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its attempted Venus orbit insertion (which may be re-
attempted in 2015).
Future Venus exploration (Bullock et al. 2009) is likely
to include platforms able to return image data on spatial
scales
employing either higher-resolution (possibly interferomet-
ric) radar from orbit, or near-infrared imaging from a bal-
loon near the surface. Such future missions will likely
reveal many more duneforms than are presently known, and
would likely reinvigorate aeolian studies on Venus.
1-2
orders
of
magnitude
better
than
Magellan,
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