Volcanology of Venus
The surface of Venus is dominated by volcanic features and has more volcanoes than any other planet in the Solar System. It has a surface that is 90% basalt, and about 65% of the planet consists of a mosaic of volcanic lava plains, indicating that volcanism played a major role in shaping its surface. There are more than 1,000 volcanic structures and possible periodic resurfacing of Venus by floods of lava. The planet may have had a major global resurfacing event about 500 million years ago, from what scientists can tell from the density of impact craters on the surface. Venus has an atmosphere rich in carbon dioxide, with a density that is 90 times greater than Earth's atmosphere.
Lori Glaze
Glaze was the Principal Investigator for a proposed NASA Discovery mission to Venus, Deep Atmosphere Venus Investigation of Noble gases, Chemistry, and Imaging (DAVINCI). This mission would send a probe on a journey through Venus' atmosphere, descending over the planet's roughest and most geologically complex terrain. The DAVINCI probe would explore the planet's atmosphere from top to bottom, including the deep atmospheric layers largely hidden from Earth-based instruments and orbiting spacecraft. DAVINCI would be the first U.S. probe in nearly four decades to target Venus' atmosphere.