EVIDENCE FOR LATE HESPERIAN FLUVIAL ACTIVITY IN NIRGAL VALLIS ON MARS
This study investigates the deposit on the floor of Uzboi Vallis at the confluence of Nirgal Vallis using MOLA and HiRISE data. The estimated volume of the deposit is significantly smaller than the total volume of material removed by Nirgal Vallis. The deposit consists of a fairly symmetric fan-shaped landform (~40 km3) at the mouth of Nirgal that is stratigraphically on top of a larger mound of material (~200 km3) that is offset downstream toward Holden. The proximal fan surface consists of light-toned material that incorporates meter-scale blocks and lacks obvious layering whereas craters near the distal fan margin (~15 km from Nirgal) expose fine-grained, light toned, horizontal layers.
The net difference in volume between the deposit on the floor of Uzboi relative to the volume of material eroded from Nirgal Vallis suggests that 1) most of the material transported in Nirgal debouched into Uzboi when there was active flow through the system, thereby resulting in much of the sediment being transported downstream, and 2) the majority of incision in Nirgal likely pre-dates deposition into Lake Uzboi. The nature of the fan-shaped deposit at the mouth of Nirgal Vallis, however, is consistent with deposition into standing water in Lake Uzboi. If correct, this implies that late fluvial activity in Nirgal was concurrent with Lake Uzboi and (or) was related to water draining out of Uzboi as water in the lake drained northward into Holden.