Difference between revisions of "June 23, 2004"

From LPOD
Jump to: navigation, search
 
(10 intermediate revisions by the same user not shown)
Line 1: Line 1:
 
__NOTOC__
 
__NOTOC__
 
=Concentric Craters=
 
=Concentric Craters=
 
+
<!-- Start of content -->
      </p>
+
<table width="640"  border="0" align="center" cellpadding="6" cellspacing="2">
<table width="640"  border="0" align="center" cellpadding="6" cellspacing="2">
+
<tr>
    <tr>
+
</tr>
      <td><h2 align="left">Concentric Craters</h2></td>
+
</table>
      <td><h2 align="right">June 23, 2004</h2></td>
+
<table width="85%"  border="0" align="center" cellpadding="6" cellspacing="2">
    </tr>
+
<tr>
</table>
+
<td colspan="2"><div align="center">
<table width="85%"  border="0" align="center" cellpadding="6" cellspacing="2">
+
[[File:LPOD-2004-06-23.jpeg|LPOD-2004-06-23.jpeg]]</div></td>
    <tr>
+
</tr>
      <td colspan="2"><div align="center">
 
  <IMG SRC="images/LPOD-2004-06-23.jpeg" NAME="main_image" width="441" height="424" border="0"></div></td>
 
    </tr>
 
 
</table>
 
</table>
 
<table width="100%"  border="0" cellpadding="8">
 
<table width="100%"  border="0" cellpadding="8">
    <tr>
+
<tr>
      <td><div align="center" span class="main_sm">Image Credit:  [mailto:cwood@observingthesky.org" class="one Chuck Wood]  &amp; [http://www.lpi.usra.edu/research/lunar_orbiter/" class="one Luna Orbiter IV] </div></td>
+
<td><div align="center"><p>Image Credit:  [mailto:tychocrater@yahoo.com Chuck Wood]</p></div></td>
    </tr>
+
</tr>
  </table>
 
</p>
 
  <table class="story" border="0" bgcolor="#FFFFFF" width="90%" cellpadding="10" align="center"><tr><td>
 
  <p class="story" align="center"><b>Concentric Craters</b></p>
 
  <p class="story" align="left">The nearside of the Moon contains more than 11,000 craters larger than 3.5 km wide. Virtually all of them are standard impact craters, mostly small, ranging from very fresh to quite degraded.
 
  There are a handful of oddball craters and one of the weirdest and least studied are concentric craters. These are small craters - on average 8 km in diameter, that contain an inner ring approximately half the crater width.
 
  The most famous concentric crater is Hesiodus A on the south shore of Mare Nubium. According to a paper I published in 1978 (see link) Hesiodus A is 14.9 km wide, 1.7 km deep impact crater, surrounded by a faint ejecta blanket.
 
  Inside Hesiodus A is a 6 km wide donut-like ring. back in 1978 I cataloged 51 concentric craters and 70% looked similar to Hesiodus A.  It is strongly unlikely that these bulls-eye crater within crater structures formed by
 
  two unrelated chance impacts. A number of the craters are located near domes and rilles, and 70% occur on the margins of maria. These spatial relations suggested to me that the inner rings were volcanic in origin. Perhaps an
 
  effusive flow of relatively viscous magma from fractures at the edge of the crater's floors built up the inner rings. Today, this interpretation is not very compelling to me as it was 26 years ago. But, suggestions that the
 
  rings are some sort of wall slump features within normal impact craters is also unbuttressed by any significant evidence. I don't know how to interpret concentric craters - do you?
 
 
 
<p class"story"><b>Related Links:</b><br>
 
 
 
 
 
 
 
 
 
  [http://adsbit.harvard.edu/cgi-bin/nph-iarticle_query?1978LPI.....9.1264W  Lunar Concentric Craters 1978 Paper] 
 
  </p>
 
  <p class"story"> <b>Tomorrow's LPOD:</b> Gambart Environs</p>
 
  <p><img src="../../../MainPage/spacer.gif" width="640" height="1"></p></td></tr>
 
 
</table>
 
</table>
    
+
<table class="story" border="0" bgcolor="#FFFFFF" width="90%" cellpadding="10" align="center"><tr><td>
</td>
+
<p class="story" align="center"><b>Concentric Craters</b></p>
  </tr>
+
<p class="story" align="left">The nearside of the Moon contains more than 11,000 craters larger than 3.5 km wide. Virtually all of them are standard impact craters, mostly small, ranging from very fresh to quite degraded.
 
+
There are a handful of oddball craters and one of the weirdest and least studied are concentric craters. These are small craters - on average 8 km in diameter, that contain an inner ring approximately half the crater width.
 +
The most famous concentric crater is Hesiodus A on the south shore of Mare Nubium. According to a paper I published in 1978 (see link) Hesiodus A is 14.9 km wide, 1.7 km deep impact crater, surrounded by a faint ejecta blanket.
 +
Inside Hesiodus A is a 6 km wide donut-like ring. back in 1978 I cataloged 51 concentric craters and 70% looked similar to Hesiodus A.  It is strongly unlikely that these bulls-eye crater within crater structures formed by
 +
two unrelated chance impacts. A number of the craters are located near domes and rilles, and 70% occur on the margins of maria. These spatial relations suggested to me that the inner rings were volcanic in origin. Perhaps an
 +
effusive flow of relatively viscous magma from fractures at the edge of the crater's floors built up the inner rings. Today, this interpretation is not very compelling to me as it was 26 years ago. But, suggestions that the
 +
rings are some sort of wall slump features within normal impact craters is also unbuttressed by any significant evidence. I don't know how to interpret concentric craters - do you?
 +
</p>
 +
<p class="story"><b>Related Links:</b><br>
 +
[http://adsbit.harvard.edu/cgi-bin/nph-iarticle_query?1978LPI.....9.1264W  Lunar Concentric Craters 1978 Paper]    
 +
</p>
 +
<p><b>Yesterday's LPOD:</b> [[June 22, 2004|A Fundamental Relation]] </p>
 +
<p><b>Tomorrow's LPOD:</b> [[June 24, 2004|Gambart Environs]] </p>
 +
</table>
 +
<!-- start bottom -->
 +
<table width="100%"  border="0" cellspacing="2" cellpadding="4">
 
<tr>
 
<tr>
  <td colspan="2" rowspan="1">
+
<td><hr></td>
  <!-- start bottom -->
+
</tr>
  <table width="100%"  border="0" cellspacing="2" cellpadding="4">
+
<tr>
    <tr>
+
<td><p align="center" class="main_titles"><b>Author & Editor:</b><br>
      <td><hr width="640"></td>
+
[mailto:tychocrater@yahoo.com Charles A. Wood]</p>
      </tr>
+
<!-- Cleanup of credits -->
    <tr>
+
<!-- Cleanup of credits -->
      <td><p align="center" class="main_titles"><b>Author & Editor:</b><br>
+
<!-- Cleanup of credits -->
          [mailto:chuck@observingthesky.org Charles A. Wood]</p>
+
<!-- Cleanup of credits -->
        <p align="center" class="main_titles"><b>Technical Consultant:</b><br>
+
<!-- Cleanup of credits -->
            [mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
+
<!-- Cleanup of credits -->
        <p align="center" class="main_titles"><b>[mailto:webmaster@entropysponge.com Contact Webmaster]</b></p>
+
<!-- Cleanup of credits -->
        <p align="center" class="main_titles"><b>A service of:</b><br>
+
</tr>
            <a class="one" href="http://www.observingthesky.org/">ObservingTheSky.Org</a></p>
+
</table>
        <p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
+
<!-- end cal -->
          <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></td>
+
<div align="center"></div>
      </tr>
 
  </table>
 
  <!-- end cal -->
 
  <div align="center"></div></td>
 
  </table>
 
 
 
 
<p>&nbsp;</p>
 
<p>&nbsp;</p>
 
+
<!-- End of content -->
 
+
{{wiki/ArticleFooter}}
 
 
----
 
===COMMENTS?===
 
Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment.
 

Latest revision as of 19:20, 7 February 2015

Concentric Craters

LPOD-2004-06-23.jpeg

Image Credit: Chuck Wood

Concentric Craters

The nearside of the Moon contains more than 11,000 craters larger than 3.5 km wide. Virtually all of them are standard impact craters, mostly small, ranging from very fresh to quite degraded. There are a handful of oddball craters and one of the weirdest and least studied are concentric craters. These are small craters - on average 8 km in diameter, that contain an inner ring approximately half the crater width. The most famous concentric crater is Hesiodus A on the south shore of Mare Nubium. According to a paper I published in 1978 (see link) Hesiodus A is 14.9 km wide, 1.7 km deep impact crater, surrounded by a faint ejecta blanket. Inside Hesiodus A is a 6 km wide donut-like ring. back in 1978 I cataloged 51 concentric craters and 70% looked similar to Hesiodus A. It is strongly unlikely that these bulls-eye crater within crater structures formed by two unrelated chance impacts. A number of the craters are located near domes and rilles, and 70% occur on the margins of maria. These spatial relations suggested to me that the inner rings were volcanic in origin. Perhaps an effusive flow of relatively viscous magma from fractures at the edge of the crater's floors built up the inner rings. Today, this interpretation is not very compelling to me as it was 26 years ago. But, suggestions that the rings are some sort of wall slump features within normal impact craters is also unbuttressed by any significant evidence. I don't know how to interpret concentric craters - do you?

Related Links:
Lunar Concentric Craters 1978 Paper

Yesterday's LPOD: A Fundamental Relation

Tomorrow's LPOD: Gambart Environs


Author & Editor:
Charles A. Wood

 


COMMENTS?

Register, Log in, and join in the comments.