http://marspedia.org/index.php?title=Orbital_energy&feed=atom&action=historyOrbital energy - Revision history2024-03-28T23:41:58ZRevision history for this page on the wikiMediaWiki 1.34.2http://marspedia.org/index.php?title=Orbital_energy&diff=8191&oldid=prevChristiaanK: Internal links2013-02-05T16:47:30Z<p>Internal links</p>
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<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 16:47, 5 February 2013</td>
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<tr><td class='diff-marker'>−</td><td style="color: #222; 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>When a body orbits another body, it has [[kinetic energy]] (since it is moving) and [[potential energy]] (since [[gravity]] is pulling it towards the other body). The sum of these two energies is the total orbital energy, and remains constant so long as no external force acts on the body.</div></td><td class='diff-marker'>+</td><td style="color: #222; 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>When a body orbits another body, it has [[kinetic energy]] (since it is moving) and [[potential energy]] (since [[gravity]] is pulling it towards the other body). The sum of these two energies is the total orbital energy, and remains constant so long as no external force acts on the body. <ins class="diffchange diffchange-inline">The total energy is simply the mass times [[specific energy]]:</ins></div></td></tr>
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<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="color: #222; 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><ins class="diffchange diffchange-inline"><math>m \times \epsilon</math></ins></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>[[Category:Orbital Mechanics]]</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>[[Category:Orbital Mechanics]]</div></td></tr>
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</table>ChristiaanKhttp://marspedia.org/index.php?title=Orbital_energy&diff=8162&oldid=prevChristiaanK at 17:06, 4 February 20132013-02-04T17:06:44Z<p></p>
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<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 17:06, 4 February 2013</td>
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<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>When a body orbits another body, it has [[kinetic energy]] (since it is moving) and [[potential energy]] (since [[gravity]] is pulling it towards the other body). The sum of these two energies is the total orbital energy, and remains constant so long as no external force acts on the body.</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>When a body orbits another body, it has [[kinetic energy]] (since it is moving) and [[potential energy]] (since [[gravity]] is pulling it towards the other body). The sum of these two energies is the total orbital energy, and remains constant so long as no external force acts on the body.</div></td></tr>
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</table>ChristiaanKhttp://marspedia.org/index.php?title=Orbital_energy&diff=8161&oldid=prevChristiaanK: Created page2013-02-04T17:06:16Z<p>Created page</p>
<p><b>New page</b></p><div>When a body orbits another body, it has [[kinetic energy]] (since it is moving) and [[potential energy]] (since [[gravity]] is pulling it towards the other body). The sum of these two energies is the total orbital energy, and remains constant so long as no external force acts on the body.</div>ChristiaanK