Recent liquid water flow on Mars has been proposed based on geomorphological features,
such as gullies. Recurring slope lineae—seasonal flows that are darker than their …

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 …

Active dark flows known as recurring slope lineae have been observed on the warmest
slopes of equatorial Mars. The morphology, composition and seasonality of the lineae …

The recurring slope lineae on Mars have been hypothesized to originate from snow melting,
deliquescence, dry flow or shallow groundwater. Except for the dry flow origin, these …

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 …

Oxychlorine species are globally widespread across the Martian surface. Despite their
ubiquitous presence, the ability of oxychlorine species to serve as oxidants on Mars has …

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 …

Recurring slope lineae (RSL) are narrow (0.5–5 m) dark features on Mars that incrementally
lengthen down steep slopes, fade in colder seasons, and recur annually. These traits …

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 …

Current seismicity of Mars is poorly known. Geodynamic models and analysis of surface
faults indicate that Mars could be seismically active globally, particularly within the Tharsis …