Difference between revisions of "August 21, 2010"
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| − | <em>image from [http://www.nasa.gov/mission_pages/LRO/news/shrinking-moon.html NASA/LRO]. Digital topographic map with black circles representing lobate scarps discovered during the Apollo era, and white dots newly discovered scarps seen on LRO image. Inset at bottom left is scarp at Gregory crater - the white circle near the equator at far right.</em> <br /> | + | <em>image from [http://www.nasa.gov/mission_pages/LRO/news/shrinking-moon.html" rel="nofollow NASA/LRO]. Digital topographic map with black circles representing lobate scarps discovered during the Apollo era, and white dots newly discovered scarps seen on LRO image. Inset at bottom left is scarp at Gregory crater - the white circle near the equator at far right.</em> <br /> |
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| − | Teams flying spacecraft around a planet often rediscover what was found on previous missions. Press releases, or the way they are sensationalized by the press, sometimes seem to imply that the spacecraft has made a wondrous new discovery, when it is in fact merely an extension of what was learned earlier. This has happened repeatedly on Mars missions, and there is a tinge of it in recent press coverage of imaging of lunar lobate scarps by Lunar Reconnaissance Orbiter. The LRO team's press release states that such scarps were first discovered in Apollo images and the map shows the currently known distribution of Apollo (black circles) and LRO (white circle) scarps. Lobate scarps are interpreted as low angle [http://lpod.wikispaces.com/December+1%2C+2008 thrust faults], places where one piece of crust slides up over adjacent terrain. They are typically only a few tens of meters high and nearly impossible to see from Earth; perhaps the only one imageable by [http://lpod.wikispaces.com/December+17%2C+2008 amateurs] is the [http://the-moon.wikispaces.com/Scarp Lincoln-Lee Scarp] near the Apollo 17 landing site. Twenty-five years ago [http://www.sciencedirect.com/science?_ob=ArticleURL&_udi=B6WGF-47318GS-273&_user=10&_rdoc=1&_fmt=&_orig=search&_sort=d&view=c&_acct=C000050221&_version=1&_urlVersion=0&_userid=10&md5=d918f7fac765c78ab21bdd112bd4fd05 Alan Binder and Hanns Gunga] discovered and studied most of the scarps now known and determined that they are very young (perhaps a few hundred million years) and represent recent tectonic activity. The LRO team agrees, suggesting that the scarps are due to a global cooling and shrinking of the Moon's radius by about 100 m. <br /> | + | Teams flying spacecraft around a planet often rediscover what was found on previous missions. Press releases, or the way they are sensationalized by the press, sometimes seem to imply that the spacecraft has made a wondrous new discovery, when it is in fact merely an extension of what was learned earlier. This has happened repeatedly on Mars missions, and there is a tinge of it in recent press coverage of imaging of lunar lobate scarps by Lunar Reconnaissance Orbiter. The LRO team's press release states that such scarps were first discovered in Apollo images and the map shows the currently known distribution of Apollo (black circles) and LRO (white circle) scarps. Lobate scarps are interpreted as low angle [http://lpod.wikispaces.com/December+1%2C+2008 thrust faults], places where one piece of crust slides up over adjacent terrain. They are typically only a few tens of meters high and nearly impossible to see from Earth; perhaps the only one imageable by [http://lpod.wikispaces.com/December+17%2C+2008 amateurs] is the [http://the-moon.wikispaces.com/Scarp Lincoln-Lee Scarp] near the Apollo 17 landing site. Twenty-five years ago [http://www.sciencedirect.com/science?_ob=ArticleURL&_udi=B6WGF-47318GS-273&_user=10&_rdoc=1&_fmt=&_orig=search&_sort=d&view=c&_acct=C000050221&_version=1&_urlVersion=0&_userid=10&md5=d918f7fac765c78ab21bdd112bd4fd05" rel="nofollow Alan Binder and Hanns Gunga] discovered and studied most of the scarps now known and determined that they are very young (perhaps a few hundred million years) and represent recent tectonic activity. The LRO team agrees, suggesting that the scarps are due to a global cooling and shrinking of the Moon's radius by about 100 m. <br /> |
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| − | <em>[mailto:tychocrater@yahoo.com Chuck Wood]</em> <br /> | + | <em>[mailto:tychocrater@yahoo.com" rel="nofollow Chuck Wood]</em> <br /> |
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<strong>Technical Details</strong> <br /> | <strong>Technical Details</strong> <br /> | ||
| − | <em>Science</em> [http://www.sciencemag.org/cgi/content/abstract/329/5994/936 paper]. <br /> | + | <em>Science</em> [http://www.sciencemag.org/cgi/content/abstract/329/5994/936" rel="nofollow paper]. <br /> |
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| − | <div>Click the <strong>Discussion</strong> tab above. ---- The rotating globe shows locations of folks who visit LPOD. The most recent visits include location names - so you can see who else is on when you visit. For example, if you see "Wheeling/ West Virginia" I am probably editing an LPOD. After a few minutes just a small red dot appears. ---- You can support LPOD when you buy any book from Amazon thru [http://www.lpod.org/?page_id=591 LPOD!] | + | <div>Click the <strong>Discussion</strong> tab above. ---- The rotating globe shows locations of folks who visit LPOD. The most recent visits include location names - so you can see who else is on when you visit. For example, if you see "Wheeling/ West Virginia" I am probably editing an LPOD. After a few minutes just a small red dot appears. ---- You can support LPOD when you buy any book from Amazon thru [http://www.lpod.org/?page_id=591" rel="nofollow LPOD!] |
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===COMMENTS?=== | ===COMMENTS?=== | ||
Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment. | Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment. | ||
Revision as of 21:05, 4 January 2015
Continuing Deformation
image from " rel="nofollow NASA/LRO. Digital topographic map with black circles representing lobate scarps discovered during the Apollo era, and white dots newly discovered scarps seen on LRO image. Inset at bottom left is scarp at Gregory crater - the white circle near the equator at far right.
Teams flying spacecraft around a planet often rediscover what was found on previous missions. Press releases, or the way they are sensationalized by the press, sometimes seem to imply that the spacecraft has made a wondrous new discovery, when it is in fact merely an extension of what was learned earlier. This has happened repeatedly on Mars missions, and there is a tinge of it in recent press coverage of imaging of lunar lobate scarps by Lunar Reconnaissance Orbiter. The LRO team's press release states that such scarps were first discovered in Apollo images and the map shows the currently known distribution of Apollo (black circles) and LRO (white circle) scarps. Lobate scarps are interpreted as low angle thrust faults, places where one piece of crust slides up over adjacent terrain. They are typically only a few tens of meters high and nearly impossible to see from Earth; perhaps the only one imageable by amateurs is the Lincoln-Lee Scarp near the Apollo 17 landing site. Twenty-five years ago " rel="nofollow Alan Binder and Hanns Gunga discovered and studied most of the scarps now known and determined that they are very young (perhaps a few hundred million years) and represent recent tectonic activity. The LRO team agrees, suggesting that the scarps are due to a global cooling and shrinking of the Moon's radius by about 100 m.
" rel="nofollow Chuck Wood
Technical Details
Science " rel="nofollow paper.
COMMENTS?
Click on this icon File:PostIcon.jpg at the upper right to post a comment.
