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authorTimothy Pearson <kb9vqf@pearsoncomputing.net>2011-12-03 11:05:10 -0600
committerTimothy Pearson <kb9vqf@pearsoncomputing.net>2011-12-03 11:05:10 -0600
commitf7e7a923aca8be643f9ae6f7252f9fb27b3d2c3b (patch)
tree1f78ef53b206c6b4e4efc88c4849aa9f686a094d /tde-i18n-pt_BR/docs/kdeedu/kstars/meridian.docbook
parent85ca18776aa487b06b9d5ab7459b8f837ba637f3 (diff)
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-<sect1 id="ai-meridian">
-<sect1info>
-<author
-><firstname
->Jason</firstname
-> <surname
->Harris</surname
-> </author>
-</sect1info>
-<title
->O Meridiano Local</title>
-<indexterm
-><primary
->O Meridiano Local</primary>
-<seealso
->Ângula da Hora</seealso
-> <seealso
->Esfera Celestial </seealso
-> </indexterm>
-<para
->O Meridiano Local é um <link linkend="ai-greatcircle"
->Grande Círculo</link
-> imaginário na <link linkend="ai-csphere"
->Esfera Celestial</link
-> que é perpendicular ao <link linkend="ai-horizon"
->Horizonte</link
-> local. Ele passa através do ponto Norte do Horizonte, pelo <link linkend="ai-cpoles"
->Pólo Celestial</link
->, até o <link linkend="ai-zenith"
->Zénite</link
->, e pelo ponto Sul do Horizonte. </para
-><para
->Porque é fixado no Horizonte local, as estrelas parecem passar pelo Meridiano local conforme a Terra gira. Você pode usar a <link linkend="equatorial"
->Ascensão Direita</link
-> de um objeto e a <link linkend="ai-sidereal"
->Hora Sideral Local</link
-> para determinar quando ele cruzará seu Meridiano Local (veja <link linkend="ai-hourangle"
->Ângulo Horário</link
->). </para>
-</sect1>
-