“…On Earth, moment tensors are routinely calculated following significant seismic events (e.g., Dziewonski & Woodhouse, 1983) and have played a crucial role in understanding global patterns of seismicity as well as deformation across tectonic settings (e.g., Ekström et al, 2012). Techniques to constrain source characteristics of teleseismic events typically rely on data from globally distributed seismic stations, and optimal focal mechanisms are found either by fitting body wave first motions (e.g., Brumbaugh, 1979) or by fitting waveforms of intermediate period body wave (Langston & Helmberger, 1975) or surface wave phases (e.g., Arvidsson & Ekström, 1998), or complete long period waveforms (e.g., Dziewonski et al, 1981). Information about source depth comes from the lag-time of depth phases (e.g., Basham & Ellis, 1969) and/or by the frequency dependence of surface wave excitation (e.g., Tsai & Aki, 1970).On Mars, moment tensor inversions are challenging for several reasons: (a) only a single seismic station is available, limiting the sampling of the focal sphere; (b) depth phases are only rarely unequivocally identified, rendering source depth estimates inaccurate; (c) contribution of along-path structure to waveforms is difficult to estimate…”