EGU26-21022, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-21022
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Thursday, 07 May, 16:15–18:00 (CEST), Display time Thursday, 07 May, 14:00–18:00
 
Hall X4, X4.139
Interstellar dust predictions for the Destiny+ mission
Timour Jestin1, Silvan Hunziker, Peter Strubb3, Harald Krüger3, Georg Moragas-Klostermeyer, Ralf Srama, Tranquillo Janisch, and Veerle Sterken2,1
Timour Jestin et al.
  • 1ETHZ
  • 2EPFL (veerle.sterken@epfl.ch)
  • 3University of Göttingen, MPI fur Sonnensystemforschung, Göttingen, 37077, Germany

Destiny+ is a Japanese-German space mission to be launched in 2028, first flying by the near Earth Asteroid Apophis in 2029 after which it will continue on its route to the active asteroid Phaeton for a flyby in 2030. The period around 2029-2030 is in the phase of the solar cycle in which small interstellar dust and cometary dust is focused near the ecliptic plane. This presents unique and ideal conditions for in situ measurements of interstellar dust in the solar system, close to the Earth. We present predictions for the interstellar dust flux and flow direction that Desiny+ will be able to measure for different assumed material properties. We use two prediction methods of which one is designed to take into account the filtering in the heliosheath using previous in situ measurements.

How to cite: Jestin, T., Hunziker, S., Strubb, P., Krüger, H., Moragas-Klostermeyer, G., Srama, R., Janisch, T., and Sterken, V.: Interstellar dust predictions for the Destiny+ mission, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21022, https://doi.org/10.5194/egusphere-egu26-21022, 2026.