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+ 1970 News Releases (7.6 Mb PDF file) - NASA

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MSC 70-111<br />

material from 5 to 10 kilometers (3 to 6 miles) beneath the lunar<br />

surface. Copernicus is also thought to have been formed by one of<br />

the younger events _n lunar history and to be a key in dating other<br />

lunar features. Samples from the floor of Copernicus will _ive clues<br />

as to the differentiation or layering of the Moon. And material which<br />

has come from the central peaks may answer questions on the Moon's<br />

interior composition and structure.<br />

Copernicus, like Tycha_ presents a difficult landing problem;<br />

however, experience gained on the Apollo 14 and 15 missions could<br />

overcome these problems.<br />

Other landing s_Les have also seen discussed and are not ruled<br />

cut for future missions.<br />

Select:on of future sites w_ll depend in large part on the results<br />

a_d scTent_fie findings from preceding missions.

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