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We summarize the scientific potential of high contrast optical space imagingfor studies of extrasolar planets, debris disks, and planet formation. Theunique scientific capabilities offered by a 2-m class optical telescope, thetechnical requirements to achieve 10^-9 contrast, and the programmatic meansneeded to advance such a mission are discussed.

First Steps in Direct Imaging of Planetary Systems Like our Own: The Science Potential of 2-m Class Optical Space Telescopes