Abstract

Sand mobilized by wind forms decimeter-scale impact ripples and decameter-scale or larger dunes on Earth and Mars. In addition to those two bedform scales, orbital and in situ images revealed a third distinct class of larger meter-scale ripples on Mars. Since their discovery, two main hypotheses have been proposed to explain the formation of large martian ripples—that they originate from the growth in wavelength and height of decimeter-scale ripples or that they arise from the same hydrodynamic instability as windblown dunes or subaqueous bedforms instead. Here we provide evidence that large martian ripples form from the same hydrodynamic instability as windblown dunes and subaqueous ripples. Using an artificial neural network, we characterize the morphometrics of over a million isolated barchan dunes on Mars and analyze how their size and shape vary across Mars’ surface. We find that the size of Mars’ smallest dunes decreases with increasing atmospheric density with a power-law exponent predicted by hydrodynamic theory, similarly to meter-size ripples, tightly bounding a forbidden range in bedform sizes. Our results provide key evidence for a unifying model for the formation of subaqueous and windblown bedforms on planetary surfaces, offering a new quantitative tool to decipher Mars’ atmospheric evolution.

Dust storms on Mars drive water escape to space. Here, the authors show the impact Martian dust storms have on the abundance of atmospheric hydrogen and oxygen, and how this helps to overall oxidize the Martian atmosphere.

Details

Title
A distinct ripple-formation regime on Mars revealed by the morphometrics of barchan dunes
Author
Rubanenko, Lior 1   VIAFID ORCID Logo  ; Lapôtre, Mathieu G. A. 1   VIAFID ORCID Logo  ; Ewing, Ryan C. 2 ; Fenton, Lori K. 3 ; Gunn, Andrew 4 

 Stanford University, Department of Geological Sciences, Stanford, USA (GRID:grid.168010.e) (ISNI:0000000419368956) 
 Texas A&M, Department of Geology & Geophysics, College Station, USA (GRID:grid.264756.4) (ISNI:0000 0004 4687 2082) 
 SETI Institute, Carl Sagan Center, Mountain View, USA (GRID:grid.422128.f) (ISNI:0000 0001 2115 2810) 
 Stanford University, Department of Geological Sciences, Stanford, USA (GRID:grid.168010.e) (ISNI:0000000419368956); Monash University, School of Earth, Atmosphere & Environment, Clayton, Australia (GRID:grid.1002.3) (ISNI:0000 0004 1936 7857) 
Publication year
2022
Publication date
2022
Publisher
Nature Publishing Group
e-ISSN
20411723
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2739341251
Copyright
© The Author(s) 2022. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.