Like planet Earth, the geology of Venus is diverse; consisting of areas of flat plains and deformed, mountain-like terrains called tesserae. And like Earth, Mars, and the Moon, Venus is checkered with hundreds of craters.
“What’s odd about Venus’s craters, is that craters we do see are relatively young, indicating the surface of Venus has been covered by planet-wide volcanic flows,” says Martha “Marty” Gilmore, George I. Seney Professor of Geology, professor of earth and environmental sciences. “The tesserae are the only terrains older than these volcanic flows and thus our only hope at accessing rocks from the first billion years of Venus’s history, when the planet may have had an ocean and may have been habitable.”
As the recipient of a three-year $430,801 grant from NASA’s Solar System Workings Program, Gilmore and James Greenwood, assistant professor of earth and environmental sciences, will use Magellan radar data to create the first map of crater ejecta on Venus classified by origin on plains or tessera terrain. Their project is titled “Radar Emissivity and Dielectric Permittivity of the Venus Surface Beneath Crater Parabolas.” Crater parabolas refer to the shape of the ejecta deposits as they are carried westward by the high-altitude Venus winds.