CHARACTERISTICS, ORIENTATION AND ORIGIN OF STRUCTURAL COMPONENTS OF JOKWA LINEA GROOVE BELT, SE STANTON QUADRANGLE (V-38), VENUS

First Author
R. Oukhro (Department of Geology, Faculty of Sciences-Semlalia, Cadi Ayyad University, Marrakesh, Morocco)
Coauthor(s)
H. El Bilali (Department of Earth Sciences, Carleton University, Ottawa, Ontario, Canada)
R. E. Ernst (Department of Earth Sciences, Carleton University, Ottawa, Ontario, Canada; Faculty of Geology and Geography, Tomsk State University, Tomsk, Russia)
J. W. Head (Department of Earth, Environmental and Planetary Sciences, Brown University, Providence, Rhode Island, USA)
N. Youbi (Department of Geology, Faculty of Sciences-Semlalia, Cadi Ayyad University, Marrakesh, Morocco)
Session
Venus
Brief Abstract Summary
Characteristics, orientation and origin of structural components of Jokwa Linea Groove Belt, SE Stanton Quadrangle (V-38), Venus. Our preliminary mapping of >4000 extensional lineaments identifies 2 major radiating systems (interpreted to overlie dyke swarms) representing novae, and also intense linea-parallel systems.
Form of the Presentation
Oral