Volcanic activity of the Moon and chemical characterisation of the lunar mantle
The purpose of this project is to understand the evolution of the Moon’s mantle through time by deciphering the origin of the chemical characteristics of lunar basaltic rocks.
Details
- Period: 2021-01-01 – 2024-12-31
- Budget: 3,360,000 SEK
- Funder: Swedish Research Council
- Type of funding: Project grant
Description
This project involves the determination of high-accuracy in-situ U-Pb dates and initial Pb isotope ratios by SIMS in lunar gabbros and basalts.
This is followed by the determination of the initial Sr-Nd-Hf radiogenic isotope ratios and Fe stable isotope ratios by Multi-Collection Inductively Coupled Mass Spectrometry (MC-ICP-MS) using wet chemistry on the dated samples.
In addition, a new pilot project is focusing on in-situ determination by SIMS (CAMECA IMS 1280) of halogen contents (F, I, Cl, Br) and Cl isotopic ratios in phosphates from a limited number of basalts and gabbros.
Project members
Publications
A micrometeorite from a stony asteroid identified in Luna 16 soil
Part of Nature Astronomy, p. 560-567, 2022
Pb Isotope Signature of a Low-Ό (238U/204Pb) Lunar Mantle Component
Part of Journal of Petrology, 2024
Part of Geochimica et Cosmochimica Acta, p. 206-243, 2022