Hostname: page-component-cd9895bd7-lnqnp Total loading time: 0 Render date: 2024-12-26T03:24:10.612Z Has data issue: false hasContentIssue false
  • English
  • Français

3.3 Can Short Period Comets Maintain the Zodiacal Cloud?

Published online by Cambridge University Press:  12 April 2016

S. Röser
S. Röser*
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg-Königstuhl, FRG

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The combined effects of the Poynting-Robertson drag, collisions and sputtering are destroying the interplanetary dust cloud. The mass-losses estimated by different authors reveal great discrepancies. The estimations range from 1 t sec−1 (purely Poynting-Robertson loss) over some 10 t sec−1 given by Whipple (1967) to a value of 100 t sec−1 which is propagated by Bandermann (1967). The latter derives this high value from the assumption that the main mass loss is due to self-collisions.

Type
3 Cometary Dust
Information
International Astronomical Union Colloquium , Volume 31: Interplanetary Dust and Zodiacal Light , 1976 , pp. 319 - 322
Copyright
Copyright © Springer-Verlag 1976

References

Bandermann, L.W.; Physical Properties and Dynamics of Interplanetary Dust, University of Maryland, Technical Report No 771 (1967)Google Scholar
Finson, M.L. and Probstein, R.F.; A Theory of Dust Comets, ApJ 154, 327 (1968)CrossRefGoogle Scholar
Sekanina, Z. and Miller, F.D.; Comet Bennett (1970 II), Science 179, 565 (1973)Google Scholar
Wachmann, A.; in “Landold – Börnstein”, Zahlenwerte und Funktionen,< New Series, Group VI, Vol. 1, 176 (1965)Google Scholar
Whipple, F.; in “The Zodiacal Light and the Interplanetary Medium”, ed. by Weinberg, J.L., NASA SP 150, 409 (1967)Google Scholar