“…Irwin et al (2005a) estimated a minimum channel-forming discharge (Q, m 3 /s) and rate of runoff production for event floods (R e , discharge divided by contributing area, reported as cm/day) for a set of Martian interior channels, based on width and assuming weak banks. They selected a terrestrial empirical relationship from Osterkamp and Hedman (1982) with relatively low bank strength (and, thus, channels of high width/depth ratio), discharge as the dependent variable, and a recurrence interval of two years (i.e., Q 2 , which is commonly associated with channel-forming discharge (Knighton, 1998)). That relationship, when scaled for Martian gravity by a factor of 0.62 (i.e., 0.38 0.5 ) , is:…”