Difference between revisions of "April 17, 2004"

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=Cassini North=
 
=Cassini North=
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      <td width="50%"><h2 align="left">Cassini North</h2></td>
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  <td width="50%"><h2 align="right">April  17, 2004</h2></td>
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      <td colspan="2"><div align="center">
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    [javascript:;" onMouseOver="MM_swapImage('main_image','','images/LPOD-2004-04-17b.jpeg',1)" onMouseOut="MM_swapImgRestore() <IMG SRC="images/LPOD-2004-04-17.jpeg" NAME="main_image" width="327" height="425" border="0">]</div>
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<table width="100%"  border="0" cellpadding="8">
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      <td><div align="center" span class="main_sm">Image Credit:  [mailto:leecht@earthlink.net Tom Leech]</div></td>
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<table class="story" border="0" bgcolor="#FFFFFF" width="90%" cellpadding="10" align="center"><tr><td>
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  <p class="story" align="center"><b>Cassini North </b></p>
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  <p class="story" align="left">Cassini is an unusual looking crater. I think its because it is surrounded by Imbrium lavas so there is an abrupt boundary with its near rim deposits, and because it is filled with lava nearly to its rim. Cassini is a more extreme version of Archimedes. The interior of Cassini (diameter 57 km, depth 1.3 km) has peculiar hills and coarse rilles just inside its eastern rim - they don't look like remnants of a terraced wall. Along its northwest inner wall a weird little worm-like feature goes from the floor over the rim. The Lunar Orbiter IV view doesn't clarify the origin of this worm. The area north of Cassini is the lunar Alps with a front of massive mountainous blocks (massifs) and much smaller scattered hills behind. The Alps are probably crustal rocks uplifted by the Imbrium basin formation, and the smaller hills are ejecta fallback from the event. There was more than just fallback going on though. On the mouseover you will see various sets of white lines that highlight linear features in the Alpes Formation (as the US Geological Survey calls it). Some lines are radial to the Imbrium basin - they probably represent crustal fractures as the pre-existing rocks were being domed up in response to the impact &quot;explosion.&quot; Other lines, nearly at right angles to the radial set, define a linear trough that has subsided - it is filled with lavas in places. I wonder if this is equivalent to a terrace in an impact crater? Look around this marvelous image by Tom Leech to find other details we don't fully understand - it's not that they are mysteries, rather the cratering process is very complicated; we need to examine this stuff on the ground!<BR>
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  <blockquote>
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    <p align="right" class="story">&#8212; [mailto:chuck@observingthesky.org Chuck Wood]</p>
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  </blockquote>  <p><b>Technical Details:</b><br>
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  Here is a shot of Cassini taken on day 6? of the present lunar cycle [CAW - March 26?]  with a C-14, Toucam Pro 740k, k3ccdtools, 119 frames combined in Registax 1.</p>
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  <p class"story"><b>Related Links:</b><br>
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[http://www.lpi.usra.edu/meetings/LPSC99/pdf/1348.pdf Deposits of Imbrium Basin]<br>
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[http://www.lpi.usra.edu/research/lunar_orbiter/images/img/iv_110_h2.jpg Cassini Crater on the Moon (LO IV)]<br>
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[http://www.msss.com/moc_gallery/e13_e18/images/E18/E1800638.html Cassini Crater on Mars (impact)]<br>
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[http://homepage2.nifty.com/gradation/3dcg/vistapro2/mars/cassini_crater.html Cassini Crater in Arabia (probably not impact)] </p>
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  <p class"story"> <b>Tomorrow's LPOD:</b> Langrenus</p>
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  <p><img src="../../../MainPage/spacer.gif" width="640" height="1"></p>
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  <!-- start bottom -->
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  <hr width="640">
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  <p align="center" class="main_titles"><b>Author & Editor:</b><br>
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      [mailto:chuck@observingthesky.org Charles A. Wood]</p>
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      <p align="center" class="main_titles"><b>Technical Consultant:</b><br>
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      [mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
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      <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>
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      <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>
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      <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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  <p>&nbsp;</p>
  
  

Revision as of 15:37, 4 January 2015

Cassini North

Cassini North

April 17, 2004

[javascript:;" onMouseOver="MM_swapImage('main_image',,'images/LPOD-2004-04-17b.jpeg',1)" onMouseOut="MM_swapImgRestore() <IMG SRC="images/LPOD-2004-04-17.jpeg" NAME="main_image" width="327" height="425" border="0">]
Image Credit: Tom Leech

Cassini North

Cassini is an unusual looking crater. I think its because it is surrounded by Imbrium lavas so there is an abrupt boundary with its near rim deposits, and because it is filled with lava nearly to its rim. Cassini is a more extreme version of Archimedes. The interior of Cassini (diameter 57 km, depth 1.3 km) has peculiar hills and coarse rilles just inside its eastern rim - they don't look like remnants of a terraced wall. Along its northwest inner wall a weird little worm-like feature goes from the floor over the rim. The Lunar Orbiter IV view doesn't clarify the origin of this worm. The area north of Cassini is the lunar Alps with a front of massive mountainous blocks (massifs) and much smaller scattered hills behind. The Alps are probably crustal rocks uplifted by the Imbrium basin formation, and the smaller hills are ejecta fallback from the event. There was more than just fallback going on though. On the mouseover you will see various sets of white lines that highlight linear features in the Alpes Formation (as the US Geological Survey calls it). Some lines are radial to the Imbrium basin - they probably represent crustal fractures as the pre-existing rocks were being domed up in response to the impact "explosion." Other lines, nearly at right angles to the radial set, define a linear trough that has subsided - it is filled with lavas in places. I wonder if this is equivalent to a terrace in an impact crater? Look around this marvelous image by Tom Leech to find other details we don't fully understand - it's not that they are mysteries, rather the cratering process is very complicated; we need to examine this stuff on the ground!

Chuck Wood

Technical Details:
Here is a shot of Cassini taken on day 6? of the present lunar cycle [CAW - March 26?] with a C-14, Toucam Pro 740k, k3ccdtools, 119 frames combined in Registax 1.

Related Links:
Deposits of Imbrium Basin
Cassini Crater on the Moon (LO IV)
Cassini Crater on Mars (impact)
Cassini Crater in Arabia (probably not impact)

Tomorrow's LPOD: Langrenus

<img src="../../../MainPage/spacer.gif" width="640" height="1">


Author & Editor:
Charles A. Wood

Technical Consultant:
Anthony Ayiomamitis

Contact Webmaster

A service of:
<a class="one" href="http://www.observingthesky.org/">ObservingTheSky.Org</a>

Visit these other PODs:
<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>

 



COMMENTS?

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