Large Dust Grains Around Cometary Nuclei

• Published in: Earth, moon, and planets moon, and planets, 2008-06, Vol.102 (1-4), p.521-524
• Main Authors: Molina, A., Moreno, F., Jiménez-Fernández, F. J.
• Format: Article
• Language: English
• Subjects: Astronomy; Astrophysics; Astrophysics and Astroparticles; Centrifugal force; Comet nuclei; Comets; Dust; Grains; Observations and Techniques; Orbital stability; Orbits; Particle physics; Physics; Physics and Astronomy; Planetology; Radiation pressure; Rotation; Solar radiation; Space Exploration and Astronautics; Space Sciences (including Extraterrestrial Physics
• ISSN: 0167-9295; 1573-0794
• DOI: 10.1007/s11038-007-9158-2

Large amounts of particles ejected from the nucleus surface are present in the vicinity of the cometary nuclei when comets are near the Sun (at heliocentric distances ≤2 AU). The largest dust grains ejected may constitute a hazard for spatial vehicles. We tried to obtain the bounded orbits of those particles and to investigate their stability along several orbital periods. The model includes the solar and the cometary gravitational forces and the solar radiation pressure force. The nucleus is assumed to be spherical. The dust grains are also assumed to be spherical, and radially ejected. We include the effects of centrifugal forces owing to the comet rotation. An expression for the most heavy particles that can be lifted is proposed. Using the usual values adopted for the case of Halley’s comet, the largest grains that can be lifted have a diameter about 5 cm, and the term due to the rotation is negligible. However, that term increases the obtained value for the maximum diameter of the lifted grain in a significant amount when the rotation period is of the order of a few hours.