SP-424 The Voyage of Mariner
10
Fig. A-29. Close inspection of the
many individual frames used to make the mosaics of the earlier
figures provides a wealth of new information about the innermost
planet. The presence of other large basins was confirmed in (a) is
shown a flooded 240-km (150 mi) diameter basin, its walls indicated
by arrow heads, as revealed at Mercury I Another flooded basin (b)
photographed at Mercury II is 350 km (220 mi) in diameter and appears
to be flooded with plains material and then subsequently cratered by
some large impacts. Not only did the filling material partially
inundate small craters which had formed along the rim of the basin at
the lower left but also overflowed the rim and spilled onto the
surrounding terrain at the top right.
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