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  Dynamics of Dust Particles of Different Structure: Application to the Modeling of Dust Motion in the Vicinity of the Nucleus of Comet 67P/Churyumov–Gerasimenko

Reshetnyk, V. M., Skorov, Y. V., Lacerda, P., Hartogh, P., & Rezac, L. (2018). Dynamics of Dust Particles of Different Structure: Application to the Modeling of Dust Motion in the Vicinity of the Nucleus of Comet 67P/Churyumov–Gerasimenko. Solar System Research, 52(3), 266-281. doi:10.1134/S0038094618030085.

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Item Permalink: http://hdl.handle.net/21.11116/0000-0001-E713-5 Version Permalink: http://hdl.handle.net/21.11116/0000-0007-0B61-0
Genre: Journal Article

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Reshetnyk, V. M., Author
Skorov, Yuri V.1, Author              
Lacerda, P., Author
Hartogh, Paul1, Author              
Rezac, Ladislav1, Author              
Affiliations:
1Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832288              

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Free keywords: comet cometary dust coma modeling
 MPIS_PROJECTS: ROSETTA: MIRO
 Abstract: We consider the estimates of the main forces acting on dust particles near a cometary nucleus. On the basis of these estimates, the motion of dust particles of different structure and mass is analyzed. We consider the following forces: (1) the cometary nucleus gravity, (2) the solar radiation pressure, and (3) the drag on dust particles by a flow of gas produced in the sublimation of cometary ice. These forces are important for modeling the motion of dust particles relative to the cometary nucleus and may substantially influence the dust transfer over its surface. In the simulations, solid silicate spheres and homogeneous ballistic aggregates are used as model particles. Moreover, we propose a technique to build hierarchic aggregates—a new model of quasi-spherical porous particles. A hierarchic type of aggregates makes it possible to model rather large dust particles, up to a millimeter in size and larger, while no important requirements for computer resources are imposed. We have shown that the properties of such particles differ from those of classical porous ballistic aggregates, which are usually considered in the cometary physics problems, and considering the microscopic structure of particles is of crucial significance for the analysis of the observational data. With the described models, we study the dust dynamics near the nucleus of comet 67P/Churyumov–Gerasimenko at an early stage of the Rosetta probe observations when the comet was approximately at 3.2 AU from the Sun. The interrelations between the main forces acting on dust aggregates at difference distances from the nucleus have been obtained. The dependence of the velocity of dust aggregates on their mass has been found. The numerical modeling results and the data of spaceborne observations with the Grain Impact Analyzer and Dust Accumulator (GIADA) and the Cometary Secondary Ion Mass Analyzer (COSIMA) onboard the Rosetta probe are compared at a quantitative level.

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Language(s): eng - English
 Dates: 2018-08-082018
 Publication Status: Published in print
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Method: Peer
 Identifiers: DOI: 10.1134/S0038094618030085
 Degree: -

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Title: Solar System Research
  Other : Solar Syst. Res.
Source Genre: Journal
 Creator(s):
Affiliations:
Publ. Info: New York : Consultants Bureau.
Pages: - Volume / Issue: 52 (3) Sequence Number: - Start / End Page: 266 - 281 Identifier: ISSN: 0038-0946
CoNE: https://pure.mpg.de/cone/journals/resource/958480223880