Difference between revisions of "August 1, 2004"

From LPOD
Jump to: navigation, search
 
(4 intermediate revisions by the same user not shown)
Line 1: Line 1:
 
__NOTOC__
 
__NOTOC__
 
=Another Day, Another Success=
 
=Another Day, Another Success=
 +
<!-- Start of content -->
 
<br>
 
<br>
 
<table width="85%"  border="0" align="center" cellpadding="6" cellspacing="2">
 
<table width="85%"  border="0" align="center" cellpadding="6" cellspacing="2">
Line 15: Line 16:
 
<table width="100%"  border="0" cellpadding="8">
 
<table width="100%"  border="0" cellpadding="8">
 
<tr>
 
<tr>
<td><div align="center" span class="main_sm"><p>Image Credit: [http://nssdc.gsfc.nasa.gov/imgcat/html/mission_page/EM_Lunar_Orbiter_5_page1.html Lunar Orbiter V - M197 ] </div></td>
+
<td><div align="center"><p>Image Credit: [http://nssdc.gsfc.nasa.gov/imgcat/html/mission_page/EM_Lunar_Orbiter_5_page1.html Lunar Orbiter V - M197 ]</p></div></td>
 
</tr>   
 
</tr>   
 
</table>   
 
</table>   
Line 34: Line 35:
 
[http://photojournal.jpl.nasa.gov/catalog/PIA00090 Clementine View] <br>
 
[http://photojournal.jpl.nasa.gov/catalog/PIA00090 Clementine View] <br>
 
Rukl, Atlas of the Moon, Section 18.</p>
 
Rukl, Atlas of the Moon, Section 18.</p>
<p><b>Tomorrow's LPOD:</b> Jupiter Graze</p>
+
<p><b>Yesterday's LPOD:</b> [[July 31, 2004|40 Years Since Impact]] </p>
 +
<p><b>Tomorrow's LPOD:</b> [[August 2, 2004|Jupiter Graze]] </p>
 
</tr>
 
</tr>
 
</table>
 
</table>
Line 45: Line 47:
 
<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:tychocrater@yahoo.com 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>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>
+
<!-- Cleanup of credits -->
 +
<!-- Cleanup of credits -->
 
</td>
 
</td>
 
</tr>
 
</tr>
 
</table>
 
</table>
 
<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.
 

Latest revision as of 19:22, 7 February 2015

Another Day, Another Success


LPOD-2004-08-01.jpeg


Another Day, Another Success

The Lunar Orbiter program, which acquired high resolution images of the lunar surface to help identify safe landing sites for Apollo, was the most successful of America's lunar efforts. There were 5 missions and 5 successes - compare with 3 out of 9 for Ranger, 4 out of 5 for Surveyor, and 6 out of 7 for Apollo. The first 3 Orbiters were so successful at getting high resolution images of potential Apollo landing sites that the 4th was reprogrammed to map most of the Moon, and the 5th - launched 37 years ago today - focussed on areas of high geologic interest. And some of the most dramatic images from our first phase (I am an optimist!) of lunar exploration came from Orbiter V. This wonderful medium resolution view of Aristarchus is a good example. The 40 km wide, 4.25 km deep crater is very young, an estimated half billion years old, and is very well preserved. Radial ejecta deposits and secondary craters cover the nearby Oceanus Procellarum and the hapless crater Aristarchus F at the bottom right of the image. On the inner wall at least three down-dropped terraces are visible, and a central peak rises from the flat floor. Clementine multi-spectral imaging showed that parts of the peaks are made of the anorthite - the deep, plagioclase-rich rock that formed in the early Moon's magma ocean.

Chuck Wood

Technical Details:
An 80 mm lens was used to record LO V's medium resolution images on 70 mm wide film. The film was developed on the spacecraft, scanned and radioed to Earth, where it was reconstructed as a series of framelet strip photographs that were mosaicked together. You can see the individual framelets as vertical stripes in the image above.

Related Links:
LO V at NSSDC
Photographing LO V at the Moon
Destination Moon: A History of the Lunar Orbiter Program
Clementine View
Rukl, Atlas of the Moon, Section 18.

Yesterday's LPOD: 40 Years Since Impact

Tomorrow's LPOD: Jupiter Graze



Author & Editor:
Charles A. Wood

 


COMMENTS?

Register, Log in, and join in the comments.