Predicting the morphodynamics of sedimentary landscapes due to fluvial and aeolian flows
requires answering the following questions: Is the flow strong enough to initiate sediment …

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 sample analysis at Mars instrument evolved gas analyzer (SAM‐EGA) has detected
evolved water, H2, SO2, H2S, NO, CO2, CO, O2, and HCl from two eolian sediments and …

Reconstruction of the palaeoenvironmental context of Martian sedimentary rocks is central to
studies of ancient Martian habitability and regional palaeoclimate history. This paper reports …

Wind blowing over sand on Earth produces decimeter-wavelength ripples and hundred-
meter–to kilometer-wavelength dunes: bedforms of two distinct size modes. Observations …

We have developed a refined geologic map and stratigraphy for lower Mount Sharp using
coordinated analyses of new spectral, thermophysical, and morphologic orbital data …

Abstract The Mars Science Laboratory rover, Curiosity, is using a comprehensive scientific
payload to explore rocks and soils in Gale crater, Mars. Recent investigations of the Bagnold …

A high density of REMS wind measurements were collected in three science investigations
during MSL's Bagnold Dunes Campaign, which took place over∼ 80 sols around southern …

Abstract The Mars Science Laboratory Curiosity rover performed coordinated measurements
to examine the textures and compositions of aeolian sands in the active Bagnold dune field …

Aeolian ripples are common in sandy environments on Earth and Mars. On Earth, ripples in
sorted dune sands typically are< 1 cm high and are erased in high winds. On Mars in similar …