“…The episodic resurfacing model (Turcotte, 1993;Turcotte, 1995;Basilevsky and Head, 1998;Turcotte et al, 1999;Basilevsky and Head, 2000) proposes a short-lived but intense period of activity ~750 Ma ago, followed by a long period of quiescence that is consistent with the impact crater distribution but predicts minimal rates of volcanic and tectonic activity at the present day, apparently inconsistent with geological observations. Models involving some form of plate-like movement (e.g., Schubert and Sandwell, 1995;Gilmore et al, The extreme surface conditions on Venus require that these science goals must be addressed by orbital remote sensing, including interferometric synthetic aperture radar (InSAR) data, gravity data, altimetric data and multispectral infrared data.…”