Modern Mars' geomorphological activity, driven by wind, frost, and gravity
Extensive evidence of landform-scale martian geomorphic changes has been acquired in
the last decade, and the number and range of examples of surface activity have increased …
the last decade, and the number and range of examples of surface activity have increased …
Active Mars: A dynamic world
Mars exhibits diverse surface changes at all latitudes and all seasons. Active processes
include impact cratering, aeolian sand and dust transport, a variety of slope processes …
include impact cratering, aeolian sand and dust transport, a variety of slope processes …
Martian subsurface cryosalt expansion and collapse as trigger for landslides
On Mars, seasonal martian flow features known as recurring slope lineae (RSL) are
prevalent on sun-facing slopes and are associated with salts. On Earth, subsurface …
prevalent on sun-facing slopes and are associated with salts. On Earth, subsurface …
Evaluation of wet and dry recurring slope lineae (RSL) formation mechanisms based on quantitative map** of RSL in Garni Crater, Valles Marineris, Mars
Recurring slope lineae (RSL) are narrow (0.5–5 m) low-albedo features that incrementally
lengthen down steep slopes during warm seasons, fade in colder seasons, and recur each …
lengthen down steep slopes during warm seasons, fade in colder seasons, and recur each …
[HTML][HTML] Revealing active Mars with HiRISE digital terrain models
Many discoveries of active surface processes on Mars have been made due to the
availability of repeat high-resolution images from the High Resolution Imaging Science …
availability of repeat high-resolution images from the High Resolution Imaging Science …
[HTML][HTML] An aeolian grainflow model for martian recurring slope lineae
CM Dundas - Icarus, 2020 - Elsevier
Abstract Recurring Slope Lineae (RSL) on Mars have been enigmatic since their discovery;
their behavior resembles a see** liquid but sources of water remain puzzling. This work …
their behavior resembles a see** liquid but sources of water remain puzzling. This work …
Mars: Abundant recurring slope lineae (RSL) following the Planet‐Encircling Dust Event (PEDE) of 2018
Recurring slope lineae (RSL) are dark linear markings on Mars that regrow annually and
likely originate from the flow of either liquid water or granular material. Following the great …
likely originate from the flow of either liquid water or granular material. Following the great …
Implications for the origin and evolution of Martian Recurring Slope Lineae at Hale crater from CaSSIS observations
Highlights•We report the first CaSSIS observations of RSL at Hale crater, Mars.•We compare
morning CaSSIS images with afternoon HiRISE observations.•We do not find any relative …
morning CaSSIS images with afternoon HiRISE observations.•We do not find any relative …
Novel quantitative methods to enable multispectral identification of high-purity water ice exposures on Mars using High Resolution Imaging Science Experiment …
Reliable detection and characterization of water ice on the Martian surface is pivotal to not
only understand its present and past climate, but to also provide valuable information on in …
only understand its present and past climate, but to also provide valuable information on in …
Evidence for transient morning water frost deposits on the Tharsis volcanoes of Mars
A Valantinas, N Thomas, A Pommerol, O Karatekin… - Nature …, 2024 - nature.com
The present-day water cycle on Mars has implications for habitability and future human
exploration. Water ice clouds and water vapour have been detected above the Tharsis …
exploration. Water ice clouds and water vapour have been detected above the Tharsis …