Difference between revisions of "April 18, 2005"

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=The Lunar Crater Wood=
 
=The Lunar Crater Wood=
 
 
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<td width="50%"><h2><nobr>The Lunar Crater Wood</nobr></h2></td>
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    <tr><td><div align="center" class="main_sm">Image Credit: <a class="one" href="http://pdsmaps.wr.usgs.gov/explorer-bin/mapmars4.cgi?DATA_SET_NAME=moon_clementine_bw&VERSION=ADVANCED&RESAMP_METHOD=NEAREST_NEIGHBOR&BANDS=1&PIXEL_TY">Clementine</a> and <a class="one" href="http://www.lpi.usra.edu/resources/lunar_orbiter/bin/info.shtml?608">Lunar Orbiter V</a></p>
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<tr><td><div align="center" class="main_sm">Image Credit: [http://pdsmaps.wr.usgs.gov/explorer-bin/mapmars4.cgi?DATA_SET_NAME=moon_clementine_bw&VERSION=ADVANCED&RESAMP_METHOD=NEAREST_NEIGHBOR&BANDS=1&PIXEL_TY Clementine] and [http://www.lpi.usra.edu/resources/lunar_orbiter/bin/info.shtml?608 Lunar Orbiter V]</p>
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<p align="center"><b>The Lunar Crater Wood</b></p>
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<p align="center"><b>The Lunar Crater Wood</b></p>
<p align="left">At 43 degrees N, 121 degrees W, on the lunar farside, the 78 km wide crater Wood sits on the rim of Landau. Wood is an older crater, lacking the brightness of a recent impact, and the northwestern rim has a broad area of collapse, perhaps caused by a more recent crater. In any case, the rim outline on the northwest extends considerably westward, distorting the crater’s circularity. The Lunar Orbiter V image, marred by a horizontal defect, shows that the eastern floor of Wood, like the northeastern floor of Landau is surfaced with a smooth material that looks like mare lava - Wood’s floor even hosts a mare ridge. But Clementine multi-spectral data demonstrate that this is not mare lava. Once again, a highland crater has a surface that morphologically looks like lava, but spectrally isn’t. Most likely the Moon has lavas of spectral types unsampled by Apollo. These two images show that although we have some basic data for the farside, it is far from what is necessary to understand its details. All the more shame that amateur imagers can’t contribute new data!  By the way, this crater honors Robert W. Wood (1868-1955), an American physicist who discovered that the Aristarchus Plateau is the darkest spot on the Moon in ultraviolet light.</p>
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<p align="left">At 43 degrees N, 121 degrees W, on the lunar farside, the 78 km wide crater Wood sits on the rim of Landau. Wood is an older crater, lacking the brightness of a recent impact, and the northwestern rim has a broad area of collapse, perhaps caused by a more recent crater. In any case, the rim outline on the northwest extends considerably westward, distorting the crater’s circularity. The Lunar Orbiter V image, marred by a horizontal defect, shows that the eastern floor of Wood, like the northeastern floor of Landau is surfaced with a smooth material that looks like mare lava - Wood’s floor even hosts a mare ridge. But Clementine multi-spectral data demonstrate that this is not mare lava. Once again, a highland crater has a surface that morphologically looks like lava, but spectrally isn’t. Most likely the Moon has lavas of spectral types unsampled by Apollo. These two images show that although we have some basic data for the farside, it is far from what is necessary to understand its details. All the more shame that amateur imagers can’t contribute new data!  By the way, this crater honors Robert W. Wood (1868-1955), an American physicist who discovered that the Aristarchus Plateau is the darkest spot on the Moon in ultraviolet light.</p>
<blockquote><p align="right">&#8212; [mailto:tychocrater@yahoo.com Chuck Wood]</blockquote>
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<blockquote><p align="right">&#8212; [mailto:tychocrater@yahoo.com Chuck Wood]</blockquote>
 
<p align="left"><p align="left"><b>Tomorrow's LPOD: </b> I have many photos from Mike Wirths, Wes Higgins & Paolo Lazzarotti - does anyone else image the Moon?</p>
 
<p align="left"><p align="left"><b>Tomorrow's LPOD: </b> I have many photos from Mike Wirths, Wes Higgins & Paolo Lazzarotti - does anyone else image the Moon?</p>
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<p align="center" class="main_titles"><b>Author &amp; Editor:</b><br>  
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<p align="center" class="main_titles"><b>Author &amp; Editor:</b><br>  
[mailto:chuck@observingthesky.org Charles A. Wood]</p>
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[mailto:tychocrater@yahoo.com Charles A. Wood]</p>
<p align="center" class="main_titles"><b>Technical Consultant:</b><br>
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<p align="center" class="main_titles"><b>Technical Consultant:</b><br>
[mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
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[mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
<p align="center" class="main_titles"><b>Contact Translator:</b><br>
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<p align="center" class="main_titles"><b>Contact Translator:</b><br>
[mailto:pablolonnie@yahoo.com.mx" class="one Pablo Lonnie Pacheco Railey]  (Es)<br>
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[mailto:pablolonnie@yahoo.com.mx" class="one Pablo Lonnie Pacheco Railey]  (Es)<br>
[mailto:chlegrand@free.fr" class="one Christian Legrand] (Fr)</p>
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[mailto:chlegrand@free.fr" class="one Christian Legrand] (Fr)</p>
<p align="center" class="main_titles"><b>[mailto:webuser@observingthesky.org Contact Webmaster]</b></p>
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<p align="center" class="main_titles"><b>[mailto:webuser@observingthesky.org Contact Webmaster]</b></p>
<p align="center" class="main_titles"><b>A service of:</b><br>
+
<p align="center" class="main_titles"><b>A service of:</b><br>
[http://www.observingthesky.org/" class="one ObservingTheSky.Org]</p>
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[http://www.observingthesky.org/" class="one ObservingTheSky.Org]</p>
<p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
+
<p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
[http://antwrp.gsfc.nasa.gov/apod/astropix.html" class="one Astronomy] | [http://www.msss.com/" class="one Mars] | [http://epod.usra.edu/" class="one Earth]</p>
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[http://antwrp.gsfc.nasa.gov/apod/astropix.html" class="one Astronomy] | [http://www.msss.com/" class="one Mars] | [http://epod.usra.edu/" class="one Earth]</p>
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<p>&nbsp;</p>
 
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===COMMENTS?===  
 
===COMMENTS?===  
 
Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment.
 
Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment.

Revision as of 17:31, 4 January 2015

The Lunar Crater Wood

<nobr>The Lunar Crater Wood</nobr>

<img src="archive/2005/04/images/LPOD-2005-04-18.jpeg" border="0">

Image Credit: Clementine and Lunar Orbiter V


The Lunar Crater Wood

At 43 degrees N, 121 degrees W, on the lunar farside, the 78 km wide crater Wood sits on the rim of Landau. Wood is an older crater, lacking the brightness of a recent impact, and the northwestern rim has a broad area of collapse, perhaps caused by a more recent crater. In any case, the rim outline on the northwest extends considerably westward, distorting the crater’s circularity. The Lunar Orbiter V image, marred by a horizontal defect, shows that the eastern floor of Wood, like the northeastern floor of Landau is surfaced with a smooth material that looks like mare lava - Wood’s floor even hosts a mare ridge. But Clementine multi-spectral data demonstrate that this is not mare lava. Once again, a highland crater has a surface that morphologically looks like lava, but spectrally isn’t. Most likely the Moon has lavas of spectral types unsampled by Apollo. These two images show that although we have some basic data for the farside, it is far from what is necessary to understand its details. All the more shame that amateur imagers can’t contribute new data! By the way, this crater honors Robert W. Wood (1868-1955), an American physicist who discovered that the Aristarchus Plateau is the darkest spot on the Moon in ultraviolet light.

Chuck Wood

Tomorrow's LPOD: I have many photos from Mike Wirths, Wes Higgins & Paolo Lazzarotti - does anyone else image the Moon?



Author & Editor:
Charles A. Wood

Technical Consultant:
Anthony Ayiomamitis

Contact Translator:
" class="one Pablo Lonnie Pacheco Railey (Es)
" class="one Christian Legrand (Fr)

Contact Webmaster

A service of:
" class="one ObservingTheSky.Org

Visit these other PODs:
" class="one Astronomy | " class="one Mars | " class="one Earth

 


COMMENTS?

Click on this icon File:PostIcon.jpg at the upper right to post a comment.