EGU2020-2955
https://doi.org/10.5194/egusphere-egu2020-2955
EGU General Assembly 2020
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Development of the NIM Mass spectrometer for Exploration of Jupiter’s Icy Moons Exospheres

Martina Föhn1, Marek Tulej1, André Galli1, Audrey Helena Vorburger1, Davide Lasi1, Peter Wurz1, Pontus Brandt2, and Stas Barabash3
Martina Föhn et al.
  • 1University of Bern, Physics Institute, Space Research & Planetary Sciences, Bern, Switzerland (martina.foehn@space.unibe.ch)
  • 2Johns Hopkins University Applied Physics Laboratory, Laurel, MD, USA
  • 3Swedish Institute of Space Physics, Kiruna, Sweden

Investigation of habitable environments is one of the main objectives in upcoming space missions. The JUICE mission will investigate Jupiter’s environment in the solar system and its icy moons Ganymede, Callisto and Europa as examples for potentially habitable worlds around a gas giant. The Particle Environment Package (PEP) on the JUICE satellite will investigate Jupiter’s icy moons and their environment. As part of PEP, the Neutral gas and Ion Mass spectrometer (NIM) will measure the chemical composition of the exospheres of the icy moons. These measurements give information about the surface composition of the moons and will set constraints on their formation processes.

NIM is a Time of Flight mass spectrometer with two entrances for neutral particles and ions. The gas enters the instrument from spacecraft ram direction. With the open source neutral particles and ions enter the ionisation region directly. With the closed source neutral particles get thermalized using an antechamber before entering the ion source. Particles entering with higher velocity are therefore easier to detect through the antechamber.

Initial performance tests with the NIM Protoflight Model (PFM) were done. The storage capability of the ion source was tested, the functionality of the antechamber was verified and we measured masses up to 642 u to demonstrate the high-mass performance of NIM. Furthermore, different subunits of the NIM instrument were successfully tested, such as the redesigned ion source and flight electronics connected with the NIM sensor head.

How to cite: Föhn, M., Tulej, M., Galli, A., Vorburger, A. H., Lasi, D., Wurz, P., Brandt, P., and Barabash, S.: Development of the NIM Mass spectrometer for Exploration of Jupiter’s Icy Moons Exospheres, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-2955, https://doi.org/10.5194/egusphere-egu2020-2955, 2020

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