EXPERIMENTAL CONSTRAINTS ON THE ISOTOPE SIGNATURES OF THE EARLY SOLAR SYSTEM

Project Information

COSMOKEMS

Grant agreement ID: 694819

DOI

10.3030/694819

Project closed

EC signature date 20 June 2016

Start date 1 October 2016

End date 31 March 2024

Funded under

• EXCELLENT SCIENCE - European Research Council (ERC)

Total cost

€ 3 106 625,00

EU contribution

€ 3 106 625,00

Coordinated by

CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS
France

Periodic Reporting for period 5 - COSMOKEMS (EXPERIMENTAL CONSTRAINTS ON THE ISOTOPE SIGNATURES OF THE EARLY SOLAR SYSTEM)

Reporting period: 2023-04-01 to 2024-03-31

Summary of the context and overall objectives of the project

This project aimed at understanding better how the planets of the Solar System acquired their chemical and isotope compositions and how these characteristics can be used to identify the processes that transformed the initial dust of the early Solar System to typical planetary materials.
The environment around the Sun was very different from what it is today and this has greatly influenced the shaping of solid materials forming the terrestrial planet region. High temperatures, coupled with significant irradiation stemming from the young Sun could have transformed the gas and dust part of the protoplanetary disk. Similarly, the formation of the Moon resulting from a giant impact with the Earth could also have created high temperature conditions that would have modified the composition of the materials finally accreting to the Moon. In this project, we attempted to reproduce experimentally some of these conditions and investigate how such environments could have left specific isotope signatures that could be used as fingerprints for reconstructing those past environments. We will specifically study the conditions of evaporation and condensation by investigating isotope fractionation in equilibrium between condensed phase and vapor. Second we will investigated the potential role of particle irradiation on the isotope composition of dust present in the protoplanetary disk. Altogether our experiments will provide quantitative constraints on how terrestrial planets were shaped chemically.

Work performed from the beginning of the project to the end of the period covered by the report and main results achieved so far

The first part of this project was dedicated to designing and constructing a new mass spectrometer with the ability to measure the elemental and isotope composition of a vapor in chemical and isotope equilibrium with a condensed phase contained in a Knudsen cell. It was decided that the new mass spectrometer would be fitted to a currently existing double focusing instrument equipped with a multicollection system, the Neptune Plus produced by THERMO Fisher Instruments. A key issue was to ensure that the sensitivity and stability of the instrument would be sufficient for precise isotope measurements. For this purpose, we have modeled the molecular beam transmission, the electron beam emitted by filaments facing each other and the ion beam extracted into the mass spectrometer with the aim of optimizing the molecular beam transmission, improving the electron focusing onto the molecular beam and enhancing the ion extraction and focusing. An optimization of these parameters was achieved in order to provide better performances compared with existing instruments. Our design resulted in an enhancement in the ion production and transmission by a factor of approximately 100. This means that it should be possible to obtain precise measurements of isotope ratios, given that the maximum gas pressure in the Knudsen cell is 10-4 bar. Several additional improvements were also made in the design of the instrument including in the cooling system, in the oven regulation and the pumping system. In parallel, a new mechanical design of the source housing and electronics has been initiated together with a specific software for controlling the instrument.

Progress beyond the state of the art and expected potential impact (including the socio-economic impact and the wider societal implications of the project so far)

This project consists of three main subprojects: (1) we have simulated the effect of particle irradiation on solids to examine how isotopes can be fractionated by these processes to identify whether this can explain chemical variations in meteorites. We have observed that He ion irradiation could produce sizeable mass-dependent fractionation that may explain some observations in meteorites, (2) the novel KEMS instrument can be used to determine the equilibrium isotope fractionation associated with reactions between gas and condensed phases at high temperature as well as many thermodynamic and kinetic parameters associated with evaporation. This can provide new constraints on the thermodynamic conditions, T, P and fO2 during heating events that have modified the chemical composition of planetary materials, such as the formation of the Moon or dust formation in stellar outflows. These constraints can also help identify the processes that cause the depletion in volatile elements and the fractionation in refractory elements observed in planetesimals and planets, (3) We have developed several modeling techniques ranging from computational thermodynamics, molecular dynamics and ab initio calculations to examine evaporation and condensation in astrophysical and planetary environments, that go well beyond what initially planned and used these techniques for several astrophysical and geological applications.

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