{bola}}{m_{bola}}' title='v_{bola}=3&#92;frac{75+m_{bola}}{m_{bola}}' class='latex' /></p>
<p>Depois de uma pesquisa encontrei que uma bola de futebol da <a href="http://www.nike.com/nikeos/p/nike/pt_PT/">Nike</a> tem uma massa de 0.4348 kg(<a href="http://www.inmetro.gov.br/consumidor/produtos/bolafutebol.asp">aqui</a>)</p>
<p><img src='http://s0.wp.com/latex.php?latex=v_%7Bbola%7D%3D3%5Cfrac%7B75%2B0.4348%7D%7B0.4348%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='v_{bola}=3&#92;frac{75+0.4348}{0.4348}' title='v_{bola}=3&#92;frac{75+0.4348}{0.4348}' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=v_%7Bbola%7D%3D520.5%5Cquad+m%2Fs&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='v_{bola}=520.5&#92;quad m/s' title='v_{bola}=520.5&#92;quad m/s' class='latex' /></p>
<p>O jogador teria de remata a bola a 520.5 m/s o que é impensável para uma pessoa.</p>
<p>(Este artigo é dedicado a um amigo que hoje faz anos e que joga no <a href="http://www.scbraga.pt/index.php">SCBraga</a>. Parabéns!)</p>
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		<title>Que idade tem o Universo?</title>
		<link>http://wordsofphysic.wordpress.com/2010/01/13/que-idade-tem-o-universo/</link>
		<comments>http://wordsofphysic.wordpress.com/2010/01/13/que-idade-tem-o-universo/#comments</comments>
		<pubDate>Wed, 13 Jan 2010 16:13:10 +0000</pubDate>
		<dc:creator>Tiago Portela</dc:creator>
				<category><![CDATA[Lei de Hubble]]></category>
		<category><![CDATA[constante de hubble]]></category>
		<category><![CDATA[hubble]]></category>
		<category><![CDATA[idade do universo]]></category>
		<category><![CDATA[universo]]></category>

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		<description><![CDATA[Bem… Hoje apresentar-vos-ei como poderemos calcular a idade do Universo. Sabendo que a Lei de Hubble relaciona a velocidades das galáxias com a sua distancia à Terra: [1] onde H é a constante de Hubble e r a distancia à Terra; Como como Aplicando em [1] H=73km/s/Mpc = 2,5&#215;10-18 segundos(Fonte: aqui) E assim calculamos a [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=wordsofphysic.wordpress.com&amp;blog=10243983&amp;post=373&amp;subd=wordsofphysic&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<p>Bem… Hoje apresentar-vos-ei como poderemos calcular a idade do Universo.</p>
<p><a href="http://wordsofphysic.files.wordpress.com/2010/01/image.png"><img title="image" style="border-right:0;border-top:0;display:inline;border-left:0;border-bottom:0;" height="313" alt="image" src="http://wordsofphysic.files.wordpress.com/2010/01/image_thumb.png?w=290&#038;h=313" width="290" border="0" /></a> </p>
</p>
<p>Sabendo que a <a href="http://www.if.ufrgs.br/oei/cgu/leihub/leihub.htm">Lei de Hubble</a> relaciona a velocidades das galáxias com a sua distancia à Terra:</p>
<p><img src='http://s0.wp.com/latex.php?latex=v_%7Bafastamento%7D%3DHr&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='v_{afastamento}=Hr' title='v_{afastamento}=Hr' class='latex' />[1] onde H é a <a href="http://astro.if.ufrgs.br/univ/hub.htm">constante de Hubble</a> e r a distancia à Terra;</p>
<p>Como <img src='http://s0.wp.com/latex.php?latex=v%3D%5Cfrac%7B%5CDelta%7Br%7D%7D%7B%5CDelta%7Bt%7D%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='v=&#92;frac{&#92;Delta{r}}{&#92;Delta{t}}' title='v=&#92;frac{&#92;Delta{r}}{&#92;Delta{t}}' class='latex' /> como <img src='http://s0.wp.com/latex.php?latex=%5CDelta%7Br%7D%3Dr%5C%3A%2C%5C%3A%5CDelta%7Bt%7D%3Dt%5C%3Ae%5C%3Av%3Dv_%7Bafastamento%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='&#92;Delta{r}=r&#92;:,&#92;:&#92;Delta{t}=t&#92;:e&#92;:v=v_{afastamento}' title='&#92;Delta{r}=r&#92;:,&#92;:&#92;Delta{t}=t&#92;:e&#92;:v=v_{afastamento}' class='latex' /></p>
<p> <img src='http://s0.wp.com/latex.php?latex=v_%7Bafastamento%7D%3D%5Cfrac%7Br%7D%7Bt%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='v_{afastamento}=&#92;frac{r}{t}' title='v_{afastamento}=&#92;frac{r}{t}' class='latex' /> Aplicando em [1]</p>
<p><img src='http://s0.wp.com/latex.php?latex=Hr%3D%5Cfrac%7Br%7D%7Bt%7D+%5CLeftrightarrow+t%3DH%5E%7B-1%7D&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='Hr=&#92;frac{r}{t} &#92;Leftrightarrow t=H^{-1}' title='Hr=&#92;frac{r}{t} &#92;Leftrightarrow t=H^{-1}' class='latex' /> H=73km/s/Mpc = 2,5&#215;10<sup>-18</sup> segundos(Fonte: <a href="http://outrafisica.blogs.sapo.pt/4228.html">aqui</a>)</p>
<p><img src='http://s0.wp.com/latex.php?latex=t%3D13+%5Ctimes+10%5E9%5Cquad+anos&amp;bg=ffffff&amp;fg=000000&amp;s=0' alt='t=13 &#92;times 10^9&#92;quad anos' title='t=13 &#92;times 10^9&#92;quad anos' class='latex' /></p>
<p> E assim calculamos a idade aproximada do Universo.</p>
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