https://vctrac.es/index.php?action=history&feed=atom&title=constante_geoc%C3%A9ntrica_de_la_gravitaci%C3%B3n 2026-04-06T03:39:11Z Historial de revisiones para esta página en el wiki MediaWiki 1.27.0 https://vctrac.es/index.php?title=constante_geoc%C3%A9ntrica_de_la_gravitaci%C3%B3n&diff=28581&oldid=prev 2020-11-05T18:49:51Z

<p></p> <table class="diff diff-contentalign-left" data-mw="interface"> <col class='diff-marker' /> <col class='diff-content' /> <col class='diff-marker' /> <col class='diff-content' /> <tr style='vertical-align: top;' lang='es'> <td colspan='2' style="background-color: white; color:black; text-align: center;">← Revisión anterior</td> <td colspan='2' style="background-color: white; color:black; text-align: center;">Revisión del 18:49 5 nov 2020</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l1" >Línea 1:</td> <td colspan="2" class="diff-lineno">Línea 1:</td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;"><div>=constante geocéntrica de la gravitación=</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;"><div>=constante geocéntrica de la gravitación=</div></td></tr> <tr><td class='diff-marker'>−</td><td style="color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>(''&lt;span style=&quot;color: green;&quot;&gt;geocentric gravitational constant&lt;/span&gt;'') ''Fís[[Category:Física]].'' Valor del parámetro geogravitacional \({G_{\rm{N}}}{M_{\rm{T}}}\), donde \({M_{\rm{T}}}\) es la masa de la Tierra. Se usa principalmente en el cálculo de órbitas geocéntricas. Su valor es: \({G_{\rm{N}}}{M_{\rm{T}}} = (398<del class="diffchange diffchange-inline">\,</del>600.441<del class="diffchange diffchange-inline">\,</del>8 ± 0.000<del class="diffchange diffchange-inline">\,</del>8)<del class="diffchange diffchange-inline">{\kern 0.3pt}{</del>10<del class="diffchange diffchange-inline">^</del>9<del class="diffchange diffchange-inline">}\</del>;<del class="diffchange diffchange-inline">{{\rm{</del>m<del class="diffchange diffchange-inline">}}^</del>3<del class="diffchange diffchange-inline">}{\kern 0.3pt} {{\rm{</del>s<del class="diffchange diffchange-inline">}}^{ - 2}}\)</del>. Sinón.: [[constante geogravitacional]].</div></td><td class='diff-marker'>+</td><td style="color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>(''&lt;span style=&quot;color: green;&quot;&gt;geocentric gravitational constant&lt;/span&gt;'') ''Fís[[Category:Física]].'' Valor del parámetro geogravitacional \({G_{\rm{N}}}{M_{\rm{T}}}\), donde \({M_{\rm{T}}}\) es la masa de la Tierra. Se usa principalmente en el cálculo de órbitas geocéntricas. Su valor es: \({G_{\rm{N}}}{M_{\rm{T}}} =<ins class="diffchange diffchange-inline">\,</ins>(<ins class="diffchange diffchange-inline">\)</ins>398<ins class="diffchange diffchange-inline">&amp;#8239;</ins>600.441<ins class="diffchange diffchange-inline">&amp;#8239;</ins>8<ins class="diffchange diffchange-inline">&amp;#8239;</ins>±<ins class="diffchange diffchange-inline">&amp;#8239;</ins>0.000<ins class="diffchange diffchange-inline">&amp;#8239;</ins>8<ins class="diffchange diffchange-inline">$</ins>)<ins class="diffchange diffchange-inline">$</ins>10<ins class="diffchange diffchange-inline">&lt;sup&gt;</ins>9<ins class="diffchange diffchange-inline">&lt;/sup&gt;&amp;#8239;&amp;nbsp</ins>;m<ins class="diffchange diffchange-inline">&lt;sup&gt;</ins>3<ins class="diffchange diffchange-inline">&lt;/sup&gt;&amp;#8239;·&amp;#8239;</ins>s<ins class="diffchange diffchange-inline">&lt;sup&gt;−2&lt;/sup&gt;</ins>. Sinón.: [[constante geogravitacional]].</div></td></tr> </table>

Elena https://vctrac.es/index.php?title=constante_geoc%C3%A9ntrica_de_la_gravitaci%C3%B3n&diff=28065&oldid=prev 2020-06-23T10:20:26Z

<p></p> <table class="diff diff-contentalign-left" data-mw="interface"> <col class='diff-marker' /> <col class='diff-content' /> <col class='diff-marker' /> <col class='diff-content' /> <tr style='vertical-align: top;' lang='es'> <td colspan='2' style="background-color: white; color:black; text-align: center;">← Revisión anterior</td> <td colspan='2' style="background-color: white; color:black; text-align: center;">Revisión del 10:20 23 jun 2020</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l1" >Línea 1:</td> <td colspan="2" class="diff-lineno">Línea 1:</td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;"><div>=constante geocéntrica de la gravitación=</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;"><div>=constante geocéntrica de la gravitación=</div></td></tr> <tr><td class='diff-marker'>−</td><td style="color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>(''&lt;span style=&quot;color: green;&quot;&gt;geocentric gravitational constant&lt;/span&gt;'') ''Fís[[Category:Física]].'' Valor del parámetro geogravitacional \({G_{\rm{N}}}{M_{\rm{T}}}\), donde \({M_{\rm{T}}}\) es la masa de la Tierra. Se usa principalmente en el cálculo de órbitas geocéntricas. Su valor es: \({G_{\rm{N}}}{M_{\rm{T}}} = (398<del class="diffchange diffchange-inline">;</del>600.<del class="diffchange diffchange-inline">4418 pm </del>0.<del class="diffchange diffchange-inline">0008</del>) {10^9}<del class="diffchange diffchange-inline">{</del>\<del class="diffchange diffchange-inline">kern 1pt} </del>{{\rm{m}}^3}{\kern <del class="diffchange diffchange-inline">1pt</del>} {{\rm{s}}^{ - 2}}\). Sinón.: [[constante geogravitacional]].</div></td><td class='diff-marker'>+</td><td style="color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>(''&lt;span style=&quot;color: green;&quot;&gt;geocentric gravitational constant&lt;/span&gt;'') ''Fís[[Category:Física]].'' Valor del parámetro geogravitacional \({G_{\rm{N}}}{M_{\rm{T}}}\), donde \({M_{\rm{T}}}\) es la masa de la Tierra. Se usa principalmente en el cálculo de órbitas geocéntricas. Su valor es: \({G_{\rm{N}}}{M_{\rm{T}}} = (398<ins class="diffchange diffchange-inline">\,</ins>600.<ins class="diffchange diffchange-inline">441\,8 ± </ins>0.<ins class="diffchange diffchange-inline">000\,8</ins>)<ins class="diffchange diffchange-inline">{\kern 0.3pt}</ins>{10^9}\<ins class="diffchange diffchange-inline">;</ins>{{\rm{m}}^3}{\kern <ins class="diffchange diffchange-inline">0.3pt</ins>} {{\rm{s}}^{ - 2}}\). Sinón.: [[constante geogravitacional]].</div></td></tr> </table>

Elena https://vctrac.es/index.php?title=constante_geoc%C3%A9ntrica_de_la_gravitaci%C3%B3n&diff=27489&oldid=prev 2020-01-22T09:38:25Z

<p></p> <table class="diff diff-contentalign-left" data-mw="interface"> <col class='diff-marker' /> <col class='diff-content' /> <col class='diff-marker' /> <col class='diff-content' /> <tr style='vertical-align: top;' lang='es'> <td colspan='2' style="background-color: white; color:black; text-align: center;">← Revisión anterior</td> <td colspan='2' style="background-color: white; color:black; text-align: center;">Revisión del 09:38 22 ene 2020</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l1" >Línea 1:</td> <td colspan="2" class="diff-lineno">Línea 1:</td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;"><div>=constante geocéntrica de la gravitación=</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;"><div>=constante geocéntrica de la gravitación=</div></td></tr> <tr><td class='diff-marker'>−</td><td style="color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>(''&lt;span style=&quot;color: green;&quot;&gt;geocentric gravitational constant&lt;/span&gt;'') ''Fís[[Category:Física]].'' Valor del parámetro geogravitacional ({G_{rm{N}}}{M_{rm{T}}}), donde ({M_{rm{T}}}) es la masa de la Tierra. Se usa principalmente en el cálculo de órbitas geocéntricas. Su valor es: ({G_{rm{N}}}{M_{rm{T}}} = (398;600.4418 pm 0.0008)<del class="diffchange diffchange-inline">;</del>{10^9}{kern 1pt} {{rm{m}}^3}{kern 1pt} {{rm{s}}^{ - 2}}). Sinón.: [[constante geogravitacional]].</div></td><td class='diff-marker'>+</td><td style="color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>(''&lt;span style=&quot;color: green;&quot;&gt;geocentric gravitational constant&lt;/span&gt;'') ''Fís[[Category:Física]].'' Valor del parámetro geogravitacional <ins class="diffchange diffchange-inline">\</ins>({G_{<ins class="diffchange diffchange-inline">\</ins>rm{N}}}{M_{<ins class="diffchange diffchange-inline">\</ins>rm{T}}}<ins class="diffchange diffchange-inline">\</ins>), donde <ins class="diffchange diffchange-inline">\</ins>({M_{<ins class="diffchange diffchange-inline">\</ins>rm{T}}}<ins class="diffchange diffchange-inline">\</ins>) es la masa de la Tierra. Se usa principalmente en el cálculo de órbitas geocéntricas. Su valor es: <ins class="diffchange diffchange-inline">\</ins>({G_{<ins class="diffchange diffchange-inline">\</ins>rm{N}}}{M_{<ins class="diffchange diffchange-inline">\</ins>rm{T}}} = (398;600.4418 pm 0.0008) {10^9}{<ins class="diffchange diffchange-inline">\</ins>kern 1pt} {{<ins class="diffchange diffchange-inline">\</ins>rm{m}}^3}{<ins class="diffchange diffchange-inline">\</ins>kern 1pt} {{<ins class="diffchange diffchange-inline">\</ins>rm{s}}^{ - 2}}<ins class="diffchange diffchange-inline">\</ins>). Sinón.: [[constante geogravitacional]].</div></td></tr> </table>

David https://vctrac.es/index.php?title=constante_geoc%C3%A9ntrica_de_la_gravitaci%C3%B3n&diff=23434&oldid=prev 2020-01-20T09:53:16Z

<p>Imported from text file</p> <p><b>Página nueva</b></p><div>=constante geocéntrica de la gravitación=<br /> (''&lt;span style=&quot;color: green;&quot;&gt;geocentric gravitational constant&lt;/span&gt;'') ''Fís[[Category:Física]].'' Valor del parámetro geogravitacional ({G_{rm{N}}}{M_{rm{T}}}), donde ({M_{rm{T}}}) es la masa de la Tierra. Se usa principalmente en el cálculo de órbitas geocéntricas. Su valor es: ({G_{rm{N}}}{M_{rm{T}}} = (398;600.4418 pm 0.0008);{10^9}{kern 1pt} {{rm{m}}^3}{kern 1pt} {{rm{s}}^{ - 2}}). Sinón.: [[constante geogravitacional]].</div>

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