In November 2018, for the first time a dedicated geophysical station, the InSight lander, will
be deployed on the surface of Mars. Along with the two main geophysical packages, the …

Despite the importance of sand and dust to Mars geomorphology, weather, and exploration,
the processes that move sand and that raise dust to maintain Mars' ubiquitous dust haze and …

In 2018, images were released of a planet being formed around the star PDS 70, offering a
tantalizing glimpse into how planets come into being. However, many questions remain …

We characterize vortex and dust devils (DDs) at Jezero from pressure and winds obtained
with the Mars Environmental Dynamics Analyzer (MEDA) instrument on Mars 2020 over 415 …

Convective vortices and dust devils have been inferred and observed in Gale Crater, Mars,
using Mars Science Laboratory (MSL) meteorological data and camera images. Rennó et …

We report the aeolian changes observed in situ by NASA's InSight lander during the first 400
sols of operations: Granule creep, saltation, dust removal, and the formation of dark surface …

Large eddy simulation (LES) of the Martian convective boundary layer (CBL) with a Mars‐
adapted version of the Weather Research and Forecasting model is used to examine the …

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 dark linear markings on Mars that regrow annually and
likely originate from the flow of either liquid water or granular material. Following the great …

Geologic and climatic processes on modern‐day Mars are heavily influenced by aeolian
surface activity, yet the relationship between atmospheric conditions and sediment …