EGU23-10526
https://doi.org/10.5194/egusphere-egu23-10526
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Lunar Vertex: A PRISM Science Investigation of the Reiner Gamma Lunar Magnetic Anomaly and Swirl

Sarah Vines1, George Ho1, David Blewett1, Jasper Halekas2, Benjamin Greenhagen1, Brian Anderson1, Dany Waller1, Jörg-Micha Jahn3, Peter Kollmann1, Brett Denevi1, Heather Meyer1, Rachel Klima1, Joshua Cahill1, Lon Hood4, Sonia Tikoo5, Xiao-Duan Zou6, Mark Weiczorek7, Myriam Lemelin8, Shahab Fatemi9, and Edward Cloutis10
Sarah Vines et al.
  • 1Johns Hopkins University Applied Physics Laboratory, Laurel, MD, USA
  • 2University of Iowa, Iowa City, IA, USA
  • 3Southwest Research Institute, San Antonio, TX, USA
  • 4University of Arizona, Tucson, AZ, USA
  • 5Stanford University, Stanford, CA, USA
  • 6Planetary Science Institute, Tucson, AZ, USA
  • 7Observatoire de la Côte d'Azur, Nice, France
  • 8Université de Sherbrooke, Sherbrooke, QC, Canada
  • 9Umeå Universitet, Umeå, Sweden
  • 10University of Winnipeg, Winnipeg, MB, Canada

Lunar Vertex is a mission at the intersection of multiple science communities, from planetary geology to space plasma physics. As the first Payloads and Research Investigations on the Surface of the Moon (PRISM1) investigation, scheduled for delivery to the Reiner Gamma (RG) magnetic anomaly in 2024 aboard a commercial lunar lander, Lunar Vertex will unravel the nature of the RG anomaly, the connection to and origin of the associated lunar swirl surface feature, and the structure and impact of the “mini-magnetosphere” in this region. Lunar Vertex includes a suite of magnetometers (Vector Magnetometer – Lander; VML), a fixed-mounted set of cameras (Vertex Camera Array; VCA), and a low-energy ion and electron plasma analyzer (Magnetic Anomaly Plasma Spectrometer; MAPS) on the lander. In addition, a second suite of commercial fluxgate magnetometers (Vector Magnetometer – Rover; VMR) and a multispectral imager (Rover Multispectral Microscope; RMM) are mounted on a dedicated rover that will traverse a distance of at least 500 m from the lander, providing additional multi-point measurements. The combination of magnetic field measurements taken during cruise and descent by VML and during surface operations by both VML and VMR will characterize the surface magnetic field within a strong lunar magnetic anomaly. The combined magnetic field and plasma measurements from VML and MAPS will provide direct observations of plasma populations reaching the lunar surface and the associated local magnetic field configuration. Furthermore, the lunar regolith within the RG magnetic anomaly and over different regions of the associated lunar swirl will be characterized by RMM and VCA to reveal the surface texture, composition, and particle distribution around both the lander and rover locations and the correspondence to potential surface weathering processes.

How to cite: Vines, S., Ho, G., Blewett, D., Halekas, J., Greenhagen, B., Anderson, B., Waller, D., Jahn, J.-M., Kollmann, P., Denevi, B., Meyer, H., Klima, R., Cahill, J., Hood, L., Tikoo, S., Zou, X.-D., Weiczorek, M., Lemelin, M., Fatemi, S., and Cloutis, E.: Lunar Vertex: A PRISM Science Investigation of the Reiner Gamma Lunar Magnetic Anomaly and Swirl, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-10526, https://doi.org/10.5194/egusphere-egu23-10526, 2023.