Difference between revisions of "Head and Gifford, 1980"

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=Head and Gifford: ''Lunar mare domes - Classification and modes of origin''=
 
=Head and Gifford: ''Lunar mare domes - Classification and modes of origin''=
 
  (glossary entry)<br /> <div id="toc">
 
  (glossary entry)<br /> <div id="toc">
=Table of Contents=
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<div style="margin-left: 1em">[#Head and Gifford: Lunar mare domes - Classification and modes of origin Head and Gifford: Lunar mare domes - Classification and modes of origin]</div><div style="margin-left: 2em">[#Head and Gifford: Lunar mare domes - Classification and modes of origin-Description Description]</div><div style="margin-left: 2em">[#Head and Gifford: Lunar mare domes - Classification and modes of origin-Additional Information Additional Information]</div><div style="margin-left: 2em">[#Head and Gifford: Lunar mare domes - Classification and modes of origin-LPOD Articles LPOD Articles]</div><div style="margin-left: 2em">[#Head and Gifford: Lunar mare domes - Classification and modes of origin-Bibliography Bibliography]</div></div><br />  
 
 
==Description==
 
==Description==
  Extensive list of probable and suspected [/domes domes] identified on [/Lunar%20Orbiter Lunar Orbiter] and [/Apollo%20program Apollo] photos.<br /> <br />  
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  Extensive list of probable and suspected [[domes|domes]] identified on [[Lunar%20Orbiter|Lunar Orbiter]] and [[Apollo%20program|Apollo]] photos.<br /> <br />  
 
==Additional Information==
 
==Additional Information==
* Lunar surface features tend to become invisible when the [/sun%20angle sun angle] exceeds the surface slopes. As a result, despite their excellent spatial resolution, only relatively steep-walled domes are likely to be detectable in most satellite photos (taken with moderately high sun). <span class="membersnap">- [http://www.wikispaces.com/user/view/JimMosher [[Image:JimMosher-lg.jpg|16px|JimMosher]]] [http://www.wikispaces.com/user/view/JimMosher JimMosher]</span>
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* Lunar surface features tend to become invisible when the [[sun%20angle|sun angle]] exceeds the surface slopes. As a result, despite their excellent spatial resolution, only relatively steep-walled domes are likely to be detectable in most satellite photos (taken with moderately high sun). <span class="membersnap">- JimMosher</span>
 
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==LPOD Articles==
 
==LPOD Articles==
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  This page has been edited 1 times. The last modification was made by <span class="membersnap">- [http://www.wikispaces.com/user/view/tychocrater [[Image:tychocrater-lg.jpg|16px|tychocrater]]] [http://www.wikispaces.com/user/view/tychocrater tychocrater]</span> on Jun 13, 2009 3:24 pm - ''mgx2''</div>
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Latest revision as of 21:16, 16 April 2018

Head and Gifford: Lunar mare domes - Classification and modes of origin

(glossary entry)


Description

Extensive list of probable and suspected domes identified on Lunar Orbiter and Apollo photos.

Additional Information

  • Lunar surface features tend to become invisible when the sun angle exceeds the surface slopes. As a result, despite their excellent spatial resolution, only relatively steep-walled domes are likely to be detectable in most satellite photos (taken with moderately high sun). - JimMosher


LPOD Articles


Bibliography