Difference between revisions of "May 31, 2011"

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<em>image by [mailto:tolentino@fumec.br Ricardo Jose Vaz Tolentino], Belo Horizonte / MG, Brazil</em><br />
 
<em>image by [mailto:tolentino@fumec.br Ricardo Jose Vaz Tolentino], Belo Horizonte / MG, Brazil</em><br />
 
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Why do impact craters so often have twin central peaks? From theory, nuclear bomb craters, and geology of terrestrial impact craters we understand that central peaks form by the rebound of a impact-generated pressure wave that lifts up buried strata. Ideally, I would imagine that the rebound is like a set of concentric circles, each inner one representing increasing intensity of uplift, with the center doming from the deepest depth and being most intensely shocked. I picture the peak as being a conical mountain with one summit. But the shadow inside Langrenus shows that it has two closely spaced peaks. Other examples are [http://www.lpod.org/?m=20060304 Philolaus] and [http://the-moon.wikispaces.com/Carpenter Carpenter]. In fact, many craters deviate from the ideal conical mountain mass. Many peaks are not centered in the crater, and sometimes there is more a field of hills than a massive rebounded peak. I suppose that local conditions of target rocks and the obliquity of impact affect the size, shape and location of <em>central</em> peaks, but those details have not been closely investigated.<br />
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Why do impact craters so often have twin central peaks? From theory, nuclear bomb craters, and geology of terrestrial impact craters we understand that central peaks form by the rebound of a impact-generated pressure wave that lifts up buried strata. Ideally, I would imagine that the rebound is like a set of concentric circles, each inner one representing increasing intensity of uplift, with the center doming from the deepest depth and being most intensely shocked. I picture the peak as being a conical mountain with one summit. But the shadow inside Langrenus shows that it has two closely spaced peaks. Other examples are [[March_4,_2006|Carpenter]]. In fact, many craters deviate from the ideal conical mountain mass. Many peaks are not centered in the crater, and sometimes there is more a field of hills than a massive rebounded peak. I suppose that local conditions of target rocks and the obliquity of impact affect the size, shape and location of <em>central</em> peaks, but those details have not been closely investigated.<br />
 
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<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br />
 
<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br />
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<strong>Related Links</strong><br />
 
<strong>Related Links</strong><br />
Rükl plate [http://the-moon.wikispaces.com/R%C3%BCkl+49 49]<br />
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Rükl plate [https://the-moon.us/wiki/R%C3%BCkl_49 49]<br />
 
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<p><b>Yesterday's LPOD:</b> [[May 30, 2011|Cratering a Cooling Liquid?]] </p>
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<p><b>Tomorrow's LPOD:</b> [[June 1, 2011|Color Clues]] </p>
 
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Latest revision as of 18:53, 13 October 2018

Peeking At Peaks

LPOD-May31-11.jpg
image by Ricardo Jose Vaz Tolentino, Belo Horizonte / MG, Brazil

Why do impact craters so often have twin central peaks? From theory, nuclear bomb craters, and geology of terrestrial impact craters we understand that central peaks form by the rebound of a impact-generated pressure wave that lifts up buried strata. Ideally, I would imagine that the rebound is like a set of concentric circles, each inner one representing increasing intensity of uplift, with the center doming from the deepest depth and being most intensely shocked. I picture the peak as being a conical mountain with one summit. But the shadow inside Langrenus shows that it has two closely spaced peaks. Other examples are Carpenter. In fact, many craters deviate from the ideal conical mountain mass. Many peaks are not centered in the crater, and sometimes there is more a field of hills than a massive rebounded peak. I suppose that local conditions of target rocks and the obliquity of impact affect the size, shape and location of central peaks, but those details have not been closely investigated.

Chuck Wood

Technical Details
2011 Feb 20, 06:26 UT; SkyWatcher 12" DOB + Celestron Ultima 2 X Barlow + ORION StarShoot Solar System Color Imager II; just one frame.

Related Links
Rükl plate 49

Yesterday's LPOD: Cratering a Cooling Liquid?

Tomorrow's LPOD: Color Clues



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