Linkage Infrastructure, Equipment And Facilities - Grant ID: LE210100044
Funder
Australian Research Council
Funding Amount
$905,654.00
Summary
Ultra-precise dating in Earth, planetary and archaeological science. An advanced facility incorporating next generation, multi-collector mass spectrometer and ultra-clean gas line systems, capable of ultra-precise dating of Earth, planetary and archaeological material. This joint Melbourne-Curtin facility seeks to generate ultra-precise age data from ever smaller and younger samples, such as minute particles from space return missions and tiny inclusions in diamonds. The facility is expected to ....Ultra-precise dating in Earth, planetary and archaeological science. An advanced facility incorporating next generation, multi-collector mass spectrometer and ultra-clean gas line systems, capable of ultra-precise dating of Earth, planetary and archaeological material. This joint Melbourne-Curtin facility seeks to generate ultra-precise age data from ever smaller and younger samples, such as minute particles from space return missions and tiny inclusions in diamonds. The facility is expected to revolutionise noble gas dating techniques, resulting in new knowledge on solar system genesis, hominid evolution, indigenous migrations, palaeo-climate change, natural hazards and ore deposit formation, while further enhancing Australia’s international leadership and competitive advantage in the discipline.
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The history of accretion in our Solar System. This project aims to determine precise timing of formation and primary melting of asteroids of various compositions, and to trace the stellar sources and mixing processes that caused the compositional diversity of asteroids and planets in our Solar System. This can be attained by comprehensive study of achondrites, meteorites derived from asteroids that were once partially melted. Using the world’s foremost facilities for cosmochemical research in Au ....The history of accretion in our Solar System. This project aims to determine precise timing of formation and primary melting of asteroids of various compositions, and to trace the stellar sources and mixing processes that caused the compositional diversity of asteroids and planets in our Solar System. This can be attained by comprehensive study of achondrites, meteorites derived from asteroids that were once partially melted. Using the world’s foremost facilities for cosmochemical research in Australia and the United States of America, the processes leading to the formation of planets will be explored. This project is intended to advance fundamental knowledge of the environment in which planets emerge and evolve, and the place of our Solar System among planetary systems in the Galaxy.Read moreRead less
Analysis of asteroid samples returned by Hayabusa 2 and Osiris-REx . This year sees the highly anticipated return of the Hayabusa2 spacecraft to Woomera carrying samples of the asteroid Ryugu. This is only the fifth extraterrestrial sample return mission in history. The research team has been invited to participate in the preliminary examination which will take place in Japan in early 2021. The investigators have developed unique analytical skills that allow measurement of small amounts of rock ....Analysis of asteroid samples returned by Hayabusa 2 and Osiris-REx . This year sees the highly anticipated return of the Hayabusa2 spacecraft to Woomera carrying samples of the asteroid Ryugu. This is only the fifth extraterrestrial sample return mission in history. The research team has been invited to participate in the preliminary examination which will take place in Japan in early 2021. The investigators have developed unique analytical skills that allow measurement of small amounts of rock for oxygen isotope compositions at unprecedented precision. This project aims to characterise a suite of carbonaceous chondrites, which appear to be the best match to Ryugu, and therefore will provide the exemplar data to understand the provenance of Ryugu, and place it in the context of solar system materials.
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Linkage Infrastructure, Equipment And Facilities - Grant ID: LE100100064
Funder
Australian Research Council
Funding Amount
$450,000.00
Summary
A facility for sensitive and precise isotopic dating of the earth's and extraterrestrial rocks. SPIDE2R will be a new generation mass spectrometer for very precise and sensitive dating and forensics applications in earth and planetary sciences, hydrology, climate studies, and nuclear and archaeological fingerprinting. The unprecedented sensitivity of this unique instrument will provide enhanced capabilities for solving long-standing problems requiring precise geological time resolution, as well ....A facility for sensitive and precise isotopic dating of the earth's and extraterrestrial rocks. SPIDE2R will be a new generation mass spectrometer for very precise and sensitive dating and forensics applications in earth and planetary sciences, hydrology, climate studies, and nuclear and archaeological fingerprinting. The unprecedented sensitivity of this unique instrument will provide enhanced capabilities for solving long-standing problems requiring precise geological time resolution, as well as opening new areas of research. It will be the instrument of choice for analysing small, rare samples such as those returned by space missions. The Australian-built high sensitivity source and ion detection systems can be retrofitted onto other mass spectrometers, opening a new area of commercialisation.Read moreRead less
Consequences of extraterrestrial impacts on the biosphere and geosphere. This project will investigate whether high-velocity meteorite impacts can account for the Earth's mass extinctions and whether meteorite impacts and mass extinctions were synchronous. This work will help scientists understand the long-term climatic and biologic effects of massive injections of greenhouse gases into the atmosphere.
Precise cross-calibration of 40Ar/39Ar, Rb-Sr and U-Pb chronometers: towards an integrated geochronology toolbox. Application of the 40Ar/39Ar isotopic geochronometer to dating rocks, minerals, fossils and meteorites is limited by insufficient precision and consistency in existing determinations of the half-life of its parent isotope 40K. This project proposes novel methods for determination of the half-life and branching ratio of 40K, by age comparison against well calibrated 87Rb-87Sr and 40K- ....Precise cross-calibration of 40Ar/39Ar, Rb-Sr and U-Pb chronometers: towards an integrated geochronology toolbox. Application of the 40Ar/39Ar isotopic geochronometer to dating rocks, minerals, fossils and meteorites is limited by insufficient precision and consistency in existing determinations of the half-life of its parent isotope 40K. This project proposes novel methods for determination of the half-life and branching ratio of 40K, by age comparison against well calibrated 87Rb-87Sr and 40K-40Ca geochronometers. The ages with all isotopic systems will be determined in the same minerals, thus eliminating the main source of uncertainty in the previous studies. Independently The project will measure the 40K decay rate by decay counting of highly enriched 40K salt and expects a five-fold improvement in precision and accuracy of known 40K decay rate.Read moreRead less
High resolution timeframe for hominin evolution in the Turkana Basin, Kenya. This project aims to establish a high-resolution timeframe for hominin evolution in the famed Omo-Turkana Basin, Kenya. The Basin hosts a vast array of hominin fossils that cover more than four million years of human evolution, and interbedded volcanic deposits within the Basin sediments has provided much of our current constraints on the timing of hominin evolution. However critical knowledge gaps remain. Using new ins ....High resolution timeframe for hominin evolution in the Turkana Basin, Kenya. This project aims to establish a high-resolution timeframe for hominin evolution in the famed Omo-Turkana Basin, Kenya. The Basin hosts a vast array of hominin fossils that cover more than four million years of human evolution, and interbedded volcanic deposits within the Basin sediments has provided much of our current constraints on the timing of hominin evolution. However critical knowledge gaps remain. Using new instrumentation and dating methods, this project will provide an ultra-precise chronological framework for the basin. This is critical for transforming our understanding of hominin evolution and migration, under changing climatic and environmental conditions.Read moreRead less
Investigation of the early history of the moon. The project will address outstanding questions related to the early evolution of planets in the solar system, including the earth, by investigating major events that took place on the moon, where the record of early history is preserved exceptionally well. It will test major models describing the chemical evolution of both the moon and earth.
A detrital apatite archive to track crustal growth. This project will establish apatite as a new tool to study the evolution of the continental crust. The crust shaped the composition of the atmosphere and the oceans with consequences for the evolution of life through the availability of oxygen and nutrients. However, when and how the continental crust was generated remains a core question. Current models for continental crust development rely on the mineral zircon. However, zircons only record ....A detrital apatite archive to track crustal growth. This project will establish apatite as a new tool to study the evolution of the continental crust. The crust shaped the composition of the atmosphere and the oceans with consequences for the evolution of life through the availability of oxygen and nutrients. However, when and how the continental crust was generated remains a core question. Current models for continental crust development rely on the mineral zircon. However, zircons only record the history of evolved rocks. To address this bias we will use the mineral apatite which forms in less evolved rocks. We will develop a detrital apatite database of Pb-Nd (model) ages and integrate this with the zircon record to provide a more holistic description for how our planet developed.Read moreRead less
Carbon dioxide sequestration more than 3.7 billion years ago and the oldest climate cycles. More than 3.7 billion years ago atmospheric greenhouse CO2 was sequestered into limestone sedimentary rocks deposited in ice-free oceans. Why then, with the 30-25 per cent cooler sun in those times, was our earth not frozen over? Solving this oldest climate problem, will give the deepest-time perspective to the earth's changing climate feedback loops.