Colin Dundas, PhD
Colin Dundas is a Research Geologist with the Astrogeology Science Center. He studies planetary geomorphology and surface processes using spacecraft imagery and topography data as well as numerical modeling, with a particular focus on active processes and change detection. He is a Co-Investigator and Science Theme Lead for Mass Wasting on the HiRISE camera team.
Biography
Ph.D., Planetary Science (Geoscience minor), The University of Arizona, 2009
B.S., Planetary Science, California Institute of Technology, 2004
Past and current research areas include:
- Current activity on Martian slopes, including Recurring Slope Lineae and changes in gullies
- Martian ground ice, ice-exposing impact craters and scarps, and sublimation-thermokarst landforms
- Large lava flows and lava-volatile interactions on Mars, Io, and Earth
- Effects of target properties and secondary craters on crater chronology
- Floods in Martian outflow channels
- Volatile-loss landforms in the Solar System
Science and Products
3-D Structure of Buried Ice Sheets on Mars Revealed by High-Resolution Images
For the first time, high-resolution images show the three-dimensional structure of massive ice deposits on Mars. According to an in-depth analysis led by the USGS, the images reveal never-before-observed details about the ice sheets, including that some begin just a few feet below the Martian surface and extend to depths greater than 300 feet.
Previous Evidence of Water on Mars Now Identified as Grainflows
Dark features previously proposed as evidence for significant liquid water flowing on Mars have now been identified as granular flows, where sand and dust move rather than liquid water, according to a new article published in Nature Geoscience by the U.S. Geological Survey.