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On structural properties of Comet 67/P dust particles collected in situ by ROSETTA/COSIMA from observations of electrical fragmentation

MPS-Authors
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Stenzel,  Oliver J.
Planetary Science Department, Max Planck Institute for Solar System Research, Max Planck Society;

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Merouane,  Sihane
Planetary Science Department, Max Planck Institute for Solar System Research, Max Planck Society;

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Fischer,  Henning
Planetary Science Department, Max Planck Institute for Solar System Research, Max Planck Society;

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Paquette,  John
Planetary Science Department, Max Planck Institute for Solar System Research, Max Planck Society;

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Hilchenbach,  Martin
Planetary Science Department, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Hornung, K., Maria Mellado, E., Stenzel, O. J., Langevin, I., Merouane, S., Fray, N., et al. (2023). On structural properties of Comet 67/P dust particles collected in situ by ROSETTA/COSIMA from observations of electrical fragmentation. Planetary and Space Science, 236, 105747. doi:10.1016/j.pss.2023.105747.


Cite as: https://hdl.handle.net/21.11116/0000-000F-33A2-0
Abstract
After landing on the target, the kinetic energy can be dissipated within the fragment if it consists of many elements (as in the example of the Kerttu-Ender fragment, Fig. 2). If it consists of only a few elements, as is the case for most fragments traveling longer distances, the kinetic energy is dissipated by rolling. In the case of impact fragmentation, rolling was the only possible displacement process of the fragments. Their typical rolling distances were of the order of several 100 μm , suggesting that the relevant forces between dust and target are of the van der Waals type. After adding the rolling contribution for the simplest case of a single element emitted, the total ejection distance becomes