ARC Centre of Excellence for Gravitational Wave Discovery. ARC Centre of Excellence for Gravitational Wave Discovery. The mission of our Centre is to use gravitational waves to investigate the fundamental nature of relativistic gravity, ultra-dense matter, and cosmology. This will generate critical discoveries that cement Australia's leadership role in the gravitational wave mega-science instruments of the 2030s and 2040s. By bringing together a world-class team with broad and complementary expe ....ARC Centre of Excellence for Gravitational Wave Discovery. ARC Centre of Excellence for Gravitational Wave Discovery. The mission of our Centre is to use gravitational waves to investigate the fundamental nature of relativistic gravity, ultra-dense matter, and cosmology. This will generate critical discoveries that cement Australia's leadership role in the gravitational wave mega-science instruments of the 2030s and 2040s. By bringing together a world-class team with broad and complementary expertise we will develop core technologies for future detectors, discover new sources of gravitational waves, probe fundamental physics, and lay the foundations for an Australian gravitational wave observatory. Our discoveries will inspire Australia's youth to pursue high tech careers and position our staff and students to become leaders in both industry and academia.Read moreRead less
Planet Formation at Solar System Scales with the James Webb Space Telescope. Planetary systems like our own form within vast disks of primordial gas and dust around newborn stars. This project will observe such disks spanning a range of ages with the James Webb Space Telescope to reveal the detailed in-situ physics of planet-forming disks themselves. We will deliver the sharpest-ever infrared images in astronomy, exploiting the only Australian-designed instrument on the spacecraft: the Aperture ....Planet Formation at Solar System Scales with the James Webb Space Telescope. Planetary systems like our own form within vast disks of primordial gas and dust around newborn stars. This project will observe such disks spanning a range of ages with the James Webb Space Telescope to reveal the detailed in-situ physics of planet-forming disks themselves. We will deliver the sharpest-ever infrared images in astronomy, exploiting the only Australian-designed instrument on the spacecraft: the Aperture Masking Interferometer. This yields new physics for actively growing protoplanets, carved rings and gaps in disks, and gravitationally sculpted patterns of leftover cometary debris. Confronting state-of-the-art models with these data will immediately yield profound insights into planetary system formation, including our own.Read moreRead less
Designing a spectrometer to search for life on extrasolar planets. Finding indicators of life on extrasolar planets is one of the greatest science questions of our time. Astronomers have found rocky, earth-like exoplanets; now we need powerful spectrometers to search for biomarkers in their atmospheres, detecting the faint imprints from molecules associated with life in the colour spectrum of stars. This project will develop the instruments and technologies required to enable spectroscopy with m ....Designing a spectrometer to search for life on extrasolar planets. Finding indicators of life on extrasolar planets is one of the greatest science questions of our time. Astronomers have found rocky, earth-like exoplanets; now we need powerful spectrometers to search for biomarkers in their atmospheres, detecting the faint imprints from molecules associated with life in the colour spectrum of stars. This project will develop the instruments and technologies required to enable spectroscopy with massively multiplexed telescopes. A spectrometer design with large spectral bandwidth and high resolution, optimised for a facility consisting of thousands of small telescopes, and novel optical fibres to link them, will open the door for breakthrough science requiring an entirely new class of telescope.Read moreRead less
Revealing the Unseen Universe with Gravitational Lensing. This project will analyse new Australian led observations from the Hubble Space Telescope of light being bent around massive galaxies by gravity. To analyse these images we must develop advanced physical models and statistical techniques. This analysis will give us highly magnified views of early galaxy evolution revealing physical details otherwise impossible to see. It will also allow us to put constraints on the nature of invisible dar ....Revealing the Unseen Universe with Gravitational Lensing. This project will analyse new Australian led observations from the Hubble Space Telescope of light being bent around massive galaxies by gravity. To analyse these images we must develop advanced physical models and statistical techniques. This analysis will give us highly magnified views of early galaxy evolution revealing physical details otherwise impossible to see. It will also allow us to put constraints on the nature of invisible dark matter with the possibility of detecting warm dark matter signatures and enable us to probe the expansion of the Universe, testing whether the unseen dark energy is evolving in time. The Hubble sample is much larger and a major advance on previous work, and enables breakthrough science in these areas.Read moreRead less
Artificial Self-Replication of Peptide Nanocapsules. Replication is key to the operation of biology, but how molecular replicators arose spontaneously on early Earth remains an open question. The ability of molecules to self-replicate must have come before the development of the highly evolved enzymes that biology currently employs. The aim of this Future Fellowship is to develop a peptide nanocapsule capable of replicating itself nonenzymatically by self-templated ligation, thus offering a plat ....Artificial Self-Replication of Peptide Nanocapsules. Replication is key to the operation of biology, but how molecular replicators arose spontaneously on early Earth remains an open question. The ability of molecules to self-replicate must have come before the development of the highly evolved enzymes that biology currently employs. The aim of this Future Fellowship is to develop a peptide nanocapsule capable of replicating itself nonenzymatically by self-templated ligation, thus offering a platform that possesses the traits needed for Darwinian evolution to emerge. By obtaining a better understanding of the design and function of self-replicating systems, this project is expected to transform our understanding of some of the key chemical principles needed for life's emergence.Read moreRead less
Australian Laureate Fellowships - Grant ID: FL220100117
Funder
Australian Research Council
Funding Amount
$2,497,216.00
Summary
How Old Are The Stars? Looking Inside Stars with Asteroseismology. Stars are the building blocks of the Universe. Understanding their structure and evolution underpins much of modern astrophysics, from characterising the growing number of extra-solar planets to unravelling the history of our Milky Way Galaxy. This research program will use the technique of asteroseismology, the study of starquakes, to probe the interiors of stars in extraordinary detail and measure their ages with unprecedented ....How Old Are The Stars? Looking Inside Stars with Asteroseismology. Stars are the building blocks of the Universe. Understanding their structure and evolution underpins much of modern astrophysics, from characterising the growing number of extra-solar planets to unravelling the history of our Milky Way Galaxy. This research program will use the technique of asteroseismology, the study of starquakes, to probe the interiors of stars in extraordinary detail and measure their ages with unprecedented precision. Having accurate ages for large numbers of stars will help us understand how the Milky Way galaxy formed and developed. We will generate a deep understanding of the processes that occur inside stars, mentor a new generation of researchers and establish Australia as a world leader in stellar astrophysics.Read moreRead less
Ensemble modelling of space-weather drivers. This project aims to develop methods for forecasting the evolution of magnetic fields on the Sun's surface, and to use the results to drive an ensemble of numerical simulations of the evolution of the magnetic field in the overlying atmosphere. The project expects to create a new framework for forecasting the evolution of solar active regions, applying, for the first time, methods established in Numerical Weather Prediction. The expected outcomes are ....Ensemble modelling of space-weather drivers. This project aims to develop methods for forecasting the evolution of magnetic fields on the Sun's surface, and to use the results to drive an ensemble of numerical simulations of the evolution of the magnetic field in the overlying atmosphere. The project expects to create a new framework for forecasting the evolution of solar active regions, applying, for the first time, methods established in Numerical Weather Prediction. The expected outcomes are physics-based prediction of solar atmospheric magnetic field evolution, including explosive eruptions. The results should have significant benefit in improving prediction of extreme space weather events, which pose an increasing threat to our technologically-dependent society.Read moreRead less
Closing the Solar Cycle. This project aims to decisively settle the debate about the mechanism driving magnetic activity on the surface of the Sun. By drawing on extensive, big-data analysis of solar observations the project intends to use the technique of helioseismology to reveal differences in the statistical evolution of magnetic regions. Expected outcomes of this project will powerfully refine our models of the interaction between convective flows and magnetic fields in the Sun, resulting i ....Closing the Solar Cycle. This project aims to decisively settle the debate about the mechanism driving magnetic activity on the surface of the Sun. By drawing on extensive, big-data analysis of solar observations the project intends to use the technique of helioseismology to reveal differences in the statistical evolution of magnetic regions. Expected outcomes of this project will powerfully refine our models of the interaction between convective flows and magnetic fields in the Sun, resulting in a leap forward in solar dynamo theory, one of the fundamental problems in astrophysics. The anticipated benefits include moving from nowcasting to forecasting space weather, mitigating the billion dollar economic effects of geomagnetic storms.Read moreRead less