• DocumentCode
    3675317
  • Title

    Electrostatic dust levitation near asteroid Itokawa

  • Author

    Christine M. Hartzell;Michael Zimmerman

  • Author_Institution
    University of Maryland, College Park, 20742, United States
  • fYear
    2015
  • fDate
    5/1/2015 12:00:00 AM
  • Firstpage
    1
  • Lastpage
    1
  • Abstract
    A plasma sheath is created when the solar wind and solar UV radiation interact with the surface of airless planetary bodies, such as the Moon and asteroids. It has been hypothesized that, due to the low gravity of these bodies (as much as 5 orders of magnitude smaller than Earth´s gravity), small dust grains may levitate in the plasma sheaths. Observational evidence for planetary dust levitation is weak: Surveyor horizon glow observations from the Moon have been attributed to zodiacal light after re-analysis. and levitation is one of several possible explanations for the ‘dust ponds’ on the asteroid Eros. However, electrostatic dust levitation has been observed in the lab. Additionally, we have shown that dust levitation is possible (and that stable levitation can occur) near asteroids using numerical simulations with simplified asteroid shape and plasma models.
  • Publisher
    ieee
  • Conference_Titel
    Radio Science Conference (URSI AT-RASC), 2015 1st URSI Atlantic
  • Type

    conf

  • DOI
    10.1109/URSI-AT-RASC.2015.7303165
  • Filename
    7303165