Issue |
A&A
Volume 678, October 2023
|
|
---|---|---|
Article Number | A192 | |
Number of page(s) | 24 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/202346442 | |
Published online | 24 October 2023 |
Size-dependent charging of dust particles in protoplanetary disks
Can turbulence cause charge separation and lightning?
1
Austrian Academy of Science, Space Research Institute,
Schmiedlstrasse 6,
8042
Graz,
Austria
e-mail: Thorsten.Balduin@oeaw.ac.at
2
TU Graz, Faculty of Mathematics, Physics and Geodesy,
Petersgasse 16,
8010
Graz,
Austria
3
Centre for ExoLife Sciences (CELS), Niels Bohr Institute,
Østervoldgade 5,
1350
Copenhagen,
Denmark
4
Max Planck Institute for Extraterrestrial Physics,
Giessenbachstrasse 1,
85748
Garching,
Germany
Received:
16
March
2023
Accepted:
1
August
2023
Context. Lightning can have a profound impact on the chemistry of planetary atmospheres. In a similar manner, as protoplanetary disks are the foundation of planet formation, the emergence of lightning in protoplanetary disks can substantially alter their chemistry.
Aims. We aim to study under which conditions lightning could emerge within protoplanetary disks.
Methods. We employed the PRODIMO code to make 2D thermo-chemical models of protoplanetary disks. We included a new way of how the code handles dust grains, which allows the consideration of dust grains of different sizes. We investigated the chemical composition, dust charging behavior, and charge balance of these models to determine which regions could be most sufficient for lightning.
Results. We identify six regions within the disks where the charge balance is dominated by different radiation processes and find that the emergence of lightning is most probable in the lower and warmer regions of the midplane. This is due to the low electron abundance (nе/n〈H〉 < 10−15) in these regions and dust grains being the most abundant negative charge carriers (nZ/n〈H〉 > 10−13). We find that NH4+ is the most abundant positive charge carrier in those regions at the same abundances as the dust grains. We developed a method of inducing electric fields via turbulence within this mix of dust grains and NH4+. The electric fields generated with this mechanism are however several orders of magnitude weaker than required to overcome the critical electric field.
Key words: protoplanetary disks
© The Authors 2023
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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