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A permanent, asymmetric dust cloud around the Moon

Author

Listed:
  • M. Horányi

    (Laboratory for Atmospheric and Space Physics, University of Colorado
    University of Colorado
    Institute for Modeling Plasma, Atmospheres, and Cosmic Dust (IMPACT), University of Colorado)

  • J. R. Szalay

    (Laboratory for Atmospheric and Space Physics, University of Colorado
    University of Colorado
    Institute for Modeling Plasma, Atmospheres, and Cosmic Dust (IMPACT), University of Colorado)

  • S. Kempf

    (Laboratory for Atmospheric and Space Physics, University of Colorado
    University of Colorado
    Institute for Modeling Plasma, Atmospheres, and Cosmic Dust (IMPACT), University of Colorado)

  • J. Schmidt

    (Astronomy and Space Physics, University of Oulu)

  • E. Grün

    (Laboratory for Atmospheric and Space Physics, University of Colorado
    Institute for Modeling Plasma, Atmospheres, and Cosmic Dust (IMPACT), University of Colorado
    Max-Planck-Institut für Kernphysik)

  • R. Srama

    (Institut für Raumfahrtsysteme, Universität Stuttgart, Raumfahrtzentrum Baden Württemberg)

  • Z. Sternovsky

    (Laboratory for Atmospheric and Space Physics, University of Colorado
    Institute for Modeling Plasma, Atmospheres, and Cosmic Dust (IMPACT), University of Colorado
    Aerospace Engineering Sciences, University of Colorado)

Abstract

Observations are reported of a permanent, asymmetric dust cloud around the Moon, caused by impacts of high-speed cometary dust particles on eccentric orbits, as opposed to particles of asteroidal origin following near-circular paths striking the Moon at lower speeds.

Suggested Citation

  • M. Horányi & J. R. Szalay & S. Kempf & J. Schmidt & E. Grün & R. Srama & Z. Sternovsky, 2015. "A permanent, asymmetric dust cloud around the Moon," Nature, Nature, vol. 522(7556), pages 324-326, June.
    • Handle: RePEc:nat:nature:v:522:y:2015:i:7556:d:10.1038_nature14479
    DOI: 10.1038/nature14479
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