Difference between revisions of "January 30, 2004"

From LPOD
Jump to: navigation, search
 
(11 intermediate revisions by the same user not shown)
Line 1: Line 1:
 
__NOTOC__
 
__NOTOC__
 
=Lake of Death=
 
=Lake of Death=
 +
<!-- Start of content -->
 
<table width="85%"  border="0" align="center" cellpadding="6" cellspacing="2">
 
<table width="85%"  border="0" align="center" cellpadding="6" cellspacing="2">
 
<tr>
 
<tr>
Line 13: Line 14:
 
<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:kcpaulhk@yahoo.com.hk K.C. Pau]</div></td>
+
<td><div align="center"><p>Image Credit:  [mailto:kcpaulhk@yahoo.com.hk K.C. Pau]</p></div></td>
 
</tr>
 
</tr>
 
</table>
 
</table>
</p>
 
 
<table class="story" border="0" bgcolor="#FFFFFF" width="90%" cellpadding="10" align="center"><tr><td>
 
<table class="story" border="0" bgcolor="#FFFFFF" width="90%" cellpadding="10" align="center"><tr><td>
 
<p class="story" align="center"><b>Lake of Death</b></p>
 
<p class="story" align="center"><b>Lake of Death</b></p>
Line 27: Line 27:
 
the Imbrium basin. Notice also that the walls of Lacus Mortis do not define a circle or an ellipse - they have distinct  
 
the Imbrium basin. Notice also that the walls of Lacus Mortis do not define a circle or an ellipse - they have distinct  
 
straight edges. These linear wall segments are part of the lunar grid system, marked also by the polygonal sides of  
 
straight edges. These linear wall segments are part of the lunar grid system, marked also by the polygonal sides of  
Ptolemaeus, the [LPOD-2004-01-11.htm Straight Wall], the Alpine Valley and other straight features. Some  
+
Ptolemaeus, the [[January_11,_2004|Straight Wall]], the Alpine Valley and other straight features. Some  
 
of these linear features are related to basins, but others could have formed by tidal stressing early in lunar history  
 
of these linear features are related to basins, but others could have formed by tidal stressing early in lunar history  
 
when the Moon was much closer to Earth.  
 
when the Moon was much closer to Earth.  
 +
</p>
 
<p><b>Technical Details:</b><br>
 
<p><b>Technical Details:</b><br>
 
Imaged 18 July 2003 in Hong Kong with a 212 mm Newtonian Cassegrain and a 2x Barlow and Phillips Toucam Pro  
 
Imaged 18 July 2003 in Hong Kong with a 212 mm Newtonian Cassegrain and a 2x Barlow and Phillips Toucam Pro  
 
webcam. 212 frames were stacked and the seeing was good (8/10) and transparency fair (5/20). </p>
 
webcam. 212 frames were stacked and the seeing was good (8/10) and transparency fair (5/20). </p>
<p class"story"><b>Related Links:</b><br>
+
<p class="story"><b>Related Links:</b><br>
 
[http://observingthesky.org/index.php?p=174 KC Pau]<br>
 
[http://observingthesky.org/index.php?p=174 KC Pau]<br>
 
[http://www.lpi.usra.edu/research/lunar_orbiter/images/img/iv_091_h2.jpg Lunar Orbiter image]</p>
 
[http://www.lpi.usra.edu/research/lunar_orbiter/images/img/iv_091_h2.jpg Lunar Orbiter image]</p>
<p class"story"> <b>Tomorrow's LPOD:</b> Hooke &amp; Hipparchus</p>
+
<p><b>Yesterday's LPOD:</b> [[January 29, 2004|Nodding Moon]] </p>
<p><img src="../../../MainPage/spacer.gif" width="640" height="1"></p></td></tr>
+
<p><b>Tomorrow's LPOD:</b> [[January 31, 2004|Hooke & Hipparchus]] </p>
 
</table>
 
</table>
</td>
 
</tr>
 
<tr>
 
<td colspan="2" rowspan="1">
 
 
<!-- start bottom -->
 
<!-- start bottom -->
 
<table width="100%"  border="0" cellspacing="2" cellpadding="4">
 
<table width="100%"  border="0" cellspacing="2" cellpadding="4">
 
<tr>
 
<tr>
<td><hr width="640"></td>
+
<td><hr></td>
 
</tr>
 
</tr>
 
<tr>
 
<tr>
 
<td><p align="center" class="main_titles"><b>Author & Editor:</b><br>
 
<td><p align="center" class="main_titles"><b>Author & Editor:</b><br>
[mailto:chuck@observingthesky.org Charles A. Wood]</p>
+
[mailto:tychocrater@yahoo.com Charles A. Wood]</p>
<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>
+
<!-- Cleanup of credits -->
[http://www.observingthesky.org/ ObservingTheSky.Org]</p>
+
<!-- Cleanup of credits -->
<p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
+
<!-- Cleanup of credits -->
[http://antwrp.gsfc.nasa.gov/apod/astropix.html Astronomy] | [http://www.msss.com/ Mars] | [http://epod.usra.edu/ Earth]</p></td>
+
<!-- Cleanup of credits -->
 
</tr>
 
</tr>
 
</table>
 
</table>
 
<p>&nbsp;</p>
 
<p>&nbsp;</p>
----
+
<!-- End of content -->
===COMMENTS?===
+
{{wiki/ArticleFooter}}
Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment.
 

Latest revision as of 18:11, 7 February 2015

Lake of Death

LPOD-2004-01-30.jpeg

Image Credit: K.C. Pau

Lake of Death

Do you consider Lacus Mortis - The Lake of Death - a crater? Because of the mare-like term "lacus" some observers just see it as a patch of mare material linking Mare Frigoris and Lacus Somniorum. But if you linger, taking your eyes off the challenging rilles and superposed crater Burg, you will easily notice low walls that enclose nearly the entire lake. I say "walls" rather than "rim" for the latter term implies a rampart that projects above the surrounding environs, and these don't. Lacus Mortis is a depression lower than most of its surroundings, especially the rubbly plateau to the west. Notice the faint diagonal lineations in the rubbly material? They are probably flow marks in this jumble of ejecta from the Imbrium basin. Notice also that the walls of Lacus Mortis do not define a circle or an ellipse - they have distinct straight edges. These linear wall segments are part of the lunar grid system, marked also by the polygonal sides of Ptolemaeus, the Straight Wall, the Alpine Valley and other straight features. Some of these linear features are related to basins, but others could have formed by tidal stressing early in lunar history when the Moon was much closer to Earth.

Technical Details:
Imaged 18 July 2003 in Hong Kong with a 212 mm Newtonian Cassegrain and a 2x Barlow and Phillips Toucam Pro webcam. 212 frames were stacked and the seeing was good (8/10) and transparency fair (5/20).

Related Links:
KC Pau
Lunar Orbiter image

Yesterday's LPOD: Nodding Moon

Tomorrow's LPOD: Hooke & Hipparchus


Author & Editor:
Charles A. Wood

 


COMMENTS?

Register, Log in, and join in the comments.