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. 2021 Feb 3;7(6):eabe4459. doi: 10.1126/sciadv.abe4459

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Copyright © 2021 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works. Distributed under a Creative Commons Attribution NonCommercial License 4.0 (CC BY-NC).

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Fig. 7 — (A) Enhanced color views demonstrating RSL development (white arrows) over time at Palikir crater (inside Newton Basin) (79) for Mars years 29 to 30; HiRISE images ESP_011428_1380, ESP_022267_1380, ESP_022689_1380, and ESP_022834_1380. (B) RSL flowing first over bright bedrock (red arrows) and then over the darker fan (white arrows) in Coprates Chasma (8); HiRISE image ESP_050021_1670. (C) RSL (white arrows) within and below gullies (blue arrows) on a hillside within Juventae Chasma (8); enhanced color view from HiRISE ESP_ 032496_1755. Image credit: NASA/JPL/University of Arizona.