Aeolian strata encode information about ancient planetary surface processes and the climate at the time of deposition. By decoding these strata, insight can be gained into ancient sediment transport processes, bedform kinematics, the landscape and prevailing climate. Deciphering these environmental signatures requires detailed analysis of the sedimentary architecture to reconstruct the bedforms and conditions enabling them to form. Here we show that a distinct sandstone unit exposed on the foothills of Mount Sharp in Gale crater (Mars) represents the preserved expression of compound aeolian bedforms which accumulated in the centre of a large dune field. Interrogation of Mastcam image data of the Stimson formation shows that it consists of c...
International audienceA widely hypothesized but complex transition from widespread fluvial activity ...
Ancient sediments provide archives of climate and habitability on Mars. Gale Crater, the landing sit...
International audienceCuriosity’s southward traverse up the lower north slope of Mt. Sharp (in Gale ...
Reconstruction of the palaeoenvironmental context of Martian sedimentary rocks is central to studies...
International audienceTemporal fluctuations of wind strength and direction can influence aeolian bed...
International audienceThe basal Siccar Point group unconformity observed at the Greenheugh pediment ...
Abstract Gale Crater contains Mount Sharp, a ~5km thick stratigraphic record of Mars ’ early environ...
Unraveling the stratigraphic record is the key to understanding ancient climate and past climate cha...
International audienceThe accumulated sediments and erosional unconformities in the deposits of Mt. ...
Geomorphic mapping associated with the 2019 publication in JGR Planets entitled: "Fluvio-lacustrine ...
Dunes and dune fields are dynamic features that respond to the unique boundary conditions under whic...
International audienceThe stratigraphy preserved within Aeolis Mons (Mount Sharp) in Gale crater (Ma...
International audienceDunes have similar morphologies on the Earth and Mars. The main differences be...
International audienceA widely hypothesized but complex transition from widespread fluvial activity ...
Ancient sediments provide archives of climate and habitability on Mars. Gale Crater, the landing sit...
International audienceCuriosity’s southward traverse up the lower north slope of Mt. Sharp (in Gale ...
Reconstruction of the palaeoenvironmental context of Martian sedimentary rocks is central to studies...
International audienceTemporal fluctuations of wind strength and direction can influence aeolian bed...
International audienceThe basal Siccar Point group unconformity observed at the Greenheugh pediment ...
Abstract Gale Crater contains Mount Sharp, a ~5km thick stratigraphic record of Mars ’ early environ...
Unraveling the stratigraphic record is the key to understanding ancient climate and past climate cha...
International audienceThe accumulated sediments and erosional unconformities in the deposits of Mt. ...
Geomorphic mapping associated with the 2019 publication in JGR Planets entitled: "Fluvio-lacustrine ...
Dunes and dune fields are dynamic features that respond to the unique boundary conditions under whic...
International audienceThe stratigraphy preserved within Aeolis Mons (Mount Sharp) in Gale crater (Ma...
International audienceDunes have similar morphologies on the Earth and Mars. The main differences be...
International audienceA widely hypothesized but complex transition from widespread fluvial activity ...
Ancient sediments provide archives of climate and habitability on Mars. Gale Crater, the landing sit...
International audienceCuriosity’s southward traverse up the lower north slope of Mt. Sharp (in Gale ...