Difference between revisions of "April 9, 2004"

From LPOD
Jump to: navigation, search
 
(2 intermediate revisions by the same user not shown)
Line 1: Line 1:
 
__NOTOC__
 
__NOTOC__
 
=Copernicus on the Limb=
 
=Copernicus on the Limb=
 +
<!-- Start of content -->
 
<table width="640"  border="0" align="center" cellpadding="6" cellspacing="2">
 
<table width="640"  border="0" align="center" cellpadding="6" cellspacing="2">
 
<tr>
 
<tr>
Line 39: Line 40:
 
[http://fmallmann.free.fr/ Mallmann Web Page]<br>
 
[http://fmallmann.free.fr/ Mallmann Web Page]<br>
 
[http://www.lpi.usra.edu/research/lunar_orbiter/images/img/iv_193_h2.jpg Lunar Orbiter IV View]</p>
 
[http://www.lpi.usra.edu/research/lunar_orbiter/images/img/iv_193_h2.jpg Lunar Orbiter IV View]</p>
<p class="story"> <b>Tomorrow's LPOD:</b> Another Farside View</p>
+
<p><b>Yesterday's LPOD:</b> [[April 8, 2004|Sneaky Schneckenberg]] </p>
 +
<p><b>Tomorrow's LPOD:</b> [[April 10, 2004|Another Farside View]] </p>
 
</td>
 
</td>
 
</tr>
 
</tr>
Line 55: Line 57:
 
<!-- Cleanup of credits -->
 
<!-- Cleanup of credits -->
 
<p>&nbsp;</p>
 
<p>&nbsp;</p>
----
+
<!-- End of content -->
===COMMENTS?===
+
{{wiki/ArticleFooter}}
Register, and click on the <b>Discussion</b> tab at the top of the page.
 
<hr>
 
<!--
 
You can support LPOD when you buy any book from Amazon thru [[Support_ LPOD|LPOD]]!
 
-->
 
<span style="font-size:88%">
 
<center>
 
Contributions to http://www2.lpod.org/ are licensed under a Creative Commons Attribution No-Derivative-Works Non-Commercial 3.0 License. [http://www.creativecommons.org/licenses/by-nc-nd/3.0 http://www.wikispaces.com/i/creativecommons/by-nc-nd_3.0_80x15.png]<br>
 
</center>
 
</span>
 

Latest revision as of 18:15, 7 February 2015

Copernicus on the Limb

LPOD-2004-04-09.jpeg

Image Credit: Frederic Mallmann

Copernicus on the Limb

Ya seen one crater, ya seen em all. Sometimes that's the way it feels. Because the energy involved in impact crater formation is so immense, craters of similar size and freshness look pretty much alike. For example, consider these two behemoths. The bottom crater is Copernicus, 93 km wide and famous for its great location for viewing from Earth. The top image is Housen, 167 km wide and hardly seen at all because its right on the southwest limb beyond Bailly. Despite the difference in diameters the craters look very similar - both have scarped walls with terraces that step down to the flat floor, which littered with central mountains. Fresh impact craters from 40 km in diameter to about 200 km look pretty similar. At larger sizes there is a transition to peak ring craters and then multi-ring basins.

Chuck Wood

Technical Details:

This magnificent image of Hausen (top) was taken by Frederic Mallmann using the 24" Cassegrain telescope at Ludiver Observatory in northern France on 19 Oct. 2003. The telescope worked at f/16 and infrared filter was used. A ToUcam was used with 1/25 s exposures and the best 400 of 2700 images were used.

Full details here:http://fmallmann.free.fr/dethaus.html

The Copernicus shot (bottom) was made with more expensive equipment: Apollo 17.

Related Links:
Mallmann Web Page
Lunar Orbiter IV View

Yesterday's LPOD: Sneaky Schneckenberg

Tomorrow's LPOD: Another Farside View


Author & Editor:
Charles A. Wood

 


COMMENTS?

Register, Log in, and join in the comments.