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Characterising satellites using un-resolved optical observations . Space situational awareness is a critical priority for Australian national security and the commercial space sector as the economy is investing in space. Space debris is a growing international threat to all major economies that rely on space for communications and defence. This project will understand how defunct satellites degrade over time to produce space debris. To accomplish this the project will collaborate with the Polish ....Characterising satellites using un-resolved optical observations . Space situational awareness is a critical priority for Australian national security and the commercial space sector as the economy is investing in space. Space debris is a growing international threat to all major economies that rely on space for communications and defence. This project will understand how defunct satellites degrade over time to produce space debris. To accomplish this the project will collaborate with the Polish Space Agency to employ low resolution spectroscopy to measure the surface degradation of geostationary satellites. Read moreRead less
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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Linkage Infrastructure, Equipment And Facilities - Grant ID: LE100100111
Funder
Australian Research Council
Funding Amount
$150,000.00
Summary
A database for Australian optical astronomy. We will build an astronomy data facility to provide database facilities to analyse data from three major Australian optical astronomy projects, SkyMapper, WiggleZ and GAMA. The facility will provide efficient analysis tools not only for the researchers immediately involved with the projects, but, for the entire national and international astronomical community when the data become public. Long-term maintenance of the facility is vital, so the facilit ....A database for Australian optical astronomy. We will build an astronomy data facility to provide database facilities to analyse data from three major Australian optical astronomy projects, SkyMapper, WiggleZ and GAMA. The facility will provide efficient analysis tools not only for the researchers immediately involved with the projects, but, for the entire national and international astronomical community when the data become public. Long-term maintenance of the facility is vital, so the facility will be standards-compliant and stable to facilitate long-term support. For this reason the facility will be based at the ANU Supercomputer Facility (ANUSF) to leverage substantial expertise in this area and to provide long-term operations support.Read moreRead less
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
Innovative solutions to enhance space situational awareness. This project seeks to significantly advance Australia's space situational awareness by researching advanced orbit prediction techniques. The development of novel space object orbit prediction techniques will greatly improve collision warnings for satellite operators that provide essential space-based services to Australian Government and industries.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE160100031
Funder
Australian Research Council
Funding Amount
$1,000,000.00
Summary
Expanding our view of the Universe with the Murchison Widefield Array. Expanding our view of the Universe with the Murchison Widefield Array:
This project aims to build a Phase 2 Murchison Widefield Array (MWA) to boost the capabilities of the Phase 1 MWA by an order of magnitude. The Epoch of Reionisation (EoR), when the first stars and galaxies lit up the universe, is the last unstudied phase of cosmic evolution. The MWA is at the frontier of EoR research and all-sky survey astrophysics, is t ....Expanding our view of the Universe with the Murchison Widefield Array. Expanding our view of the Universe with the Murchison Widefield Array:
This project aims to build a Phase 2 Murchison Widefield Array (MWA) to boost the capabilities of the Phase 1 MWA by an order of magnitude. The Epoch of Reionisation (EoR), when the first stars and galaxies lit up the universe, is the last unstudied phase of cosmic evolution. The MWA is at the frontier of EoR research and all-sky survey astrophysics, is the only low frequency precursor for the Square Kilometre Array (SKA), and is the only SKA precursor delivering science quality data. This project to construct a Phase 2 MWA would double the number of antennas in the array, double the maximum baseline length, and boost our all-sky survey and EoR capabilities. 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