Fig. 1: Investigated martian craters and possible occurrence of self-secondaries around Tooting.
From: Contemporaneous formation of self-secondaries and layered ejecta deposits on Mars
a Locations of martian craters investigated in this work (red dots). b Morphology of earlier-reported self-secondaries on the southeastern crater rim of Tooting16. The location is marked in (d). c, d Predicted landing positions of Tooting’s ejecta launched from the crater center with ejection angles θ = 60° and 89°, respectively. Modeled ejecta particles are color-coded according to their flight time (see Methods). The white dashed circle in (c) indicates the rim crest of Tooting. IDs and available addresses of base images used are in the Supplementary Table 2.
