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Mineralogical, Elemental, and Tomographic Reconnaissance Investigation for CLPS (METRIC): A Proposed Mission to the Lunar South Pole-Aitken BasinThe global Lunar Magma Ocean (LMO) hypothesis is based on analyses of ferroan anorthosites (FAN), magnesian plutonic rocks (Mg-suite), and KREEPy (Potassium - K; Rare Earth Elements - REE; Phosphorous - P) material present at the Apollo landing sites and the assumed global distribution of these lithologies. However, orbital spacecraft data over the last two decades have highlighted that the location of the Apollo missions within and near the Procellarum KREEP Terrane (PKT) is compositionally anomalous and not representative of the entire lunar surface and suggests that Apollo samples provide a biased view of the Moon. Further, meteorites, which originate from random areas on the lunar surface, including those not visited by Apollo, Luna, or Chang’E-5, provide complementary datasets that reveal a more complex lunar formation and evolution than the simple LMO onion skin model. While many recent investigations support and refine the LMO model, other recent studies have questioned whether this mechanism alone is responsible for the primordial differentiation of the Moon. Thus, relating the distinct and asymmetrically distributed geochemical terranes on the Moon, especially KREEP which is a predicted global LMO product, to lunar formation and differentiation remains a fundamental goal of lunar science.

The South Pole-Aitken (SPA) impact carved a two-and-a-half thousand-kilometer basin into the Moon’s ancient crust, excavating material from as deep as the upper mantle. Orbital remote sensing of the basin indicates compositions with elevated thorium (Th) contents and unique mineralogies that provide a window into early lunar structure and LMO processes. We propose to land a powerful characterization laboratory at Birkeland crater on the far side of the Moon–where Th-rich SPA ejecta have been re-exposed near the surface–in order to address outstanding questions about the evolution of the Moon.
Document ID
20230000383
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
K M Cannon
(Colorado School of Mines Golden, Colorado, United States)
E Rampe
(Johnson Space Center Houston, Texas, United States)
E Malaret
(ACT Inc.)
I King
(Honeybee Robotics (United States) Brooklyn, New York, United States)
J Chen
(Baja Technology)
J Gross
(Rutgers University Houston, Texas, United States)
A Yen
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Z Wilbur
(University of Arizona Tucson, Arizona, United States)
R Ewing
(Texas A&M University System College Station, Texas, United States)
P Mcnally
(University of Michigan–Ann Arbor Ann Arbor, Michigan, United States)
R Hanna
(The University of Texas at Austin Austin, Texas, United States)
A Udry
(University of Nevada, Las Vegas Las Vegas, Nevada, United States)
D Vaniman
(Planetary Science Institute Tucson, Arizona, United States)
J Barnes
(University of Arizona Tucson, Arizona, United States)
M Gailhanou
(Aix-Marseille University Marseille, France)
J Hamilton
(Johnson Space Center Houston, Texas, United States)
D P Moriarty
(University of Maryland, College Park College Park, Maryland, United States)
D Blake
(Ames Research Center Mountain View, California, United States)
D Bergman
(Honeybee Robotics (United States) Brooklyn, New York, United States)
R Obbard
(SETI Institute Mountain View, California, United States)
V A Sole
(European Synchrotron Radiation Facility Grenoble, Rhône-Alpes, France)
P G Lucey
(University of Hawaii System Honolulu, Hawaii, United States)
P Sarrazin
(Examinart, LLC Mountain View, California, United States)
J Hammer
(University of Hawaii System Honolulu, Hawaii, United States)
B L Valverde
(SETI Institute Mountain View, California, United States)
R Downs
(University of Arizona Tucson, Arizona, United States)
C Haberle
(Northern Arizona University Flagstaff, Arizona, United States)
R Christoffersen
(Jacobs (United States) Dallas, Texas, United States)
K Prissel
(Jacobs (United States) Dallas, Texas, United States)
J Bullard
(Texas A&M University System College Station, Texas, United States)
T Prissel
(Jacobs (United States) Dallas, Texas, United States)
K Thompson
(SETI Institute Mountain View, California, United States)
N Vo
(Brookhaven National Laboratory Upton, New York, United States)
Date Acquired
January 10, 2023
Subject Category
Lunar and Planetary Science and Exploration
Meeting Information
Meeting: 54th Lunar and Planetary Science Conference (LPSC)
Location: The Woodlands, TX
Country: US
Start Date: March 13, 2023
End Date: March 17, 2023
Sponsors: Lunar and Planetary Institute
Funding Number(s)
WBS: 811073.02.52.01.11
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
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