Abstract

Agenor Linea is a ∼1500 km long, ∼20–30 km wide geologically young zone of deformation on Jupiter's icy moon, Europa. On the basis of recent Galileo high‐resolution images, we interpret Agenor Linea as a strike‐slip zone formed in three stages by a combination of lithospheric separation, extension, and dextral horizontal shear. Agenor Linea exhibits excellent examples of strike‐slip duplexes in an icy lithosphere, unobscured by vegetation and unaltered by erosion.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.