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

Authors :
Sarah Vines
George Ho
David Blewett
Jasper Halekas
Benjamin Greenhagen
Brian Anderson
Dany Waller
Jörg-Micha Jahn
Peter Kollmann
Brett Denevi
Heather Meyer
Rachel Klima
Joshua Cahill
Lon Hood
Sonia Tikoo
Xiao-Duan Zou
Mark Weiczorek
Myriam Lemelin
Shahab Fatemi
Edward Cloutis
Publication Year :
2023
Publisher :
Copernicus GmbH, 2023.

Abstract

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.

Details

Database :
OpenAIRE
Accession number :
edsair.doi...........33a3083a29b1d1ebf442b8bf357b61ee
Full Text :
https://doi.org/10.5194/egusphere-egu23-10526