Physical and Chemical Processes in Titan's Interdunes


Titan's organic sand seas cover ~20% of its surface, a higher fraction than on any other planetary body. The sand coverage within those seas is not continuous, however. As on Earth, Titan's sand seas are characterized... [ view full abstract ]


  1. Jason Barnes (University of Idaho)
  2. Shannon MacKenzie (University of Idaho)
  3. Ralph Lorenz (APL)
  4. Jani Radebaugh (BYU)
  5. Alexander Hayes (Cornell)
  6. Elizabeth Turtle (JHU/APL)

Topic Area

Topics: Depositional systems on Mars and Titan


MS11 » Planetary Sedimentology II (11:00 - Wednesday, 25th May, FES 1)

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