“…We obtain admissible ranges of rock‐mass properties for both sets of Martian slopes by defining cohesion and friction pairs for representative rock masses using the Rock Mass Rating (RMR) system [e.g., Bieniawski , 1993] with the nonlinear Hoek‐Brown strength criterion [e.g., Schultz , 1996; Hoek , 1998; Dawson et al , 2000]. We represent intact crystalline rock with RMR = 100, unconfined compressive strength σ c = 300 MPa, and Hoek‐Brown parameter m i = 33; bedded lava flows, RMR = 75, σ c = 200 MPa, and m i = 22; sedimentary rock, RMR = 50, σ c = 100 MPa, and m i = 8; and soft rock/strong soil, RMR = 25, σ c = 50 MPa, and m i = 2.…”