Difference between revisions of "April 26, 2005"
| (9 intermediate revisions by the same user not shown) | |||
| Line 1: | Line 1: | ||
__NOTOC__ | __NOTOC__ | ||
=More Spectacular Flows in Imbrium= | =More Spectacular Flows in Imbrium= | ||
| + | <!-- 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> | ||
| − | |||
</tr> | </tr> | ||
</table> | </table> | ||
<table width="85%" border="0" align="center" cellpadding="6" cellspacing="2"> | <table width="85%" border="0" align="center" cellpadding="6" cellspacing="2"> | ||
<tr><td colspan="2" valign="top"><div align="center"> | <tr><td colspan="2" valign="top"><div align="center"> | ||
| − | + | <!-- Mouse style 1 --> | |
| − | + | {{HoverImage|LPOD-2005-04-26.jpeg|LPOD-2005-04-26b.jpeg}} | |
| − | |||
| − | |||
</div></td> | </div></td> | ||
</tr> | </tr> | ||
</table> | </table> | ||
<table width="80%" border="0" align="center" cellpadding="8"> | <table width="80%" border="0" align="center" cellpadding="8"> | ||
| − | <tr><td><div align="center" class="main_sm">Image Credit: [mailto:kcpaulhk@yahoo.com.hk K.C. Pau]</p> | + | <tr><td><div align="center" class="main_sm"><p>Image Credit: [mailto:kcpaulhk@yahoo.com.hk K.C. Pau]</p> |
</div></td> | </div></td> | ||
</tr> | </tr> | ||
| Line 23: | Line 21: | ||
<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 align="center"><b>More Spectacular Flows in Imbrium</b></p> | <p align="center"><b>More Spectacular Flows in Imbrium</b></p> | ||
| − | <p align="left">The lava flow in Mare Imbrium shown in a recent [ | + | <p align="left">The lava flow in Mare Imbrium shown in a recent [[April_23,_2005|LPOD]] is the most conspicuous, but not the only flow, and certainly not the longest one. KC Pau has now provided yet another astonishing image of Imbrium lava flows. In this highly stretched image, flow #1 (see mouseover) is the flow shown previously, and #2 is a slightly older, and much longer one, that still has well-preserved margins. Flow #3 also has a identifiable margns, but #4 is only definable because of the texture difference to its right. Flows appear to emerge from two low ridges which may be the fissure vents that fed the flows. The lava flows are estimated from crater counts to be possibly only 2.5 b.y.old, much younger than most of the lava flows in Imbrium and elsewhere on the Moon. These flows have never before been photographed so distinctly from Earth! WOW! |
</p> | </p> | ||
| − | <blockquote><p align="right">— [mailto:tychocrater@yahoo.com Chuck Wood]</blockquote> | + | <blockquote> |
| − | <p align="left" | + | <p align="right">— [mailto:tychocrater@yahoo.com Chuck Wood]</p></blockquote> |
| + | <p align="left"><b>Technical Details:</b><br> | ||
April 18, 2005. 10" f/6 Newtonian + 5X barlow + Philips Toucam Pro. Seeing was 6/10.</p> | April 18, 2005. 10" f/6 Newtonian + 5X barlow + Philips Toucam Pro. Seeing was 6/10.</p> | ||
<p><b>Related Links:</b><br> | <p><b>Related Links:</b><br> | ||
| Line 32: | Line 31: | ||
] | ] | ||
<br>Rukl Plates 10, 20 | <br>Rukl Plates 10, 20 | ||
| − | <p | + | </p> |
| + | <p><b>Yesterday's LPOD:</b> [[April 25, 2005|A Chain of Mystery]] </p> | ||
| + | <p><b>Tomorrow's LPOD:</b> [[April 27, 2005|A Busy Place]] </p> | ||
</tr> | </tr> | ||
</table> | </table> | ||
| Line 43: | Line 44: | ||
<p align="center" class="main_titles"><b>Author & Editor:</b><br> | <p align="center" class="main_titles"><b>Author & Editor:</b><br> | ||
[mailto:tychocrater@yahoo.com Charles A. Wood]</p> | [mailto:tychocrater@yahoo.com Charles A. Wood]</p> | ||
| − | < | + | <!-- Cleanup of credits --> |
| − | + | <!-- Cleanup of credits --> | |
| − | < | + | <!-- Cleanup of credits --> |
| − | + | <!-- Cleanup of credits --> | |
| − | + | <!-- Cleanup of credits --> | |
| − | < | + | <!-- Cleanup of credits --> |
| − | < | + | <!-- Cleanup of credits --> |
| − | + | <!-- Cleanup of credits --> | |
| − | < | + | <!-- Cleanup of credits --> |
| − | + | <!-- Cleanup of credits --> | |
</td></tr> | </td></tr> | ||
</table> | </table> | ||
<p> </p> | <p> </p> | ||
| − | ---- | + | <!-- End of content --> |
| − | + | {{wiki/ArticleFooter}} | |
| − | |||
Latest revision as of 14:14, 15 March 2015
More Spectacular Flows in Imbrium
|
Image Credit: K.C. Pau |
|
More Spectacular Flows in Imbrium The lava flow in Mare Imbrium shown in a recent LPOD is the most conspicuous, but not the only flow, and certainly not the longest one. KC Pau has now provided yet another astonishing image of Imbrium lava flows. In this highly stretched image, flow #1 (see mouseover) is the flow shown previously, and #2 is a slightly older, and much longer one, that still has well-preserved margins. Flow #3 also has a identifiable margns, but #4 is only definable because of the texture difference to its right. Flows appear to emerge from two low ridges which may be the fissure vents that fed the flows. The lava flows are estimated from crater counts to be possibly only 2.5 b.y.old, much younger than most of the lava flows in Imbrium and elsewhere on the Moon. These flows have never before been photographed so distinctly from Earth! WOW! Technical Details: Related Links: Yesterday's LPOD: A Chain of Mystery Tomorrow's LPOD: A Busy Place |
Ap 15 Extreme Closeup of Flow #1
]
|
Author & Editor: |
COMMENTS?
Register, Log in, and join in the comments.
