EGU25-13945, updated on 04 May 2025
https://doi.org/10.5194/egusphere-egu25-13945
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Plasma on the lunar surface: Terra Incognita to be explored
Stas Barabash1, Yoshifumi Futaana1, Philipp Wittmann1, Thomas Maynadié1, Akbar Whizin2, and Angele Pontoni2
Stas Barabash et al.
  • 1Swedish Institute of Space Physics, Kiruna, Sweden (stas@irf.se)
  • 2Southwest Research Institute, San Antonio, USA

To date, plasma observations on the lunar surface have been very limited. Most of these observations were conducted during the Apollo program, relying on technology that is now over 50 years old, or by a few individual sensors with narrowly defined scientific objectives on Chinese landers. Our knowledge of the plasma environment and the processes that govern it remains sparse, relying heavily on orbital measurements and theoretical models. This current level of understanding is insufficient to support the large-scale exploration efforts that are about to commence. In essence, we are navigating a "Terra Incognita" in this domain.

To characterize and understand near-surface plasma and its interactions with the lunar surface are required for:

  • Properly modeling surface and man-made object charging and potentials;
  • Investigating dust dynamics, including dust release and dust-plasma interactions;
  • Studying weathering processes that modify surface characteristics and compositions;
  • Establishing the role of the space environment in the formation, release, and dynamics of volatiles within the lunar exosphere;
  • Understanding plasma dynamics at the surface and interactions with various plasma domains as the Moon moves along the orbit.

Plasma and its interaction processes need to be studied across four fundamental scales:

  • Microscale (kinetic, 10-4 – 10-2 cm) to address microphysics of the particle – surface interaction
  • Mesoscale (sub-Debye, 10 cm–10 m) to investigate plasma process when quasi-neutrality breaks creating strong electric fields
  • Macroscale (MHD, 10 m–1 km) to explore connections between plasma dynamics and topography
  • Global scale (MHD, 1 km–1,000 km) to reveal effects of large-scale structures, such as magnetic anomalies and the terminator, on local plasma populations.

In this presentation, we demonstrate the limitations of our current knowledge, highlight the critical importance of advancing it, and outline steps to explore the "Terra Incognita" of plasma on the lunar surface.

 

How to cite: Barabash, S., Futaana, Y., Wittmann, P., Maynadié, T., Whizin, A., and Pontoni, A.: Plasma on the lunar surface: Terra Incognita to be explored, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13945, https://doi.org/10.5194/egusphere-egu25-13945, 2025.