Hostname: page-component-848d4c4894-tn8tq Total loading time: 0 Render date: 2024-07-05T15:39:31.406Z Has data issue: false hasContentIssue false
  • English
  • Français

Sources of 10 micron Interplanetary Dust: The Contribution from the Kuiper Belt

Published online by Cambridge University Press:  27 February 2018

G. J. Flynn
G. J. Flynn*
Affiliation:
Dept of Physics, SUNY-Plattsburgh, Plattsburgh, NY 12901

Abstract

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.

Two major sources are observed to contribute to the Zodiacal Cloud: main-belt asteroids and active comets. However, the discovery of 100 km size objects in trans-Neptunian orbits (Jewitt & Luu 1993) coupled with Pioneer 10 measurements showing an essentially constant flux of 10 μm dust from 4 to 18 AU with indications that dust may be in near-circular orbits (Humes 1980) suggests that collisions in the Kuiper Belt may contribute significantly to the Zodiacal Cloud and to the interplanetary dust collected from the Earth's stratosphere. Kuiper Belt dust collected at Earth could be identified by high densities of solar flare tracks, unusually thick amorphous rims, and high concentrations of spallogenic isotopes.

Type
IV. Origin of the Interplanetary Dust Cloud
Information
International Astronomical Union Colloquium , Volume 150: Physics, Chemistry and Dynamics of Interplanetary Dust , 1996 , pp. 171 - 175
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

Bibring, J. P et al. 1972, Science, 175, 753 Google Scholar
Bradley, J. P. & Brownlee, D. E. 1986, Science, 231, 1542 Google Scholar
Christopherson, R. & McKay, D. 1995, Lunar & Planetary Science XXVI, 245 Google Scholar
Cochran, A. L., Levison, H. F., Stern, S. A., & Duncan, M. J. 1995, Ap.J., in press.Google Scholar
Dermott, S. F. et al. 1994, in Asteroids, Comets, and Meteors 1993, Milani, A. et al. eds., Dordrecht: Kluwer, 153 Google Scholar
Flynn, G.J. 1989, Icarus, 77, 287 Google Scholar
Flynn, G. J. 1992, in Asteroids, Comets, and Meteors 1991, Harris, A. W. & Bowell, E. eds., Houston: LPI Publication Services, 195 Google Scholar
Flynn, G. J. 1994, Lunar & Planetary Science XXV, 379 Google Scholar
Humes, D. H. 1974, J. Geophys. Res., 79, 3677 Google Scholar
Humes, D. H. 1980, J. Geophys. Res., 85, 5841 Google Scholar
Jackson, A. A. & Zook, H. A. 1992, Icarus, 97, 70 Google Scholar
Jewitt, D. & Luu, J. 1993, Nature, 362, 730 Google Scholar
Jewitt, D. & Luu, J. 1995, Astron. J., 109, 1867 Google Scholar
Liou, J. C. et al. 1995, Lunar & Planetary Science XXVI, 853 Google Scholar
Liou, J. C. et al. 1996, these proceedingsGoogle Scholar
Love, S. G. & Brownlee, D. E. 1993, Science, 262, 550 Google Scholar
Nishiizumi, K. et al. 1991, Earth and Planet. Sci. Lett., 104, 315 CrossRefGoogle Scholar
Sandford, S. A. & Bradley, J. P. 1990, Icarus, 82, 146 Google Scholar