The availability of Magellan radar images of Venus on CDROM allows sma
ll research groups to engage in planetary physics projects using simpl
e image processing systems. The material lends itself to short project
s for high school students or Masters students. Our initial investigat
ions using the Magellan data have evolved into a Masters project which
concentrates on the morphology of small scale structures which have t
errestrial counterparts. These include studies of volcanic cone fields
, lava tubes and other collapse features, and impact features.