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| Apollo 15 Lunar Geology Investigation |
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Apollo 15 |
The Hadley/Apennine
site was selected for multiple objectives:
The Apennine Mountain front forms the arcuate southeastern
rim of Mare Imbrium. It borders Palus Putredinis and, in the area of the
site, it rises 12,000 feet (3658 m) above the surrounding mare. The second important objective of the mission was to study and sample the Hadley Rille, which runs parallel to the Apennine Mountain front and incises the Palus Putredinis mare material. The rille is a sinuous or meandering channel, much like a river gorge on Earth. It displays a V-shaped cross section, with an average slope of about 25 degrees. In the vicinity of the landing site, the rille is about one mile (1.6 km) wide and 1,300 feet (396 meters) deep. The third objective of the mission was to study and sample the reasonably flat mare material of Palus Putredinis on which the LM landed. Analysis of the samples showed that this mare surface was younger than that visited on Apollo 11, and was closer to the age of the Apollo 12 mare site. A complex of domical structures about 5 km north of the landing site constituted another objective of the mission. The hills may be made of volcanic domes superposed on the surrounding mare or buried domical structures thinly covered by the mare-like material From Apollo 15 Press Kit |
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