Dust particle ejection from the surface of a gas-filled cavity
The direct simulation Monte Carlo method was applied for calculation of dynamics of the gas-dust particle system within a problem of the near-nucleus gas-dust atmosphere of a comet. The study considers a gas-dynamic mechanism of dust particle ejection from the comet nucleus. This assumes existence of a dust-plugged cavity filled by sublimation products of icy content. Calculation offers the data on dust particle velocity as a function of key parameters. It is shown that the ejection velocity for a dust particle is described by one generalized parameter.
Authors
- N. Y. Bykov (ORCID: https://orcid.org/0000-0003-0041-9971)
- М. А. Никитин (ORCID: https://orcid.org/0000-0003-4855-8057)
- N V Obraztsov (ORCID: https://orcid.org/0000-0003-1107-3259)
- Viktor Zakharov (ORCID: https://orcid.org/0000-0001-9626-8543)
- I. A. Keresten (ORCID: https://orcid.org/0000-0001-7536-2258)
- D. N. Tonkov
Institutions
- Peter the Great St. Petersburg Polytechnic University (RU)
- Observatoire de Paris (FR)
Publication Details
- Journal
- Thermophysics and Aeromechanics
- Published
- 2025-07-25
- DOI
- https://doi.org/10.1134/s0869864324060180
- Primary Topic
- Astro and Planetary Science
- Type
- article
- Field-Weighted Citation Impact
- 0.00