Difference between revisions of "Head and Gifford, 1980"
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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 /> | <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 [ | + | 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 [ | + | * 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> |
<br /> | <br /> | ||
==LPOD Articles== | ==LPOD Articles== | ||
Revision as of 14:51, 15 April 2018
Contents
Head and Gifford: Lunar mare domes - Classification and modes of origin
(glossary entry)Table of Contents
[#Head and Gifford: Lunar mare domes - Classification and modes of origin Head and Gifford: Lunar mare domes - Classification and modes of origin]
[#Head and Gifford: Lunar mare domes - Classification and modes of origin-Description Description]
[#Head and Gifford: Lunar mare domes - Classification and modes of origin-Additional Information Additional Information]
[#Head and Gifford: Lunar mare domes - Classification and modes of origin-LPOD Articles LPOD Articles]
[#Head and Gifford: Lunar mare domes - Classification and modes of origin-Bibliography Bibliography]
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 JimMosher
LPOD Articles
Bibliography
- Head, J. W.; Gifford, A. 1980. Lunar mare domes - Classification and modes of origin. Moon and the Planets, vol. 22, pp. 235-258.
This page has been edited 1 times. The last modification was made by - tychocrater tychocrater on Jun 13, 2009 3:24 pm - mgx2
