Mayssa El YazidiCsilla OrgelElliot Sefton-NashGuido De MarchiBahia RickbirDavid BaratouxSylvain BouleyJustin FilibertoPiero D’InceccoGiovanni LeoneNajet Slim ShimiFeyda SrarfiBalázs BradákLEONE GIOVANNI2025-05-232025-05-232024El Yazidi, M., Orgel, C., Sefton-Nash, E., De Marchi, G., Rickbir, B., Baratoux, D., Bouley, S., Filiberto, J., D’Incecco, P., Leone, G., Slim Shimi, N., Srarfi, F., & Bradák, B. (2024). Icarus, 415, 116075.https://hdl.handle.net/20.500.12740/22466This article analyzes the tectonic and magmatic processes responsible for the formation of Noctis Labyrinthus on Mars. It presents a high-resolution structural map and identifies three main fault systems, linking their orientations and interactions to tectonic phases and magmatic influences. Pit chains are examined and classified into four evolutionary stages, suggesting a formation driven by both extensional tectonics and magmatic chamber deflation. The study proposes a deformational model involving early extension and magmatic plumbing as co-occurring drivers.application/pdfNoctis LabyrinthusFaultsPit chainsExtensional tectonicsMarsMagmatic plumbingother10.1016/j.icarus.2024.116075