Sources and processes in the early solar system - an isotopic study. Our solar system formed over 4.5 billion years ago. We aim to develop techniques that will allow us to determine the sequence of events that led to our planetary system with unprecedented detail. The same techniques can be applied to dating geological events, for example, correlating ore-forming events and dating opal formation. This project utilizes new Australian technologies that will have potential economic benefits both ....Sources and processes in the early solar system - an isotopic study. Our solar system formed over 4.5 billion years ago. We aim to develop techniques that will allow us to determine the sequence of events that led to our planetary system with unprecedented detail. The same techniques can be applied to dating geological events, for example, correlating ore-forming events and dating opal formation. This project utilizes new Australian technologies that will have potential economic benefits both in instrument sales and applications.Read moreRead less
Deciphering the early Solar System chronology and planetary chemistry using isotope systematics of meteoritic zircon. This project addresses the early evolution of our Solar System that is one of the most important questions in Earth and Planetary sciences. It will use Australia's meteorites and innovative analytical techniques developed in Australia. High impact scientific results produced in this project will be to the national benefit in terms of international recognition of our unique capabi ....Deciphering the early Solar System chronology and planetary chemistry using isotope systematics of meteoritic zircon. This project addresses the early evolution of our Solar System that is one of the most important questions in Earth and Planetary sciences. It will use Australia's meteorites and innovative analytical techniques developed in Australia. High impact scientific results produced in this project will be to the national benefit in terms of international recognition of our unique capability in this high profile and competitive research field. Furthermore, by providing new constraints on the initial state of geochemical evolution of the terrestrial planets, this work will further our knowledge of the subsequent evolution of the Earth's mantle and crust, leading to better models for Australian continent development and its deep-Earth resources.Read moreRead less