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| | =Waves of Rings= | | =Waves of Rings= |
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| + | <p> [[File:Stefan-hippalus.jpg|Stefan-hippalus.jpg]]</p> |
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| − | <p> [[File:Stefan-hippalus.jpg|Stefan-hippalus.jpg]]</p> | |
| | <p><em>image by [mailto:slamm@blueyonder.co.uk Stefan Lammel], Uxbridge, England</em></p> | | <p><em>image by [mailto:slamm@blueyonder.co.uk Stefan Lammel], Uxbridge, England</em></p> |
| | <p> | | <p> |
| − | [http://www.lpod.org/?m=20070508 Nectaris] and Humorum have the best exposed concentric structures of any impact basins on the lunar nearside. Nectaris has a huge partial rim - the [http://www.lpod.org/?m=20061022 Altai Scarp] - and arcs of two more inner rings. Humorum doesn’t have massive mountainous rings as much as concentric rilles and mare ridges, beautifully seen in Stefan’s recent image. The reasons for the differences in these basins is totally unknown. When a small impact event occurs, the resulting few kilometers wide craters are so similar they could have been turned out on a lathe. But surprisingly the prodigious impacts that produced impact basins create structures of surprisingly diverse character. Perhaps small craters look so similar because they each form in a fairly homogeneous patch of crustal rocks, but basins are each unique because they excavate into large areas that encompasses multiple rock types and history. I am speculating that the energy of impact is less important than crustal structure in determining the looks of craters and basins. | + | [[May_8,_2007|Nectaris]] and Humorum have the best exposed concentric structures of any impact basins on the lunar nearside. Nectaris has a huge partial rim - the [[October_22,_2006|Altai Scarp]] - and arcs of two more inner rings. Humorum doesn’t have massive mountainous rings as much as concentric rilles and mare ridges, beautifully seen in Stefan’s recent image. The reasons for the differences in these basins is totally unknown. When a small impact event occurs, the resulting few kilometers wide craters are so similar they could have been turned out on a lathe. But surprisingly the prodigious impacts that produced impact basins create structures of surprisingly diverse character. Perhaps small craters look so similar because they each form in a fairly homogeneous patch of crustal rocks, but basins are each unique because they excavate into large areas that encompasses multiple rock types and history. I am speculating that the energy of impact is less important than crustal structure in determining the looks of craters and basins. |
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| | <p>[mailto:tychocrater@yahoo.com Chuck Wood]</p> | | <p>[mailto:tychocrater@yahoo.com Chuck Wood]</p> |
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| | Rükl charts 52 & 53 <br /> | | Rükl charts 52 & 53 <br /> |
| | [http://www.slamm.pwp.blueyonder.co.uk/moon/moon.htm Stefan’s website]</p> | | [http://www.slamm.pwp.blueyonder.co.uk/moon/moon.htm Stefan’s website]</p> |
| − | <div align="center"><strong>Don’t forget to add yourself - as I have done - to the growing list (91 so far) of lunatics at [http://www.lpod.org/?m=20070509 Frappr LPOD]!</strong></p> | + | <p><b>Yesterday's LPOD:</b> [[May 17, 2007|A New Fault]] </p> |
| − | <p><em>LPOD earns a commision when you buy ANY book from Amazon thru [[LPOD]] Have you bought a book lately?</em></div></p> | + | <p><b>Tomorrow's LPOD:</b> [[May 19, 2007|Lavafall Over a Low Nose?]] </p> |
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| − | ===COMMENTS?===
| + | <p> </p> |
| − | Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment.
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