Comet Size Distributions and Distant Activity View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

2000

AUTHORS

Karen J. Meech , Olivier R. Hainaut , Brian G. Marsden

ABSTRACT

.We present the results of observations of distant comet nuclei as observed with the Keck II telescope during 1997 December. Our sample included 17 SP Jupiter-family comets, 3 Halley-family comets, and 1 dynamically new comet. The nucleus radii ranged between 0.6 and 12.7 km (assuming a 4% albedo), the average near RN\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$\sim$\end{document}3 km showing that, in general, the comet nuclei are relatively small. This doubles the known sample of size estimates for the comet population. These data are compared to the size distributions for the Centaurs and the Edgeworth-Kuiper Belt objects. More... »

PAGES

75-80

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/10651968_10

DOI

http://dx.doi.org/10.1007/10651968_10

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1024091227


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