Abundant Recurring Slope Lineae (RSL) Following the Great Martian Dust Storm of 2018

Post contributed by Dr. Alfred S. McEwen, Lunar and Planetary Laboratory, University of Arizona, USA.

Recurring slope lineae (RSL) are dark linear markings on steep slopes of Mars that regrow annually and likely originate from the flow of either liquid water or dry granular material. Following the great dust storm (or planet-encircling dust event) of Mars Year 34 (in 2018), the High Resolution Imaging Science Experiment (HiRISE; McEwen et al., 2007) on Mars Reconnaissance Orbiter (MRO)  has seen many more candidate RSL than in typical Mars years (Image 1). These RSL sites show evidence for recent dust deposition and dust devil activity, so dust lifting processes may initiate and sustain RSL activity on steep slopes.

Image 1:  RSL and dust devil tracks on a hill in the southern middle latitudes (41.1ºS, 187.4ºE).  Inset shows some of the RSL at higher resolution.  Hundreds of dark dust devil tracks are seen on the full image as the more diffuse lines that cut across topography.  HiRISE image ESP_058122_1385, acquired after the 2018 dust storm.  Credit: NASA/JPL/University of Arizona


The thermal environment of recurring slope lineae on Mars

Post by Dr. Norbert Schorghofer. Senior Scientist, Planetary Science Institute

Recurring slope lineae (RSL) are dark narrow streaks on Mars that have puzzled scientists since their discovery in 2011. Image 1 shows a 3-dimensional perspective of a landscape with some of these flow features. RSL form and grow annually and mostly in the warm season, so the mechanism by which they form and grow is tantalizing. To what extent are RSL related to temperature or water? In rugged terrain there are stark temperature contrasts between pole‐facing and equator‐facing slopes that infrared cameras on Mars-orbiting spacecraft cannot spatially resolve. New modeling capabilities make it possible to overcome this limitation and provide surface temperatures at high spatial resolution.


Image 1: An image combining orbital imagery with 3-D modeling shows RSL on a slope inside Newton Crater. Image credit: NASA/JPL-Caltech/University of Arizona.


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