Linkage Infrastructure, Equipment And Facilities - Grant ID: LE200100012
Funder
Australian Research Council
Funding Amount
$632,000.00
Summary
Exploring the Dynamic Universe with DREAMS. DREAMS is a revolutionary wide-field infrared surveyor designed to allow astronomers to unlock new science and foster international collaborations focused on important but elusive, infrared transient cosmic phenomena. Continually scanning the southern sky, DREAMS will provide “real time” data that will transform the depth and quality of astronomical observation. Combining off-the-shelf parts with scientific expertise from around the world, this telesco ....Exploring the Dynamic Universe with DREAMS. DREAMS is a revolutionary wide-field infrared surveyor designed to allow astronomers to unlock new science and foster international collaborations focused on important but elusive, infrared transient cosmic phenomena. Continually scanning the southern sky, DREAMS will provide “real time” data that will transform the depth and quality of astronomical observation. Combining off-the-shelf parts with scientific expertise from around the world, this telescope will help answer questions that are both practical and profound. DREAMS is an important component of a longer-term international strategy that will reinforce Australia’s global leadership in the realm of Infrared Transient Astronomy.Read moreRead less
Supernovae as the origin of antimatter in our galaxy. This project aims to uncover the origin of the bulk of the antimatter in our Milky Way Galaxy. Astrophysicists have known for forty years that our Galaxy glows with gamma-rays emitted by the annihilation of huge numbers of positrons, the antimatter partners to electrons. Certain supernovae are the likely source of these positrons. To fully investigate this idea and its ramifications, this project will perform three-dimensional supercomputer s ....Supernovae as the origin of antimatter in our galaxy. This project aims to uncover the origin of the bulk of the antimatter in our Milky Way Galaxy. Astrophysicists have known for forty years that our Galaxy glows with gamma-rays emitted by the annihilation of huge numbers of positrons, the antimatter partners to electrons. Certain supernovae are the likely source of these positrons. To fully investigate this idea and its ramifications, this project will perform three-dimensional supercomputer simulations of thermonuclear supernova explosions. This project aspires to resolve a long-standing mystery in astrophysics and provide an exemplar for best usage of Australian investment in astronomy and supercomputing infrastructure.Read moreRead less
Precision pair spectroscopy of the Hoyle state. This project aims to develop a novel new spectrometer to observe and characterise electron-positron pairs of high energy nuclear transitions with unprecedented precision. Building on unique Australian expertise and equipment, the outcomes will include new applications of electron spectroscopy to nuclear structure studies, and a better understanding of element synthesis in the universe, including the formation of 12C in the universe.
Understanding other worlds: the composition, structure and evolution of exoplanet atmospheres. This project will advance our understanding of the rapidly growing number of planets being found around other stars. The project will develop new techniques to determine what their atmospheres are made of, how the planets form and evolve, and whether they have the potential to host life.
Adolescent stars and planets in our neighbourhood from Gaia and FunnelWeb. This project aims to understand how infant stars in their stellar nurseries reach adulthood in the Galactic disk, and link stellar birth to the presence and evolution of adolescent planetary systems. The billion dollar Gaia satellite will change the study of stellar adolescence, with data beginning to flow with an initial public release this year. FunnelWeb – the largest star survey of its kind, covering the entire Southe ....Adolescent stars and planets in our neighbourhood from Gaia and FunnelWeb. This project aims to understand how infant stars in their stellar nurseries reach adulthood in the Galactic disk, and link stellar birth to the presence and evolution of adolescent planetary systems. The billion dollar Gaia satellite will change the study of stellar adolescence, with data beginning to flow with an initial public release this year. FunnelWeb – the largest star survey of its kind, covering the entire Southern sky – will augment this data. This project will combine these datasets, identifying the birthplace of the majority of nearby adolescent stars in the Southern sky and helping to discover and characterise their planetary systems. The results relating to the origin and Galactic context of our solar system are of broad public interest.Read moreRead less
Characterization of extrasolar planets using high-precision polarimetry. Close to a thousand exoplanets have been found since the discovery of a planet around a Sun-like star, 51 Peg in 1995. With the Kepler space telescope, we are now capable of finding Earth-size worlds around other stars. But how do we know if these Earth-like planets have all the right ingredients for life like ours to flourish? Polarimetry is a powerful method of exoplanet characterisation that could one day answer such que ....Characterization of extrasolar planets using high-precision polarimetry. Close to a thousand exoplanets have been found since the discovery of a planet around a Sun-like star, 51 Peg in 1995. With the Kepler space telescope, we are now capable of finding Earth-size worlds around other stars. But how do we know if these Earth-like planets have all the right ingredients for life like ours to flourish? Polarimetry is a powerful method of exoplanet characterisation that could one day answer such questions and can be applied, right now, to the giant planets. An innovative, portable polarimeter will be developed, that will be used to understand the atmospheric composition of exoplanets. Polarimetry is a promising method, which in the future may be the first method that can detect liquid water on extrasolar planets.Read moreRead less
The Gaia/Kepler revolution for asteroseismology and exoplanets. This project aims to combine the first results from the Gaia mission with Kepler data to improve understanding of stars and planets. The study of the structure and evolution of stars and planets in our galaxy is one of the most rapidly growing fields in astronomy. While the NASA Kepler Mission has discovered thousands of exoplanets and oscillating stars, poor knowledge of their distances has been a limitation in exploiting the data. ....The Gaia/Kepler revolution for asteroseismology and exoplanets. This project aims to combine the first results from the Gaia mission with Kepler data to improve understanding of stars and planets. The study of the structure and evolution of stars and planets in our galaxy is one of the most rapidly growing fields in astronomy. While the NASA Kepler Mission has discovered thousands of exoplanets and oscillating stars, poor knowledge of their distances has been a limitation in exploiting the data. The project is expected to yield an empirical calibration of asteroseismology, and lead to breakthrough discoveries in understanding masses and interior rotation in intermediate mass stars to accurately estimate the frequency of Earth-like planets in our galaxy.Read moreRead less
Stellar chemical signatures of planet formation. Through demanding observations with the largest telescopes and extremely accurate analyses, the project will search for the characteristic fingerprints of planet formation imprinted in the chemical compositions of the sun and stars that we have discovered. The work will shed light on the origin of the solar system and identify stars harbouring planets.
Australian Laureate Fellowships - Grant ID: FL110100074
Funder
Australian Research Council
Funding Amount
$2,627,006.00
Summary
Meteorite fireballs - illuminating the origins of the solar system. Meteorites are ancient rocks, containing a record of what conditions were like when the solar system was young; but to understand that record we need to know where they come from. This project will deliver these data, providing us with a template to understand how our planetary system came into being.
ARC Centre of Excellence for All-sky Astrophysics. The ARC Centre of Excellence for All-sky Astrophysics (CAASTRO) will establish Australia as a world-leader in the emerging discipline of wide-field astronomy. CAASTRO will answer fundamental questions about the nature of the Universe, develop innovative ways of processing enormous data-sets, and enable a diverse set of opportunities for students and early career researchers. By bringing Australia's top astronomers together into a focused collabo ....ARC Centre of Excellence for All-sky Astrophysics. The ARC Centre of Excellence for All-sky Astrophysics (CAASTRO) will establish Australia as a world-leader in the emerging discipline of wide-field astronomy. CAASTRO will answer fundamental questions about the nature of the Universe, develop innovative ways of processing enormous data-sets, and enable a diverse set of opportunities for students and early career researchers. By bringing Australia's top astronomers together into a focused collaboration, CAASTRO will cement Australia's reputation as an international leader in astrophysical research, will build unique expertise in wide-field radio and optical astronomy and will position Australia to lead the science programmes planned for the Square Kilometre Array.Read moreRead less