SpringerLink
Forum Springer Astron. Astrophys.
Forum Whats New Search Orders


Astron. Astrophys. 347, 366-369 (1999)


Table of Contents
Available formats: HTML | PDF | (gzipped) PostScript

Comet Hale-Bopp as a free-rotation rigid body

A. Molina 1,2 and F. Moreno 2

1 Departamento de Física Aplicada, Universidad de Granada, Spain
2 Instituto de Astrofísica de Andalucía, CSIC, P.O. Box 3004, E-18080 Granada, Spain

Received 28 October 1998 / Accepted 5 March 1999

Abstract

After considering the advantages of using such a simple mechanical model, the nucleus of Comet Hale-Bopp is treated as a free rotation symmetrical top. Although most authors have rejected the periodicity of more than 20 days, we considered in our analysis a possible complex rotational state with the 11.30 hour and the 20-24 day periods. From our model, a complex rotation could be possible if the large period is the spin around the axis of minimum moment of inertia (long axis) and the accepted 11.30 hour period corresponds to a free precession motion. The motion of precession should be nearly perpendicular to the direction of the long axis of the Comet, and then it should be in conflict with the observed stability of the shell structures. Because this result is independent of the axes ratio for reasonable values, we conclude that the complex rotational state is not compatible with observations.

Key words: comets: individual: C/1995 01 Hale-Bopp

Send offprint requests to: A. Molina

© European Southern Observatory (ESO) 1999

Online publication: June 18, 1999

helpdesk.link@springer.de