Eroding Dunes and Dust Devil Tracks in Terra Cimmeria
Ongoing Dune Activity in Ganges Chasma
USGS Dune Database Entry Number 1863-568
A detailed classification system for Martian dunes is currently in the works. However, we have summarized current classifications below. You can find more information on terrestrial dune classification by clicking here.
Below are other science projects associated with this project.
Mars Dune Image Galleries
Mars Dune Image Galleries: CRISM, THEMIS, MOC and HiRISE
The Mars Global Digital Dune Database
The Mars Global Digital Dune Database (MGD 3 ) The Mars Global Digital Dune Database (MGD3)was compiled and released in three parts, encompassing the area from latitude 65°N to 65°S, from 60°N to 90°N (the north polar region), and from 60° to 90°S (south polar region). All the remote sensing data for both GIS and non-GIS users is available online in three U.S. Geological Survey Open File Reports...
Consortium Announcements and Meetings
Consortium hosted meetings will be listed below. If you would like to attend any of these meetings, please be sure to register. Should your plans change after you register, you may simply reregister with your changes detailed appropriately.
Workshops
Researchers in the planetary and terrestrial aeolian community are at work all over the world; the last workshop alone had representatives from eight countries and three continents! This research is conducted locally on Earth analogs and on such far-flung places as Titan, but the common goal is to understand geological processes on the rocky planets, dwarf planets, asteroids, and satellites of our...
Mars Dunes
Sand dunes are among the most widespread aeolian features present on Mars, serving as unique indicators of the interaction between the atmosphere and surface. On a planetary body, dunes accumulate where a supply of sand-sized grains exists or may be abraded, is carried downwind by winds of saltation strength, and is subsequently deposited where these winds weaken below the threshold for sand...
Below are other science projects associated with this project.
Mars Dune Image Galleries
Mars Dune Image Galleries: CRISM, THEMIS, MOC and HiRISE
The Mars Global Digital Dune Database
The Mars Global Digital Dune Database (MGD 3 ) The Mars Global Digital Dune Database (MGD3)was compiled and released in three parts, encompassing the area from latitude 65°N to 65°S, from 60°N to 90°N (the north polar region), and from 60° to 90°S (south polar region). All the remote sensing data for both GIS and non-GIS users is available online in three U.S. Geological Survey Open File Reports...
Consortium Announcements and Meetings
Consortium hosted meetings will be listed below. If you would like to attend any of these meetings, please be sure to register. Should your plans change after you register, you may simply reregister with your changes detailed appropriately.
Workshops
Researchers in the planetary and terrestrial aeolian community are at work all over the world; the last workshop alone had representatives from eight countries and three continents! This research is conducted locally on Earth analogs and on such far-flung places as Titan, but the common goal is to understand geological processes on the rocky planets, dwarf planets, asteroids, and satellites of our...
Mars Dunes
Sand dunes are among the most widespread aeolian features present on Mars, serving as unique indicators of the interaction between the atmosphere and surface. On a planetary body, dunes accumulate where a supply of sand-sized grains exists or may be abraded, is carried downwind by winds of saltation strength, and is subsequently deposited where these winds weaken below the threshold for sand...