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Structure and Evolution of High Brightness Temperature Cores of Quasars and Galaxies. Interstellar scintillation, ISS, is a revolutionary new and powerful technique which we will use to study the highest brightness temperature cores of radio quasars with unprecedented angular resolution, and probe the interstellar medium of our Galaxy in a way not previously possible. The combination of scintillation and conventional VLBI allows imaging with light-month to light-year resolution across the known ....Structure and Evolution of High Brightness Temperature Cores of Quasars and Galaxies. Interstellar scintillation, ISS, is a revolutionary new and powerful technique which we will use to study the highest brightness temperature cores of radio quasars with unprecedented angular resolution, and probe the interstellar medium of our Galaxy in a way not previously possible. The combination of scintillation and conventional VLBI allows imaging with light-month to light-year resolution across the known Universe. Scintillation observations are challenging basic synchrotron physics by uncovering quasar cores with temperatures possibly as high as 10^15 K, and lifetimes many times longer than theory. The Ceduna and Hobart telescopes are cornerstones of our scintillation and VLBI proposals.
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Early Evolution of the Solar System: A Planetary Perspective. A geochemical study of early solar system materials will be conducted to investigate physical conditions leading to assembly of the terrestrial planets, and the chronology of early geological events that shaped the Earth and Moon. Objects from the solar nebula and samples from the Earth, Moon, Mars, and differentiated asteroids will be studied. This research will contribute toward understanding the astrophysical environment of the inn ....Early Evolution of the Solar System: A Planetary Perspective. A geochemical study of early solar system materials will be conducted to investigate physical conditions leading to assembly of the terrestrial planets, and the chronology of early geological events that shaped the Earth and Moon. Objects from the solar nebula and samples from the Earth, Moon, Mars, and differentiated asteroids will be studied. This research will contribute toward understanding the astrophysical environment of the inner solar system, establish a high-resolution absolute timescale for early geological events, and Identify the population of solid bodies present during the initial stages of planetary development.Read moreRead less
Lithic Astronomy: The age and origin of the elements and their incorporation in the solar nebula. All heavy elements are produced in stars. The signature of nucleosynthesis is the isotopic composition of the elements and thus measurement of isotopic compositions allows nuclear astrophysics to be elucidated in the laboratory. This project will examine the linkages between stellar sites and the material in our solar system through measurement of interstellar grains and other primitive material ob ....Lithic Astronomy: The age and origin of the elements and their incorporation in the solar nebula. All heavy elements are produced in stars. The signature of nucleosynthesis is the isotopic composition of the elements and thus measurement of isotopic compositions allows nuclear astrophysics to be elucidated in the laboratory. This project will examine the linkages between stellar sites and the material in our solar system through measurement of interstellar grains and other primitive material obtained from meteorites. A chronology of processes affecting the solar nebula will be determined through measurement of radionuclides. Th/U measurements in presolar grains could allow a view of galactic chemical evolution billions of years prior to the solar nebula.Read moreRead less
Studies of the Highest Energy Particles in Nature. One of the greatest mysteries of modern astrophysics is the origin of the highest energy cosmic rays. While rare, these subatomic particles possess enormous energies, some 100 million times larger than we can impart to a proton in man-made accelerators. Theory struggles to identify cosmic ray acceleration mechanisms, but these particles do exist. This project will fund our participation in the world's largest cosmic ray observatories, and ou ....Studies of the Highest Energy Particles in Nature. One of the greatest mysteries of modern astrophysics is the origin of the highest energy cosmic rays. While rare, these subatomic particles possess enormous energies, some 100 million times larger than we can impart to a proton in man-made accelerators. Theory struggles to identify cosmic ray acceleration mechanisms, but these particles do exist. This project will fund our participation in the world's largest cosmic ray observatories, and our aim is to use the characteristics of the incoming particles (mass, energy and arrival directions) to determine the likely sources of the most energetic particles known in Nature.Read moreRead less
High power optical systems for advanced interferometry - an ACIGA project. Direct detection of gravitational waves will open a whole new window on the Universe for mankind and is the most significant quest in modern Physics. We aim to continue as partners in this effort through our major contributions to an increase of detector sensitivity. We will develop and test critical new concepts and components, including high power ultra stable lasers, new methods for optical wavefront sensing and correc ....High power optical systems for advanced interferometry - an ACIGA project. Direct detection of gravitational waves will open a whole new window on the Universe for mankind and is the most significant quest in modern Physics. We aim to continue as partners in this effort through our major contributions to an increase of detector sensitivity. We will develop and test critical new concepts and components, including high power ultra stable lasers, new methods for optical wavefront sensing and correction, and new reflective and diffractive components for high power optical interferometers. This research will greatly enhance Australian scientific standing, strengthen scientific collaboration internationally and within Australia, and contribute to education in photonics.Read moreRead less
Probing the Universe with gravitational waves: from cutting-edge technology to astronomy. The direct detection of Einstein's elusive gravitational waves will not only confirm one of the most important theories in physics, it will unleash a new form of radiation (in addition to electromagnetic) with which to study the Universe. Our participation in this quest continues Australia's role in the vanguard of new astronomy and its exploitation. This proposal will produce scientists highly trained in ....Probing the Universe with gravitational waves: from cutting-edge technology to astronomy. The direct detection of Einstein's elusive gravitational waves will not only confirm one of the most important theories in physics, it will unleash a new form of radiation (in addition to electromagnetic) with which to study the Universe. Our participation in this quest continues Australia's role in the vanguard of new astronomy and its exploitation. This proposal will produce scientists highly trained in areas of national priority, including frontier technologies such as photonics and smart information use through GRID computing. Developing ways to build instruments of almost unimaginable sensitivity fosters innovation leading to spin-offs into other areas of optical sensing - fundamental research resulting in economic benefit.Read moreRead less
Pushing the frontiers of gravitational wave science: from technology to astrophysics. The direct detection of Einstein's elusive gravitational waves will not only confirm one of the most important theories in physics, it will unleash a new form of radiation (in addition to electromagnetic) with which to study the Universe. Our participation in this quest continues Australia's role in the vanguard of new astronomy and its exploitation. This proposal will produce scientists highly trained in ar ....Pushing the frontiers of gravitational wave science: from technology to astrophysics. The direct detection of Einstein's elusive gravitational waves will not only confirm one of the most important theories in physics, it will unleash a new form of radiation (in addition to electromagnetic) with which to study the Universe. Our participation in this quest continues Australia's role in the vanguard of new astronomy and its exploitation. This proposal will produce scientists highly trained in areas of national priority, including frontier technologies such as photonics and smart information use through GRID computing. Developing ways to build instruments of almost unimaginable sensitivity fosters innovation leading to spin-offs into other areas of optical sensing - fundamental research resulting in economic benefit.Read moreRead less
Photochemistry of the Middle Atmospheres of Venus and the Earth. Ongoing changes in the Earth's atmosphere, such as ozone depletion, demonstrate the need to understand the processes that control atmospheric chemistry. The proposed research will improve the fidelity of photochemical models, provide additional insight into the recent evolution of the Venus atmosphere, and examine how atmospheric chemistry and climate change interact(ed) on Venus. This research will improve our understanding of l ....Photochemistry of the Middle Atmospheres of Venus and the Earth. Ongoing changes in the Earth's atmosphere, such as ozone depletion, demonstrate the need to understand the processes that control atmospheric chemistry. The proposed research will improve the fidelity of photochemical models, provide additional insight into the recent evolution of the Venus atmosphere, and examine how atmospheric chemistry and climate change interact(ed) on Venus. This research will improve our understanding of long-standing issues, such as how much water might have been present on Venus in the recent past. The research program will provide an opportunity for Australian science to participate in at least one spacecraft mission to Venus. Read moreRead less
Will Antarctic telescopes detect the first new habitable planets? Within the next fifteen years the first habitable-zone planets will almost certainly have been detected around other stars. If, as we believe, Antarctic observatories play a leading role in this emerging field, Australia's astronomers will be exceptionally well placed to lead and to partner major international programs. This will bring Australian industry increased access to cutting edge technology, and create business opportuni ....Will Antarctic telescopes detect the first new habitable planets? Within the next fifteen years the first habitable-zone planets will almost certainly have been detected around other stars. If, as we believe, Antarctic observatories play a leading role in this emerging field, Australia's astronomers will be exceptionally well placed to lead and to partner major international programs. This will bring Australian industry increased access to cutting edge technology, and create business opportunities in the infrastructure and support of Antarctic research. This project aims to ensure that the lead Australia currently holds in Antarctic astronomy is maintained, allowing us to fully capture the benefits of future international investment.Read moreRead less
Do black holes exist? This project aims to verify if black holes can actually exist in our Universe. It is still unknown if any of the candidate objects possess the key black hole feature -- a trapped region from which no signal can escape. By focusing on conditions for existence of trapped regions, this project expects to describe their neighborhoods and observable properties. This information is critical for interpretation of the data from the next generation of gravitational wave detectors an ....Do black holes exist? This project aims to verify if black holes can actually exist in our Universe. It is still unknown if any of the candidate objects possess the key black hole feature -- a trapped region from which no signal can escape. By focusing on conditions for existence of trapped regions, this project expects to describe their neighborhoods and observable properties. This information is critical for interpretation of the data from the next generation of gravitational wave detectors and radio telescopes, and for determining the true nature of astrophysical black hole candidates. Further benefits include simplification of calculations of the observable properties of compact objects and resolution of a long-standing black hole information loss paradox.Read moreRead less