Difference between revisions of "August 31, 2004"

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=Archimedes and his Mountains=
 
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      <td><div align="center" class="main_sm">Image Credit: [mailto:kcpaulhk@yahoo.com.hk" class="one K.C. Pau ] </div></td>
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<td><div align="center" class="main_sm">Image Credit: [mailto:kcpaulhk@yahoo.com.hk" class="one K.C. Pau ] </div></td>
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  <p class="story" align="center"><b>Archimedes and his Mountains</b></p>
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<p class="story" align="center"><b>Archimedes and his Mountains</b></p>
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[http://www.lpod.org/archive/2004/04/LPOD-2004-04-05.htm Archimedes]  is the largest crater inside the Imbrium Basin (Sinus Iridum is bigger but its on the rim rather than inside). But I don't think it is observed much because its floor lacks a central peak and its small pits, unlike [http://www.lpod.org/archive/2004/01/LPOD-2004-01-24.htm Plato's],  haven't become known as a test for  seeing and optics. But south of Archimedes is an area that is even less often observed. The Archimedes Mountains are two crude arcs that run NE to SW, with a gentle curve inwards towards Imbrium. These mountains appear to be part of a 790 km wide inner ring of the Imbrium Basin, probably formed as a mega-terrace, as massive arcs of land slumped toward the hole created by the Imbrium impact. The mountains are in the midst of an area of low hills and small craters. This surface, lighter than nearby mare, is an area of KREEP volcanism called the Apennine Bench. This volcanic material was erupted onto the floor of the Imbrium basin and later was surrounded by normal mare basalts.   
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[http://www.lpod.org/archive/2004/04/LPOD-2004-04-05.htm Archimedes]  is the largest crater inside the Imbrium Basin (Sinus Iridum is bigger but its on the rim rather than inside). But I don't think it is observed much because its floor lacks a central peak and its small pits, unlike [http://www.lpod.org/archive/2004/01/LPOD-2004-01-24.htm Plato's],  haven't become known as a test for  seeing and optics. But south of Archimedes is an area that is even less often observed. The Archimedes Mountains are two crude arcs that run NE to SW, with a gentle curve inwards towards Imbrium. These mountains appear to be part of a 790 km wide inner ring of the Imbrium Basin, probably formed as a mega-terrace, as massive arcs of land slumped toward the hole created by the Imbrium impact. The mountains are in the midst of an area of low hills and small craters. This surface, lighter than nearby mare, is an area of KREEP volcanism called the Apennine Bench. This volcanic material was erupted onto the floor of the Imbrium basin and later was surrounded by normal mare basalts.   
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    <p align="right"> &#8212; [mailto:chuck@observingthesky.org Chuck Wood ]</p>
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<p align="right"> &#8212; [mailto:tychocrater@yahoo.com Chuck Wood ]</p>
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  <p><b>Technical Details:</b><br>
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<p><b>Technical Details:</b><br>
    Aug 7, 2004, 10&quot; f/6 Newtonian + 5X Barlow + Phillips Toucam Pro, 3 image mosaic.<br>
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Aug 7, 2004, 10&quot; f/6 Newtonian + 5X Barlow + Phillips Toucam Pro, 3 image mosaic.<br>
    KREEP = Potassium, rare-earth elements and phosphorus rich basalts unique to the Imbrium area. </p>
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KREEP = Potassium, rare-earth elements and phosphorus rich basalts unique to the Imbrium area. </p>
  <p><b>Related Links: </b><br>
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<p><b>Related Links: </b><br>
        [http://www.lpi.usra.edu/meetings/LPSC98/pdf/1352.pdf Geology and Composition of the Apennine Mountains]  <br>
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[http://www.lpi.usra.edu/meetings/LPSC98/pdf/1352.pdf Geology and Composition of the Apennine Mountains]  <br>
        [http://www.lpi.usra.edu/research/lunar_orbiter/images/img/iv_109_h3.jpg Lunar Orbiter IV View] </p>
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[http://www.lpi.usra.edu/research/lunar_orbiter/images/img/iv_109_h3.jpg Lunar Orbiter IV View] </p>
  <p><b>Tomorrow's LPOD:</b> Hundred Year Old Hevel</p>
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<p><b>Tomorrow's LPOD:</b> Hundred Year Old Hevel</p>
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      <td><p align="center" class="main_titles"><b>Author & Editor:</b><br>
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<td><p align="center" class="main_titles"><b>Author & Editor:</b><br>
          [mailto:chuck@observingthesky.org Charles A. Wood]</p>
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[mailto:tychocrater@yahoo.com Charles A. Wood]</p>
        <p align="center" class="main_titles"><b>Technical Consultant:</b><br>
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<p align="center" class="main_titles"><b>Technical Consultant:</b><br>
            [mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
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[mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
        <p align="center" class="main_titles"><b>[mailto:webmaster@entropysponge.com Contact Webmaster]</b></p>
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<p align="center" class="main_titles"><b>A service of:</b><br>
        <p align="center" class="main_titles"><b>A service of:</b><br>
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[http://www.observingthesky.org/ ObservingTheSky.Org]</p>
            <a class="one" href="http://www.observingthesky.org/">ObservingTheSky.Org</a></p>
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<p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
        <p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
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[http://antwrp.gsfc.nasa.gov/apod/astropix.html Astronomy] | [http://www.msss.com/ Mars] | [http://epod.usra.edu/ Earth]</p>
          <a class="one" href="http://antwrp.gsfc.nasa.gov/apod/astropix.html">Astronomy</a> | <a class="one" href="http://www.msss.com/">Mars</a> | <a class="one" href="http://epod.usra.edu/">Earth</a></p>
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===COMMENTS?===  
 
===COMMENTS?===  
 
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Revision as of 17:24, 4 January 2015

Archimedes and his Mountains


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Archimedes and his Mountains

Archimedes is the largest crater inside the Imbrium Basin (Sinus Iridum is bigger but its on the rim rather than inside). But I don't think it is observed much because its floor lacks a central peak and its small pits, unlike Plato's, haven't become known as a test for seeing and optics. But south of Archimedes is an area that is even less often observed. The Archimedes Mountains are two crude arcs that run NE to SW, with a gentle curve inwards towards Imbrium. These mountains appear to be part of a 790 km wide inner ring of the Imbrium Basin, probably formed as a mega-terrace, as massive arcs of land slumped toward the hole created by the Imbrium impact. The mountains are in the midst of an area of low hills and small craters. This surface, lighter than nearby mare, is an area of KREEP volcanism called the Apennine Bench. This volcanic material was erupted onto the floor of the Imbrium basin and later was surrounded by normal mare basalts.

Chuck Wood

Technical Details:
Aug 7, 2004, 10" f/6 Newtonian + 5X Barlow + Phillips Toucam Pro, 3 image mosaic.
KREEP = Potassium, rare-earth elements and phosphorus rich basalts unique to the Imbrium area.

Related Links:
Geology and Composition of the Apennine Mountains
Lunar Orbiter IV View

Tomorrow's LPOD: Hundred Year Old Hevel



Author & Editor:
Charles A. Wood

Technical Consultant:
Anthony Ayiomamitis

A service of:
ObservingTheSky.Org

Visit these other PODs:
Astronomy | Mars | Earth

 


COMMENTS?

Click on this icon File:PostIcon.jpg at the upper right to post a comment.