Granulometric composition of dust inclusions and the secular brightness decrease of periodic comets

Details Granulometric composition of dust inclusions and the secular brightness decrease of periodic comets Granulometric composition of dust inclusions and the secular brightness decrease of periodic comets

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...35d&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, Mar.-Apr. 1986, p. 35-38. In Russian.

Mathematics

Brightness Distribution, Comets, Cosmic Dust, Particle Size Distribution, Perihelions, Secular Variations, Branching (Mathematics), Cosmochemistry, Granular Materials, Mineralogy, Solar System

Scientific paper

The bifurcated shape of the secular brightness decrease vs perihelion distance curve is explained by the existence of two groups of periodic comets with different granulometric compositions. This conclusion implies the possibility of different origins of the dust component in the two groups of comets and may indicate that the groups themselves are of different origin (e.g., formed in different regions of the protosolar nebula).

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