This image in Athabasca Valles shows lava flows originating from Elysium Mons to the northwest. A Context Camera image shows the lava flowed from the northwest to the southeast,
diverting around obstacles as it settled. (The flow is outlined in blue with the flow direction shown in yellow, and the approximate location of the HiRISE image is represented by a white rectangle.)
The lava appears to have flowed smoothly around obstructions, almost like water,
forming streamlined islands. In the southern part of this image, a branch of the flow diverts around a small crater, and eventually rejoins the main part of the flow. Irregular-shaped ring structures appear on the northern end and are related to the
volcanic activity that formed the flows.
We also see a dense cluster of secondary craters that formed when material ejected from Corinto Crater (to the northwest) impacted the surface at high speed. At full-resolution, this terrain has the distinctive appearance of a field of
numerous, small and closely-spaced craters.
ID:
ESP_057978_1875date: 9 December 2018
altitude: 274 km
https://uahirise.org/hipod/ESP_057978_1875
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA