Planetary Dunes Workshop: A Record of Climate Change

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Planetary Dunes Workshop:A Record of Climate ChangeNOTE ADDED BY JPL WEBMASTER: This document was prepared by the Lunar and Planetary Institute. The content has not been…
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Planetary Dunes Workshop:A Record of Climate ChangeNOTE ADDED BY JPL WEBMASTER: This document was prepared by the Lunar and Planetary Institute. The content has not been approved or adopted by, NASA, JPL, or the California Institute of Technology. This document is being made available for information purposes only, and any views and opinions expressed herein do not necessarily state or reflect those of NASA, JPL, or the California Institute of Technology.Alamogordo, New MexicoApril 28 – May 2, 2008Sponsors: Lunar and Planetary Institute (Elizabeth Wagganer) NASA’s Mars Exploration ProgramOrganizing Committee: Tim Titus, USGS Rose Hayward, USGSMary Bourke, Planetary Science Institute Nick Lancaster, Desert Research Institute Lori Fenton, Carl Sagan CenterDunes common to several planetary bodies
  • Morphology and behavior reflect sedimentary and climatic history of regions where they are located
  • Yet much is not known about dunes
  • Their age, origins, sediment sources, composition, and dynamics under present/past climate conditions
  • Intent of our meeting
  • To gather our growing community and share ideas
  • To identify priorities for future planetary dune research
  • 3 ½ day workshop, with field trip on 2nd day
  • 47 attendees from 4 continents
  • 39 abstracts (2 page LPI format)
  • 5 oral sessions – 30 min talks (45 min invited)
  • Titan, Earth, Mars I, Mars II, Modeling
  • 2 poster sessions:
  • Earth/Titan/Instruments, Mars
  • (from Zimbelman, PD Wkshp. Abst. #7005)Modeling
  • Scaling law to understand bedform size
  • Bedform initiation and growth
  • Interactions of bedforms (e.g., collisions)
  • (From Claudin and Andreotti, PD Wkshp Abst. #7009)Titan: Hyrdrocarbon Sand
  • Equatorial belt of dunes
  • implications for humidity/precip. patterns
  • Formed by westerly winds
  •  implications for atmospheric circulation (From Radebaugh et al., PD Wkshp. Abst. #7037)Earth: The Analog Planet
  • samples and field data help determine:
  •  Geochemically identified sand sources
  • Internal dune stratigraphy
  •  Absolute age dating of sand grain deposition with OSL(From Bristow et al., PD Wkshp., Abst. #7004)Mars: North Polar Dunes
  • Wind pattern in dunes suggests a temporal shift in direction
  • Hydrated minerals present in all dunes and troughs, not just Olympia Planitia
  • Updated TI analysis suggests dunes are unconsolidated sand overlying rock or ice
  • (from Horgan et al., PD Wkshp., Abst. #7035)Mars: ContinuedBeginning to decipher how variations in morphology and mineralogy relate to dune field history, wind regime, dune activity
  • Using techniques with available Mars data and analog sites on Earth
  • Patterns on scale of regional dune field trends and individual dunes
  • MGS MOC M03/03088Field trip to White Sands National Monumentled by Dave Bustos, Ryan Ewing, Gary Kocurek10 priorities for planetary dune research:from Titus et al. (2008), Eos Trans. AGU, 89(45)
  • Facilitate better communication between scientists studying dunes on ALL planetary surfaces through joint research, future workshops, and special sessions at meetings.
  • Planetary Dunes Workshop 2010, Alamosa, CO
  • 2. More studies of terrestrial analogs are needed to better understand fundamental processes:
  • Field analog studies of BOTH morphology and processes are suggested.
  • Because Mars is a cold desert, terrestrial field study sites should include both cold deserts.
  • The potential importance of Pleistocene para- and peri-glacial landscapes is important, given the temperature regime of Mars and the widespread occurrence of frozen ground phenomena.
  • 3. Study the fundamental differences in atmospheric properties (especially density) between planetary bodies having an important effect on boundary layer characteristics and therefore sand transport processes. 4. The relations between dune orientations and winds are known in general terms, but information on specific dune fields is often lacking. 5. Development, completion and/or expansion of planetary dune databases is required.  Mars dune database nearing completion6. Additional research is needed to develop or refine dune classification schemes to consider both morphology and formation processes7. More research on the formation process of linear dunes is needed, especially those formed in the lee of topographic obstacles.8. More research is required to constrain physical properties of dune sands. 9. Additional numerical and laboratory studies are a priority for understanding observed dune patterns and the sedimentary history they record.10. Quantification of atmospheric parameters important to aeolian processes is necessary for understanding fundamental aspects of sediment transport on planetary surfacesyet such data are rarely acquired by landers and rovers. Inclusion of such instruments on future planetary missions is needed to advance understanding of the dynamics of wind transport of sediment on planetary surfaces.
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