From dust to planets: New initiatives to refine models of the inner Solar System's earliest history. This project will help continue the proud tradition of Australia as an international leader in mass spectrometric analyses and cosmochemistry. The questions surrounding the origin and significance of terrestrial planets are closely related to our very presence: "Are we alone"?
Research into meteorites is one of the few areas of science that truly captures the imagination of the general public. T ....From dust to planets: New initiatives to refine models of the inner Solar System's earliest history. This project will help continue the proud tradition of Australia as an international leader in mass spectrometric analyses and cosmochemistry. The questions surrounding the origin and significance of terrestrial planets are closely related to our very presence: "Are we alone"?
Research into meteorites is one of the few areas of science that truly captures the imagination of the general public. This project, through its integration with the WA Museum, gives the public a possibility to share in this experience.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE200100035
Funder
Australian Research Council
Funding Amount
$610,000.00
Summary
WA CRC-MC-ICPMS for Earth, Planetary and Environmental science. This Application aims to provide a mass spectrometer for Australian researchers collaborating on NASA, Japanese Aerospace Exploration Agency and China National Space Administration extra-terrestrial sample return missions as they characterise unique samples of dust and rock collected from asteroids, the Moon and meteorites. The Application will also support government geoscience agencies who will generate nationally significant isot ....WA CRC-MC-ICPMS for Earth, Planetary and Environmental science. This Application aims to provide a mass spectrometer for Australian researchers collaborating on NASA, Japanese Aerospace Exploration Agency and China National Space Administration extra-terrestrial sample return missions as they characterise unique samples of dust and rock collected from asteroids, the Moon and meteorites. The Application will also support government geoscience agencies who will generate nationally significant isotopic datasets to improve mineral exploration success, and scientists monitoring Earth’s environment. Expected outcomes will ensure that Australia remains at the forefront of cosmochemistry, minerals research and environmental studies, which will provide significant benefits to our economy and society.
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The fossil record of galaxy formation. This Australian-led team recently used the Anglo-Australian Telescope to discover large numbers of a new type of very small galaxy in the centres of two galaxy clusters. This project will maintain Australian leadership in this new area of astrophysics research, whilst using the best international expertise and facilities.
The formation and structure of distant galaxies. (i) The proposed galaxy evolution science involves the study of one of the most fundamental processes within the universe, thereby contributing to the Priority Goal of 'Breakthrough Science' under National Research Priority 3. (ii) It will bring national benefit through international collaborations with prestigious US, UK, and Canadian institutions. (iii) These collaborations will lead to new research capacity being built within Australia, with co ....The formation and structure of distant galaxies. (i) The proposed galaxy evolution science involves the study of one of the most fundamental processes within the universe, thereby contributing to the Priority Goal of 'Breakthrough Science' under National Research Priority 3. (ii) It will bring national benefit through international collaborations with prestigious US, UK, and Canadian institutions. (iii) These collaborations will lead to new research capacity being built within Australia, with considerable knowledge and expertise being vested in young postgraduate and postdoctoral researchers.Read moreRead less
Galaxy recycling in clusters of galaxies. Large galaxies are thought to form by merging smaller dwarf galaxies, but recent discoveries reveal a more violent picture: some dwarf galaxies are torn apart by the gravity of their companions, their contents strewn across inter-galactic space.
We will investigate how much this debris is recycled into other galaxies. We will examine Hubble Space Telescope images of dwarf galaxies to test if they are broken up to form the ultra-compact dwarf galaxies we ....Galaxy recycling in clusters of galaxies. Large galaxies are thought to form by merging smaller dwarf galaxies, but recent discoveries reveal a more violent picture: some dwarf galaxies are torn apart by the gravity of their companions, their contents strewn across inter-galactic space.
We will investigate how much this debris is recycled into other galaxies. We will examine Hubble Space Telescope images of dwarf galaxies to test if they are broken up to form the ultra-compact dwarf galaxies we recently discovered. We will model the rate at which dwarf galaxies are disrupted to determine how the dark matter is distributed in such galaxies.Read moreRead less
Uncovering the Fossil Record of Galaxy Formation. Our Australian-led team recently used the Anglo-Australian Telescope to discover large numbers of a new type of very small galaxy in the centres of two galaxy clusters. This project will allow us to maintain Australian leadership in this new area of astrophysics research, whilst using leading international facilities.
Galactic Cannibalism: The link between dwarf galaxies and globular star clusters. The formation of bright globular star clusters in giant galaxies like our own Milky Way remains an unsolved problem in astrophysics. Galactic cannibalism is the theory that they formed by the disruption of dwarf galaxies that came too close to the gravitational field of giant galaxies. We will use the new Gemini Telescopes to test this theory with sensitive comparisons of the properties of globular clusters, dwarf ....Galactic Cannibalism: The link between dwarf galaxies and globular star clusters. The formation of bright globular star clusters in giant galaxies like our own Milky Way remains an unsolved problem in astrophysics. Galactic cannibalism is the theory that they formed by the disruption of dwarf galaxies that came too close to the gravitational field of giant galaxies. We will use the new Gemini Telescopes to test this theory with sensitive comparisons of the properties of globular clusters, dwarf galaxies and our newly-discovered ultra-compact dwarf galaxies which may be the missing link in this process.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0882778
Funder
Australian Research Council
Funding Amount
$201,224.00
Summary
Water vapour radiometers for millimetre-wave phase correction for the Australia Telescope. Australia has a tradition of excellence in astronomy. Inspired by wonder about the cosmos, it stimulates public interest in science, so leading to the training of highly skilled graduates. In turn, this drives the development of technologies needed to pursue the science. The nation has invested in the technology for millimetre-wave astronomy, building the first interferometer in our hemisphere. This equipm ....Water vapour radiometers for millimetre-wave phase correction for the Australia Telescope. Australia has a tradition of excellence in astronomy. Inspired by wonder about the cosmos, it stimulates public interest in science, so leading to the training of highly skilled graduates. In turn, this drives the development of technologies needed to pursue the science. The nation has invested in the technology for millimetre-wave astronomy, building the first interferometer in our hemisphere. This equipment will capitalise on this investment, extending the capabilities of the Australia Telescope to maintain it as a front line instrument, attracting the best scientists here to use it. This will help nurture a vigorous radio-science community, one able to actively participate in the billion-dollar investment being made internationally in the field.Read moreRead less
How typical is our Local Galaxy Group? This project will uncover how unusual the Local Group is by comparing the Milky Way and Andromeda Galaxy (known as M31) halos to similar mass systems in the local Universe. By using well understood galaxy groups created as part of the Galaxy And Mass Assembly project (GAMA), the study will be able to uncover the mass distribution of galaxies found in different mass groups. It will go further than any previous work by combining these robust groups with faint ....How typical is our Local Galaxy Group? This project will uncover how unusual the Local Group is by comparing the Milky Way and Andromeda Galaxy (known as M31) halos to similar mass systems in the local Universe. By using well understood galaxy groups created as part of the Galaxy And Mass Assembly project (GAMA), the study will be able to uncover the mass distribution of galaxies found in different mass groups. It will go further than any previous work by combining these robust groups with fainter imaging data. The combination of both datasets will allow the determination of whether the Local Group is typical or unusual. Putting the Local Group into a cosmological context is vital since many future Galactic archaeology surveys assume that it is typical, and can meaningfully inform us about the wider universe.Read moreRead less
Utilising artificial intelligence to elucidate the physics of galaxies. For decades astronomers have puzzled over the connection between the structure and evolution of galaxies and the role played by host environments. This project aims to resolve this problem by combining multi-wavelength observations, multi-component simulations, and pioneering data analysis using artificial intelligence. In particular, we target the nearby Fornax galaxy cluster as a laboratory for studying galaxy formation in ....Utilising artificial intelligence to elucidate the physics of galaxies. For decades astronomers have puzzled over the connection between the structure and evolution of galaxies and the role played by host environments. This project aims to resolve this problem by combining multi-wavelength observations, multi-component simulations, and pioneering data analysis using artificial intelligence. In particular, we target the nearby Fornax galaxy cluster as a laboratory for studying galaxy formation in dense environments. Using our novel machine learning techniques, we will elucidate the physical mechanisms that drive the rapid evolution of star formation, galactic nuclei, and gas and dust content within Fornax. Our predictions will benefit ongoing and future surveys at the national and international level. Read moreRead less