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‘Game-changing' NSW medical accelerator to break ground in Sydney's inner-west

‘Game-changing' NSW medical accelerator to break ground in Sydney's inner-west

West Australian20-05-2025

A world-class biomedical accelerator which will house more than 1200 researchers and clinician scientists will break ground in Sydney's inner-west.
The $780m Sydney Biomedical Accelerator in Camperdown will break ground on Wednesday morning, three years ahead of its planned opening in 2028.
The facility will span the University of Sydney and Royal Prince Alfred Hospital, and will bring together biology and medicine disciplines to 'fast-track' scientific discovery.
Health Minister Ryan Park said the research and education complex would 'change the game' when it came to research into medical diagnostics and treatments in Australia.
'Benchmarked against the world's leading biomedical facilities, the Accelerator is set to change the landscape of medical research and I hope it becomes a major drawcard for world class health researchers.
'Cutting-edge laboratories will empower researchers to accelerate the discovery of cures and treatments for a wide range of diseases, driving medical breakthroughs with greater speed and precision.'
Australian-owned Richard Crookes Constructions will build the facility, which will include two new biomedical research buildings over eight level and a bridge connecting the university with the hospital.
Connecting the two will enable 'seamless exchange of knowledge from lab to bedside', including clinical trials, and would help turn discoveries into patient outcomes.
'We know that for NSW to be a world leader in medical research we need to continue to foster collaboration across government, health, industry and academia,' Medical Health Minister David Harris said.
'By bringing together scientists, clinicians and innovators under one roof, we're laying the foundation for discoveries that will shape the future of healthcare in this country and across the globe.'
University of Sydney Vice-Chancellor and President, Professor Mark Scott AO described the Sydney Biomedical Accelerator as 'a bold step forward in Australia's research and development landscape'.
'What makes it unique is its integration of world-class research with innovation, commercial translation, and real-world clinical outcomes,' he said.
'It will be a place for discovery – but also one where ideas transform into impact, accelerating solutions from the lab bench to the bedside and beyond.'
The Accelerator will include laboratory and collaboration spaces for researchers clinicians and the industry, including an innovation and start-up hub.
It will also feature a hi-tech biobank – a storage facility for tissue samples, cells, blood, and DNA – high-performing computing, precision medicine, surgery and anatomy research and teaching, core research facilities for microscopy, preclinical imaging, drug discovery, protein production and purification, and spaces for clinical trials.

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Aussie astronomer tests theories of planet formation

In a leap forward in the search for life beyond Earth, an Australian astronomer has detected an unusual mix of gases in the atmosphere of a planet 850 light years away. The discovery, an international effort led by University of Newcastle's Dr Tom Evans-Soma, offers insight into how planets form and whether they could once have supported existence. Published in Nature Astronomy, the research focuses on WASP-121b, or "Tylos" - an ultra-hot gas giant similar to Jupiter but with surface temperatures exceeding 2500C. Using NASA's $A15 billion James Webb Space Telescope, the team observed the Tylos - called an exoplanet as it is beyond our solar system - continuously over 40 hours, capturing more than 3500 exposures. Examining the results pixel-by-pixel, Dr Evans-Soma was able to "essentially take a chemical inventory of the atmosphere" to establish the key chemical "building blocks" of the planet, and the results were striking. 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"The silicon enrichment of the atmosphere suggests Tylos incorporated a huge amount of rocky material as it formed - a quantity equivalent to about 30 times the mass of Earth ... (which was) likely delivered by asteroid-like bodies colliding with the planet and becoming engulfed in the atmosphere," he said. This rocky material, vaporised by intense heat, released gases such as silicon monoxide into the planet's atmosphere. It changes astronomers' understanding of how these gasses circulate in the atmosphere and therefore how planets form, he said. "It's opened up potentially a new window that people may not have been thinking about," he said. "And that is a really valuable ingredient when it comes to linking the observations to our theories of planet formation." Though Tylos is far too hot to support life as we know it, the research contributes to a growing body of knowledge that could one day identify life beyond our solar system. "Of course, one day we hope to answer the age-old question of whether there's life elsewhere in the universe," Dr Evans-Soma said. "Although Tylos is too hot to support life as we know it, by refining our observational techniques and improving our understanding of these exotic atmospheres, we hope to make steady progress towards characterising more Earth-like planets in the future." In a leap forward in the search for life beyond Earth, an Australian astronomer has detected an unusual mix of gases in the atmosphere of a planet 850 light years away. The discovery, an international effort led by University of Newcastle's Dr Tom Evans-Soma, offers insight into how planets form and whether they could once have supported existence. Published in Nature Astronomy, the research focuses on WASP-121b, or "Tylos" - an ultra-hot gas giant similar to Jupiter but with surface temperatures exceeding 2500C. 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"And that is a really valuable ingredient when it comes to linking the observations to our theories of planet formation." Though Tylos is far too hot to support life as we know it, the research contributes to a growing body of knowledge that could one day identify life beyond our solar system. "Of course, one day we hope to answer the age-old question of whether there's life elsewhere in the universe," Dr Evans-Soma said. "Although Tylos is too hot to support life as we know it, by refining our observational techniques and improving our understanding of these exotic atmospheres, we hope to make steady progress towards characterising more Earth-like planets in the future." In a leap forward in the search for life beyond Earth, an Australian astronomer has detected an unusual mix of gases in the atmosphere of a planet 850 light years away. The discovery, an international effort led by University of Newcastle's Dr Tom Evans-Soma, offers insight into how planets form and whether they could once have supported existence. Published in Nature Astronomy, the research focuses on WASP-121b, or "Tylos" - an ultra-hot gas giant similar to Jupiter but with surface temperatures exceeding 2500C. Using NASA's $A15 billion James Webb Space Telescope, the team observed the Tylos - called an exoplanet as it is beyond our solar system - continuously over 40 hours, capturing more than 3500 exposures. Examining the results pixel-by-pixel, Dr Evans-Soma was able to "essentially take a chemical inventory of the atmosphere" to establish the key chemical "building blocks" of the planet, and the results were striking. While water vapour and carbon monoxide were expected, silicon monoxide was also detected - the first time this gas has been observed in any planetary atmosphere. Even more surprising was the presence of methane on the cooler nightside, a molecule typically only found on far colder planets. "The exciting progress that is groundbreaking about this is the detection of multiple molecules with a single observation that let us get the carbon, oxygen and silicon abundances together," Dr Evans-Soma told AAP. "This has allowed us to really test our theories of planet formation for this particular planet in a way that just hasn't really been possible before." Dr Evans-Soma said the chemical signatures challenge existing models of atmospheric chemistry and suggest Tylos formed in a much colder region of space before migrating closer to its host star. "The silicon enrichment of the atmosphere suggests Tylos incorporated a huge amount of rocky material as it formed - a quantity equivalent to about 30 times the mass of Earth ... (which was) likely delivered by asteroid-like bodies colliding with the planet and becoming engulfed in the atmosphere," he said. This rocky material, vaporised by intense heat, released gases such as silicon monoxide into the planet's atmosphere. It changes astronomers' understanding of how these gasses circulate in the atmosphere and therefore how planets form, he said. "It's opened up potentially a new window that people may not have been thinking about," he said. "And that is a really valuable ingredient when it comes to linking the observations to our theories of planet formation." Though Tylos is far too hot to support life as we know it, the research contributes to a growing body of knowledge that could one day identify life beyond our solar system. "Of course, one day we hope to answer the age-old question of whether there's life elsewhere in the universe," Dr Evans-Soma said. "Although Tylos is too hot to support life as we know it, by refining our observational techniques and improving our understanding of these exotic atmospheres, we hope to make steady progress towards characterising more Earth-like planets in the future." In a leap forward in the search for life beyond Earth, an Australian astronomer has detected an unusual mix of gases in the atmosphere of a planet 850 light years away. The discovery, an international effort led by University of Newcastle's Dr Tom Evans-Soma, offers insight into how planets form and whether they could once have supported existence. Published in Nature Astronomy, the research focuses on WASP-121b, or "Tylos" - an ultra-hot gas giant similar to Jupiter but with surface temperatures exceeding 2500C. Using NASA's $A15 billion James Webb Space Telescope, the team observed the Tylos - called an exoplanet as it is beyond our solar system - continuously over 40 hours, capturing more than 3500 exposures. Examining the results pixel-by-pixel, Dr Evans-Soma was able to "essentially take a chemical inventory of the atmosphere" to establish the key chemical "building blocks" of the planet, and the results were striking. While water vapour and carbon monoxide were expected, silicon monoxide was also detected - the first time this gas has been observed in any planetary atmosphere. Even more surprising was the presence of methane on the cooler nightside, a molecule typically only found on far colder planets. "The exciting progress that is groundbreaking about this is the detection of multiple molecules with a single observation that let us get the carbon, oxygen and silicon abundances together," Dr Evans-Soma told AAP. "This has allowed us to really test our theories of planet formation for this particular planet in a way that just hasn't really been possible before." Dr Evans-Soma said the chemical signatures challenge existing models of atmospheric chemistry and suggest Tylos formed in a much colder region of space before migrating closer to its host star. "The silicon enrichment of the atmosphere suggests Tylos incorporated a huge amount of rocky material as it formed - a quantity equivalent to about 30 times the mass of Earth ... (which was) likely delivered by asteroid-like bodies colliding with the planet and becoming engulfed in the atmosphere," he said. This rocky material, vaporised by intense heat, released gases such as silicon monoxide into the planet's atmosphere. It changes astronomers' understanding of how these gasses circulate in the atmosphere and therefore how planets form, he said. "It's opened up potentially a new window that people may not have been thinking about," he said. "And that is a really valuable ingredient when it comes to linking the observations to our theories of planet formation." Though Tylos is far too hot to support life as we know it, the research contributes to a growing body of knowledge that could one day identify life beyond our solar system. "Of course, one day we hope to answer the age-old question of whether there's life elsewhere in the universe," Dr Evans-Soma said. "Although Tylos is too hot to support life as we know it, by refining our observational techniques and improving our understanding of these exotic atmospheres, we hope to make steady progress towards characterising more Earth-like planets in the future."

Aussie astronomer tests theories of planet formation
Aussie astronomer tests theories of planet formation

Perth Now

time10 hours ago

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Aussie astronomer tests theories of planet formation

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Aussie astronomer tests theories of planet formation
Aussie astronomer tests theories of planet formation

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Aussie astronomer tests theories of planet formation

In a leap forward in the search for life beyond Earth, an Australian astronomer has detected an unusual mix of gases in the atmosphere of a planet 850 light years away. The discovery, an international effort led by University of Newcastle's Dr Tom Evans-Soma, offers insight into how planets form and whether they could once have supported existence. Published in Nature Astronomy , the research focuses on WASP-121b, or "Tylos" - an ultra-hot gas giant similar to Jupiter but with surface temperatures exceeding 2500C. Using NASA's $A15 billion James Webb Space Telescope, the team observed the Tylos - called an exoplanet as it is beyond our solar system - continuously over 40 hours, capturing more than 3500 exposures. Examining the results pixel-by-pixel, Dr Evans-Soma was able to "essentially take a chemical inventory of the atmosphere" to establish the key chemical "building blocks" of the planet, and the results were striking. While water vapour and carbon monoxide were expected, silicon monoxide was also detected - the first time this gas has been observed in any planetary atmosphere. Even more surprising was the presence of methane on the cooler nightside, a molecule typically only found on far colder planets. "The exciting progress that is groundbreaking about this is the detection of multiple molecules with a single observation that let us get the carbon, oxygen and silicon abundances together," Dr Evans-Soma told AAP. "This has allowed us to really test our theories of planet formation for this particular planet in a way that just hasn't really been possible before." Dr Evans-Soma said the chemical signatures challenge existing models of atmospheric chemistry and suggest Tylos formed in a much colder region of space before migrating closer to its host star. "The silicon enrichment of the atmosphere suggests Tylos incorporated a huge amount of rocky material as it formed - a quantity equivalent to about 30 times the mass of Earth ... (which was) likely delivered by asteroid-like bodies colliding with the planet and becoming engulfed in the atmosphere," he said. This rocky material, vaporised by intense heat, released gases such as silicon monoxide into the planet's atmosphere. It changes astronomers' understanding of how these gasses circulate in the atmosphere and therefore how planets form, he said. "It's opened up potentially a new window that people may not have been thinking about," he said. "And that is a really valuable ingredient when it comes to linking the observations to our theories of planet formation." Though Tylos is far too hot to support life as we know it, the research contributes to a growing body of knowledge that could one day identify life beyond our solar system. "Of course, one day we hope to answer the age-old question of whether there's life elsewhere in the universe," Dr Evans-Soma said. "Although Tylos is too hot to support life as we know it, by refining our observational techniques and improving our understanding of these exotic atmospheres, we hope to make steady progress towards characterising more Earth-like planets in the future."

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