Head and Gifford, 1980
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 domes] identified on [/Lunar%20Orbiter Lunar Orbiter] and [/Apollo%20program Apollo] photos.
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). - 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
