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Orbital Evolution of Interplanetary Dust

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Interplanetary Dust

Part of the book series: Astronomy and Astrophysics Library ((AAL))

Abstract

The two most important dynamical features of the zodiacal cloud are: (i) t he dust bands associated with t he major Hirayama asteroid families, and (ii) the circumsolar ring of dust particles in resonant lock with th e Eart h. Oth er important dynamical features include the offset of th e center of symmetry of th e cloud from the Sun, the radial gradient of the ecliptic polar brightness at th e Earth, and th e warp of th e cloud. The dust bands provide th e st rongest evidence th at a substantial and possibly dominant fraction of the cloud originate s from aster oids. However, the characteristic diameter of these asteroidal particles is probably several hundred microns and the migration of th ese large particles towards th e inner Solar System due to Poynting Robert son light drag and their slow passage through secular resonances at the inner edge of the asteroid belt result s in large increases in th eir eccent ricities and inclinations. Because of these orbital changes, the dividing line between asteroidal and comet ary type orbits in the inner Solar System is probably not sharp, and it may be difficult to distinguish clearly between ast eroidal and cometary particles on dynamical grounds alone.

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Author information

Authors and Affiliations

  1. University Of Florida, Gainesville, Florida, USA

    Stanley F. Dermott & Thomas J. J. Kehoe

  2. Laboratory for Astronomy and Solar Physics, NASA Goddard Space Flight Center Code 681, 20771-0003, Greenbelt, MD, USA

    Keith Grogan

  3. Southwest Research Institute, 1050 Walnut Street, Suite 426, 80302, Boulder, CO, USA

    Daniel D. Durda

  4. Astronomy and Geophysics Divison, Vanguard Research, Inc., 5321 Scotts Valley Drive, Suite 204, 95066, Scotts Valley, CA, USA

    Sumita Jayaraman

  5. University of Maryland, Department of Astronomy, 1204 CSS Bldg, Stadium Dr, 20742-2421, College Park, MD, USA

    Stephen J. Kortenkamp

  6. University of Maryland, Department of Astronomy, 1204 CSS Bldg, Stadium Dr, 20742-2421, College Park, MD, USA

    Stephen J. Kortenkamp

  7. UK Astronomy Technology Centre, Royal Observatory, Blackford Hill, EH9 3HJ, Edinburgh, UK

    Mark C. Wyatt

Authors
  1. Stanley F. Dermott
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  2. Thomas J. J. Kehoe
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  3. Keith Grogan
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  4. Daniel D. Durda
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  5. Sumita Jayaraman
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  6. Stephen J. Kortenkamp
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  7. Mark C. Wyatt
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Editor information

Editors and Affiliations

  1. Saupfercheckweg 1, Max-Planck-Institut für Kernphysik, 69117, Heidelberg, Germany

    Eberhard Grün  & Hugo Fechtig  & 

  2. University of Florida, Department of Astronomy, 32611-2055, Gainesville, FL, USA

    Bo Å. S. Gustafson  & Stan Dermott  & 

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© 2001 Springer-Verlag Berlin Heidelberg

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Dermott, S.F. et al. (2001). Orbital Evolution of Interplanetary Dust. In: Grün, E., Gustafson, B.Å.S., Dermott, S., Fechtig, H. (eds) Interplanetary Dust. Astronomy and Astrophysics Library. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-56428-4_12

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  • DOI: https://doi.org/10.1007/978-3-642-56428-4_12

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-642-62647-0

  • Online ISBN: 978-3-642-56428-4

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