https://www2.lpod.org/index.php?title=December_23,_2013&feed=atom&action=history
December 23, 2013 - Revision history
2024-03-29T13:28:07Z
Revision history for this page on the wiki
MediaWiki 1.31.1
https://www2.lpod.org/index.php?title=December_23,_2013&diff=43078&oldid=prev
Regan at 03:45, 28 October 2018
2018-10-28T03:45:09Z
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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><em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /></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><em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /></div></td></tr>
<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><del style="font-weight: bold; text-decoration: none;"><strong>This is a classic LPOD</strong> from [http://lpod.wikispaces.com/June+27,+2010 June 27, 2010]; make sure you check the good [http://lpod.wikispaces.com/page/messages/June+27%2C+2010 comments] that appeared then and consider if there is more to add, 3.5 years later. <br /></del></div></td><td colspan="2"> </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><br /></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><br /></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><p><b>Yesterday's LPOD:</b> [[December 22, 2013|Happenstance Earthrise]] </p></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><p><b>Yesterday's LPOD:</b> [[December 22, 2013|Happenstance Earthrise]] </p></div></td></tr>
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Regan
https://www2.lpod.org/index.php?title=December_23,_2013&diff=33110&oldid=prev
Api at 22:48, 8 February 2015
2015-02-08T22:48:59Z
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Api
https://www2.lpod.org/index.php?title=December_23,_2013&diff=29399&oldid=prev
Api at 01:37, 8 February 2015
2015-02-08T01:37:51Z
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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><p><b>Tomorrow's LPOD:</b> [[December 24, 2013|Roadmap]] </p></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><p><b>Tomorrow's LPOD:</b> [[December 24, 2013|Roadmap]] </p></div></td></tr>
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Api
https://www2.lpod.org/index.php?title=December_23,_2013&diff=28465&oldid=prev
Api at 20:03, 7 February 2015
2015-02-07T20:03:00Z
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<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 20:03, 7 February 2015</td>
</tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l10" >Line 10:</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><strong>This is a classic LPOD</strong> from [http://lpod.wikispaces.com/June+27,+2010 June 27, 2010]; make sure you check the good [http://lpod.wikispaces.com/page/messages/June+27%2C+2010 comments] that appeared then and consider if there is more to add, 3.5 years later. <br /></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><strong>This is a classic LPOD</strong> from [http://lpod.wikispaces.com/June+27,+2010 June 27, 2010]; make sure you check the good [http://lpod.wikispaces.com/page/messages/June+27%2C+2010 comments] that appeared then and consider if there is more to add, 3.5 years later. <br /></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><br /></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><br /></div></td></tr>
<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 style="font-weight: bold; text-decoration: none;"><p><b>Yesterday's LPOD:</b> [[December 22, 2013|Happenstance Earthrise]] </p></ins></div></td></tr>
<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 style="font-weight: bold; text-decoration: none;"><p><b>Tomorrow's LPOD:</b> [[December 24, 2013|Roadmap]] </p></ins></div></td></tr>
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Api
https://www2.lpod.org/index.php?title=December_23,_2013&diff=18487&oldid=prev
Api at 01:13, 12 January 2015
2015-01-12T01:13:41Z
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<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 01:13, 12 January 2015</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><em>image from [http://lroc.sese.asu.edu/news/index.php?/archives/240-Forked-Impact-Melt-Flows-at-Farside-Crater.html<del class="diffchange diffchange-inline">" rel="nofollow </del>LROC Featured Image] (NASA/GSFC/ASU)</em><br /></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><em>image from [http://lroc.sese.asu.edu/news/index.php?/archives/240-Forked-Impact-Melt-Flows-at-Farside-Crater.html LROC Featured Image] (NASA/GSFC/ASU)</em><br /></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><br /></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><br /></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>The hyper-resolution of LRO is disclosing phenomena that we haven't seen before. One type of feature that has been especially well depicted is impact melt. Studies in the 1970s from Lunar Orbiter images and Apollo photos demonstrated that thin veneers of melt were commonly splashed around fresh impact craters. This image of a 3.1 km diameter crater at 161°E and 30°N shows an impact melt that is strange because it is so massive. It appears that a broad swath of the left exterior of the crater has a patina of dark melt, that flowed downhill, including turning nearly 90° to the right, before breaking into two wide lobes (right image). B. Ray Hawke, who wrote the caption for the LRO Featured Image story, suggests that a local high spot divided the advancing flow into two. The other end of the flow is fascinating too. The flow at the rim crest has a sharply defined right edge, which continues down the inner wall of the crater to the floor. This suggests that the flow was propelled up the crater wall - not ballistically launched - and flowed over the top and downslope along the surface as we see it. Can impact melt behave like a ground surge that effortlessly rises up and down slopes until it cools enough to freeze in place?<br /></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>The hyper-resolution of LRO is disclosing phenomena that we haven't seen before. One type of feature that has been especially well depicted is impact melt. Studies in the 1970s from Lunar Orbiter images and Apollo photos demonstrated that thin veneers of melt were commonly splashed around fresh impact craters. This image of a 3.1 km diameter crater at 161°E and 30°N shows an impact melt that is strange because it is so massive. It appears that a broad swath of the left exterior of the crater has a patina of dark melt, that flowed downhill, including turning nearly 90° to the right, before breaking into two wide lobes (right image). B. Ray Hawke, who wrote the caption for the LRO Featured Image story, suggests that a local high spot divided the advancing flow into two. The other end of the flow is fascinating too. The flow at the rim crest has a sharply defined right edge, which continues down the inner wall of the crater to the floor. This suggests that the flow was propelled up the crater wall - not ballistically launched - and flowed over the top and downslope along the surface as we see it. Can impact melt behave like a ground surge that effortlessly rises up and down slopes until it cools enough to freeze in place?<br /></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><br /></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><br /></div></td></tr>
<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><em>[mailto:tychocrater@yahoo.com<del class="diffchange diffchange-inline">" rel="nofollow </del>Chuck Wood]</em><br /></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><em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /></div></td></tr>
<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><strong>This is a classic LPOD</strong> from [http://lpod.wikispaces.com/June+27,+2010 June 27, 2010]; make sure you check the good [http://lpod.wikispaces.com/page/messages/June+27%2C+2010<del class="diffchange diffchange-inline">" rel="nofollow </del>comments] that appeared then and consider if there is more to add, 3.5 years later. <br /></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><strong>This is a classic LPOD</strong> from [http://lpod.wikispaces.com/June+27,+2010 June 27, 2010]; make sure you check the good [http://lpod.wikispaces.com/page/messages/June+27%2C+2010 comments] that appeared then and consider if there is more to add, 3.5 years later. <br /></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><br /></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><br /></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><hr /></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><hr /></div></td></tr>
</table>
Api
https://www2.lpod.org/index.php?title=December_23,_2013&diff=15217&oldid=prev
Api at 05:54, 5 January 2015
2015-01-05T05:54:07Z
<p></p>
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<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td>
<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 05:54, 5 January 2015</td>
</tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l1" >Line 1:</td>
<td colspan="2" class="diff-lineno">Line 1:</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>__NOTOC__</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>__NOTOC__</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>=Y or Why?=</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>=Y or Why?=</div></td></tr>
<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><del style="font-weight: bold; text-decoration: none;"></del></div></td><td colspan="2"> </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><!-- ws:start:WikiTextHeadingRule:0:&lt;h1&gt; --></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><!-- ws:start:WikiTextHeadingRule:0:&lt;h1&gt; --></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><!-- ws:start:WikiTextLocalImageRule:6:&lt;img src=&quot;/file/view/LPOD-June27-10.jpg/150649309/LPOD-June27-10.jpg&quot; alt=&quot;&quot; title=&quot;&quot; /&gt; -->[[File:LPOD-June27-10.jpg|LPOD-June27-10.jpg]]<!-- ws:end:WikiTextLocalImageRule:6 --><br /></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><!-- ws:start:WikiTextLocalImageRule:6:&lt;img src=&quot;/file/view/LPOD-June27-10.jpg/150649309/LPOD-June27-10.jpg&quot; alt=&quot;&quot; title=&quot;&quot; /&gt; -->[[File:LPOD-June27-10.jpg|LPOD-June27-10.jpg]]<!-- ws:end:WikiTextLocalImageRule:6 --><br /></div></td></tr>
<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><em>image from [http://lroc.sese.asu.edu/news/index.php?/archives/240-Forked-Impact-Melt-Flows-at-Farside-Crater.html LROC Featured Image] (NASA/GSFC/ASU)</em><br /></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><em>image from [http://lroc.sese.asu.edu/news/index.php?/archives/240-Forked-Impact-Melt-Flows-at-Farside-Crater.html<ins class="diffchange diffchange-inline">" rel="nofollow </ins>LROC Featured Image] (NASA/GSFC/ASU)</em><br /></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><br /></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><br /></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>The hyper-resolution of LRO is disclosing phenomena that we haven't seen before. One type of feature that has been especially well depicted is impact melt. Studies in the 1970s from Lunar Orbiter images and Apollo photos demonstrated that thin veneers of melt were commonly splashed around fresh impact craters. This image of a 3.1 km diameter crater at 161°E and 30°N shows an impact melt that is strange because it is so massive. It appears that a broad swath of the left exterior of the crater has a patina of dark melt, that flowed downhill, including turning nearly 90° to the right, before breaking into two wide lobes (right image). B. Ray Hawke, who wrote the caption for the LRO Featured Image story, suggests that a local high spot divided the advancing flow into two. The other end of the flow is fascinating too. The flow at the rim crest has a sharply defined right edge, which continues down the inner wall of the crater to the floor. This suggests that the flow was propelled up the crater wall - not ballistically launched - and flowed over the top and downslope along the surface as we see it. Can impact melt behave like a ground surge that effortlessly rises up and down slopes until it cools enough to freeze in place?<br /></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>The hyper-resolution of LRO is disclosing phenomena that we haven't seen before. One type of feature that has been especially well depicted is impact melt. Studies in the 1970s from Lunar Orbiter images and Apollo photos demonstrated that thin veneers of melt were commonly splashed around fresh impact craters. This image of a 3.1 km diameter crater at 161°E and 30°N shows an impact melt that is strange because it is so massive. It appears that a broad swath of the left exterior of the crater has a patina of dark melt, that flowed downhill, including turning nearly 90° to the right, before breaking into two wide lobes (right image). B. Ray Hawke, who wrote the caption for the LRO Featured Image story, suggests that a local high spot divided the advancing flow into two. The other end of the flow is fascinating too. The flow at the rim crest has a sharply defined right edge, which continues down the inner wall of the crater to the floor. This suggests that the flow was propelled up the crater wall - not ballistically launched - and flowed over the top and downslope along the surface as we see it. Can impact melt behave like a ground surge that effortlessly rises up and down slopes until it cools enough to freeze in place?<br /></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><br /></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><br /></div></td></tr>
<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><em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /></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><em>[mailto:tychocrater@yahoo.com<ins class="diffchange diffchange-inline">" rel="nofollow </ins>Chuck Wood]</em><br /></div></td></tr>
<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><strong>This is a classic LPOD</strong> from [http://lpod.wikispaces.com/June+27,+2010 June 27, 2010]; make sure you check the good [http://lpod.wikispaces.com/page/messages/June+27%2C+2010 comments] that appeared then and consider if there is more to add, 3.5 years later. <br /></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><strong>This is a classic LPOD</strong> from [http://lpod.wikispaces.com/June+27,+2010 June 27, 2010]; make sure you check the good [http://lpod.wikispaces.com/page/messages/June+27%2C+2010<ins class="diffchange diffchange-inline">" rel="nofollow </ins>comments] that appeared then and consider if there is more to add, 3.5 years later. <br /></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><br /></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><br /></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><hr /></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><hr /></div></td></tr>
</table>
Api
https://www2.lpod.org/index.php?title=December_23,_2013&diff=10966&oldid=prev
Api at 07:55, 3 January 2015
2015-01-03T07:55:42Z
<p></p>
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<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td>
<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 07:55, 3 January 2015</td>
</tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l2" >Line 2:</td>
<td colspan="2" class="diff-lineno">Line 2:</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>=Y or Why?=</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>=Y or Why?=</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;"></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;"></td></tr>
<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><del class="diffchange diffchange-inline">  </del><!-- ws:start:WikiTextHeadingRule:0:&lt;h1&gt; --></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><!-- ws:start:WikiTextHeadingRule:0:&lt;h1&gt; --></div></td></tr>
<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><del class="diffchange diffchange-inline"> </del><!-- ws:start:WikiTextLocalImageRule:6:&lt;img src=&quot;/file/view/LPOD-June27-10.jpg/150649309/LPOD-June27-10.jpg&quot; alt=&quot;&quot; title=&quot;&quot; /&gt; -->[[File:LPOD-June27-10.jpg|LPOD-June27-10.jpg]]<!-- ws:end:WikiTextLocalImageRule:6 --><br /></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><!-- ws:start:WikiTextLocalImageRule:6:&lt;img src=&quot;/file/view/LPOD-June27-10.jpg/150649309/LPOD-June27-10.jpg&quot; alt=&quot;&quot; title=&quot;&quot; /&gt; -->[[File:LPOD-June27-10.jpg|LPOD-June27-10.jpg]]<!-- ws:end:WikiTextLocalImageRule:6 --><br /></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><em>image from [http://lroc.sese.asu.edu/news/index.php?/archives/240-Forked-Impact-Melt-Flows-at-Farside-Crater.html LROC Featured Image] (NASA/GSFC/ASU)</em><br /></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><em>image from [http://lroc.sese.asu.edu/news/index.php?/archives/240-Forked-Impact-Melt-Flows-at-Farside-Crater.html LROC Featured Image] (NASA/GSFC/ASU)</em><br /></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><br /></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><br /></div></td></tr>
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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><del style="font-weight: bold; text-decoration: none;"></del></div></td><td colspan="2"> </td></tr>
<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><del style="font-weight: bold; text-decoration: none;">----</del></div></td><td colspan="2"> </td></tr>
<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><del style="font-weight: bold; text-decoration: none;">===COMMENTS?=== </del></div></td><td colspan="2"> </td></tr>
<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><del style="font-weight: bold; text-decoration: none;">Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment.</del></div></td><td colspan="2"> </td></tr>
</table>
Api
https://www2.lpod.org/index.php?title=December_23,_2013&diff=8093&oldid=prev
Api: Created page with "__NOTOC__ =Y or Why?= <!-- ws:start:WikiTextHeadingRule:0:<h1> --> <!-- ws:start:WikiTextLocalImageRule:6:<img src="/file/view/LPOD-June27-10.jpg/150649309/L..."
2015-01-02T05:38:34Z
<p>Created page with "__NOTOC__ =Y or Why?= <!-- ws:start:WikiTextHeadingRule:0:<h1> --> <!-- ws:start:WikiTextLocalImageRule:6:<img src="/file/view/LPOD-June27-10.jpg/150649309/L..."</p>
<p><b>New page</b></p><div>__NOTOC__<br />
=Y or Why?=<br />
<br />
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<em>image from [http://lroc.sese.asu.edu/news/index.php?/archives/240-Forked-Impact-Melt-Flows-at-Farside-Crater.html LROC Featured Image] (NASA/GSFC/ASU)</em><br /><br />
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The hyper-resolution of LRO is disclosing phenomena that we haven't seen before. One type of feature that has been especially well depicted is impact melt. Studies in the 1970s from Lunar Orbiter images and Apollo photos demonstrated that thin veneers of melt were commonly splashed around fresh impact craters. This image of a 3.1 km diameter crater at 161°E and 30°N shows an impact melt that is strange because it is so massive. It appears that a broad swath of the left exterior of the crater has a patina of dark melt, that flowed downhill, including turning nearly 90° to the right, before breaking into two wide lobes (right image). B. Ray Hawke, who wrote the caption for the LRO Featured Image story, suggests that a local high spot divided the advancing flow into two. The other end of the flow is fascinating too. The flow at the rim crest has a sharply defined right edge, which continues down the inner wall of the crater to the floor. This suggests that the flow was propelled up the crater wall - not ballistically launched - and flowed over the top and downslope along the surface as we see it. Can impact melt behave like a ground surge that effortlessly rises up and down slopes until it cools enough to freeze in place?<br /><br />
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<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /><br />
<strong>This is a classic LPOD</strong> from [http://lpod.wikispaces.com/June+27,+2010 June 27, 2010]; make sure you check the good [http://lpod.wikispaces.com/page/messages/June+27%2C+2010 comments] that appeared then and consider if there is more to add, 3.5 years later. <br /><br />
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