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How this Australian particle accelerator highlights a crisis facing AUKUS

How this Australian particle accelerator highlights a crisis facing AUKUS

The Age29-04-2025

In another room, physicists shoot nitrogen atoms into diamonds, creating the 'qubit' building blocks of future quantum computers. Global scientists have the accelerator booked out for months in advance.
And the accelerator plays a crucial role in a more esoteric quest: the hunt for new elements.
How to make a new element
The accelerator room's a riot of coloured wires, chrome pipes, Ferrari red particle-boosting magnets and metal chambers where the sped-up ions smash into their target.
Hinde built much of the custom equipment in this room himself.
He's one of the scientists who have gathered at the brutalist beacon of the accelerator's building to celebrate a milestone recognition award from the prestigious Institute of Electrical and Electronics Engineers. It's the third Australian facility to receive the honour, alongside the famous Parkes Dish and the Tidbinbilla Deep Space Tracking Station.
Hinde was part of the international team that confirmed the addition of a new element to the periodic table: element 117, or tennessine. It was made by smashing together calcium-48 and berkelium-249. The intense process produced four atoms of tennessine which fell apart in milliseconds.
Element 118, oganesson, has also been recognised after five atoms were painstakingly produced across multiple experiments.
'But how do you make element 119 and 120? Turns out we, the scientific community, don't actually know,' Hinde says.
The method of smashing calcium-48 with a heavy element has reached its practical limit because, to create element 119, you'd need einsteinium; an element discovered in the debris of a hydrogen bomb test that's quick to decay and can only be manufactured in tiny quantities (nanograms, rather than grams).
That's why Hinde and Cook are investigating other ways of cooking up novel elements.
'We've discovered a whole new region of fission and nuclei that behave in an unexpected way,' Hinde says. 'That's something we've been able to do with this accelerator, perhaps something we wouldn't have been able to do anywhere else in the world.'
But why pursue new elements at all, if they flash into existence for less time than it takes to blink?
Curiosity and new cancer treatments
Part of the hunt for new elements is motivated by good old-fashioned competition. 'A lot of it, to be frank, is nationalism and national pride,' says chief executive of the facility, Dr Tom McGoram. 'For China and the United States, it's that strategic arm wrestling and posturing. Not so much here. We do it because we're fascinated by the physics of it.'
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There are no practical uses for the new elements.
'But there's no more stringent test of our ability to understand complex quantum systems than superheated nuclei,' says McGoram.
'And really, that's the same story that's always led us to applications – let's think of the hardest thing we can think of to do and have a crack at it.'
McGoram nominates lutetium-177 as an example of this; fundamental nuclear physicists examining the nuclei of this rare earth element discovered they could attach it to a molecule that concentrates in the prostate. That's morphed into a groundbreaking, targeted new treatment for metastatic prostate cancer that significantly boosts survival rates.
They didn't set out to create a new drug; the physicists just wanted to better understand the underlying science of atoms. 'It's research like that into the quantum structure of radio nuclei that leads to new therapies for treating cancer,' McGoram says. 'It's pretty cool.'
The key AUKUS warning
This is also one of the few places in the world where science students are tasked with controlling an entire particle accelerator. It's as practical as an apprenticeship, McGoram says.
Many students, though, are hired by labs in the US or elsewhere overseas. That's something Australia needs to quickly reverse.
We'll need nuclear engineers and physicists to safely house and run the AUKUS submarines slated to arrive in the late 2030s; at least 200 nuclear experts and 4300 people trained in nuclear engineering, according to one analysis.
But there aren't enough tenured nuclear physicists to provide the high-level training needed to fully embrace domestic nuclear opportunities in defence, space, medicine and agriculture. There are so few in Australia I've just met half of them in the facility's lobby.
'We're down to single-digit tenured nuclear scientists in Australia. By the OECD average we should have 40 or 50,' McGoram says. The Australian Academy of Science calls it a nuclear skills crisis.
The lack of senior academic talent is partly a consequence of cuts to nuclear science in the 1980s, the scientists tell me. That serves as a warning of how future prosperity suffers from underfunded science; knock-on effects echo through the decades.
As Rick Spinrad, former head of the US's National Oceanic and Atmospheric Administration, warned this week about the Trump administration's massive funding freezes to research: 'This is not like tariffs. You can't just turn a science switch off and then turn it back on again.'

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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. 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"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. 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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

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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
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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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