Whence Comets?

Author:

A'Hearn Michael F.1

Affiliation:

1. Department of Astronomy, University of Maryland, College Park, MD 20742–2421, USA.

Abstract

Recent advances in cometary science have indicated the importance of mixing of materials in the disk where the planets of our solar system formed. Now, the results from the Stardust Discovery Mission unambiguously show that even more extensive and earlier mixing of the material took place, raising new challenges for theories of the protoplanetary disk and the formation of comets.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference10 articles.

1. M. Duncan, H. Levison, L. Dones, in Comets II, M. C. Festou, H. U. Keller, H. A. Weaver, Eds. (Univ. of Arizona Press, Tucson, AZ, 2004), pp. 193–204.

2. The scattered disk population as a source of Oort cloud comets: evaluation of its current and past role in populating the Oort cloud

3. Comparison of USGS and DLR topographic models of Comet Borrelly and photometric applications

4. The nucleus of Comet Borrelly: a study of morphology and surface brightness

5. R. L. Kirk et al., Lunar Planet. Sci.XXXVI, 2244 (2005).

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