Modeling of the orbital evolution of vaporizing dust particles near the sun

  • Zdenek Sekanina
5 Dynamics and Evolution
Part of the Lecture Notes in Physics book series (LNP, volume 48)


Kcal Mole Interplanetary Magnetic Field Radiation Pressure Solar Radiation Pressure Final Particle Size 
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  1. Robertson, H. P. (1937), Mon. Not. Roy. Astron. Soc., 97, 423.Google Scholar
  2. Whipple, F. L. (1955), Astrophys. J., 121, 750.Google Scholar
  3. Whipple, F. L. (1967), in “The Zodiacal Light and the Interplanetary Medium”, Weinberg, J.L., Ed., NASA SP-150, Washington, D.C., p. 409.Google Scholar
  4. Wyatt, S. P., and Whipple, F. L. (1950), Astrophys. J., 111, 134.Google Scholar

Copyright information

© Springer-Verlag 1976

Authors and Affiliations

  • Zdenek Sekanina
    • 1
  1. 1.Center for Astrophysics Harvard College Observatory and Smithsonian Astrophysical ObservatoryCambridgeUSA

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