- journal_title：Geology
- Contributor：Nathan T. Bridges ; Mary C. Bourke ; Paul E. Geissler ; Maria E. Banks ; Cindy Colon ; Serina Diniega ; Matthew P. Golombek ; Candice J. Hansen ; Sarah Mattson ; Alfred S. McEwen ; Michael T. Mellon ; Nicholas Stantzos ; Bradley J. Thomson
- Publisher：Geological Society of America
- Date：2012-
- Format：text/html
- Language：en
- Identifier：10.1130/G32373.1
- journal_abbrev：Geology
- issn：0091-7613
- volume：40
- issue：1
- firstpage：31
- section：Articles
Prior to Mars Reconnaissance Orbiter data, images of Mars showed no direct evidence for dune and ripple motion. This was consistent with climate models and lander measurements indicating that winds of sufficient intensity to mobilize sand were rare in the low-density atmosphere. We show that many sand ripples and dunes across Mars exhibit movement of as much as a few meters per year, demonstrating that Martian sand migrates under current conditions in diverse areas of the planet. Most motion is probably driven by wind gusts that are not resolved in global circulation models. A past climate with a thicker atmosphere is only required to move large ripples that contain coarse grains.