Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Assessing the Behavior of Moderately Volatile Elements on the Moon in Order to Constrain Processes of Magmatic Evolution and Planetary Accretion

Technical Report ·
DOI:https://doi.org/10.2172/2229028· OSTI ID:2229028
 [1]
  1. Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)

Heterogeneous isotopic compositions of Zn and Ga in lunar basalts and highlands rocks indicate that secondary processing affected the stable isotopic composition of major lunar reservoirs. It follows that these fractionating processes must be identified and characterized in order to make robust estimates for the isotopic composition of the mare basalt source regions or the bulk silicate Moon (BSM). Contrary to previous assertions (e.g., Kato & Moynier, 2017), MVEs such as Zn and Ga do not behave similarly on the Moon, in line with differences in their chemical behavior and volatility. There is clear evidence that impact reworking fractionates zinc isotopes but, in addition, zinc isotopes are also highly sensitive to the formation of Ti-bearing oxides such as ilmenite. In contrast, gallium is far less susceptible to volatile reworking, but its isotopic composition is fractionated during incorporation into plagioclase (Wimpenny et al., 2022; Render et al., 2023). Based on these findings we conclude that current isotopic compositions of Zn and Ga in lunar rocks, such as those measured for the mare basalt suite, are unlikely to be representative of the bulk Moon when it accreted. As such, estimates for the MVE isotopic composition of the BSM derived from mare basalts may not be accurate, which may have implications for the incorporation of these data into dynamical models of the Moon’s formation. In the following, we discuss the main findings from this project in more detail, focusing on the behaviour of zinc and gallium isotopic systematics in lunar rocks and the processes that control their isotopic fractionation on the Moon.

Research Organization:
Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)
Sponsoring Organization:
USDOE National Nuclear Security Administration (NNSA)
DOE Contract Number:
AC52-07NA27344
OSTI ID:
2229028
Report Number(s):
LLNL--TR-857352; 1087337
Country of Publication:
United States
Language:
English

Similar Records

Gallium isotopic constraints for the origin of the Earth-Moon system
Journal Article · Tue Apr 18 00:00:00 EDT 2023 · Earth and Planetary Science Letters · OSTI ID:1972423

The gallium isotopic composition of the Moon
Journal Article · Sun Dec 05 23:00:00 EST 2021 · Earth and Planetary Science Letters · OSTI ID:1888089

Lunar and terrestrial crust formation
Journal Article · Mon Nov 14 23:00:00 EST 1983 · J. Geophys. Res.; (United States) · OSTI ID:5016006

Related Subjects