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Stubbig Lichtenheldt 2022a - Revision history
2026-06-10T11:33:58Z
Revision history for this page on the wiki
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Scipediacontent at 12:22, 15 February 2022
2022-02-15T12:22:28Z
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<td colspan='2' style="background-color: white; color:black; text-align: center;">← Older revision</td>
<td colspan='2' style="background-color: white; color:black; text-align: center;">Revision as of 12:22, 15 February 2022</td>
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<tr><td class='diff-marker'> </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>                                                  </div></td><td class='diff-marker'> </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>                                                  </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>== <del class="diffchange diffchange-inline">Document </del>==</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>== <ins class="diffchange diffchange-inline">Abstract ==</ins></div></td></tr>
<tr><td colspan="2"> </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><ins class="diffchange diffchange-inline"><pdf>Media:Stubbig_Lichtenheldt_2022a_5293_1036_abstract.pdf</pdf></ins></div></td></tr>
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<tr><td colspan="2"> </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><ins class="diffchange diffchange-inline">== Full paper </ins>==</div></td></tr>
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Scipediacontent
http://www.colloquiam.com/wd/index.php?title=Stubbig_Lichtenheldt_2022a&diff=235719&oldid=prev
Scipediacontent: Scipediacontent moved page Draft Content 939906588 to Stubbig Lichtenheldt 2022a
2022-02-15T11:26:37Z
<p>Scipediacontent moved page <a href="/public/Draft_Content_939906588" class="mw-redirect" title="Draft Content 939906588">Draft Content 939906588</a> to <a href="/public/Stubbig_Lichtenheldt_2022a" title="Stubbig Lichtenheldt 2022a">Stubbig Lichtenheldt 2022a</a></p>
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<td colspan='1' style="background-color: white; color:black; text-align: center;">Revision as of 11:26, 15 February 2022</td>
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Scipediacontent
http://www.colloquiam.com/wd/index.php?title=Stubbig_Lichtenheldt_2022a&diff=235718&oldid=prev
Scipediacontent: Created page with "== Abstract == The MMX Rover is a contribution by CNES and DLR to JAXA's Martian Moons eXploration (MMX) mission and will explore the surface of the Mars moon Phobos. As ther..."
2022-02-15T11:26:32Z
<p>Created page with "== Abstract == The MMX Rover is a contribution by CNES and DLR to JAXA's Martian Moons eXploration (MMX) mission and will explore the surface of the Mars moon Phobos. As ther..."</p>
<p><b>New page</b></p><div>== Abstract ==<br />
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The MMX Rover is a contribution by CNES and DLR to JAXA's Martian Moons eXploration (MMX) mission and will explore the surface of the Mars moon Phobos. As there haven’t been any successful landers on Phobos, little is known about the conditions on the moon’s surface. Additionally, the gravity on Phobos is only about 1/2000 of Earth’s gravity and the behavior of regolith in such low gravity is still a topic of active research. In order to design a suitable wheel for the MMX Rover, we made worst-case assumptions about the soil conditions and implemented them in a simulation model using the Discrete Element Method. This simulation is then used within an optimization loop that automatically tests different wheel shapes on their suitability for reliable locomotion on Phobos. The result is an optimized wheel shape as well as a dataset showing how different wheel shapes affect wheel performance. These results are now being used to design the wheels for the MMX Rover.<br />
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== Video ==<br />
{{#evt:service=cloudfront|id=276723|alignment=center|filename=1036.mp4}}<br />
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== Document ==<br />
<pdf>Media:Draft_Content_9399065881036_paper.pdf</pdf></div>
Scipediacontent