70 years of scientific excellence has brought significant benefits to Australia
ANSTO is a unique national science organisation that began operating under its predecessor The Australian Atomic Energy Commission (AAEC) 70 years ago.
Showing 261 - 280 of 399 results
ANSTO is a unique national science organisation that began operating under its predecessor The Australian Atomic Energy Commission (AAEC) 70 years ago.
ANSTO is proud to host the Shorebirds Competition for the fifth year. This unique environmental poster competition is free to enter and offers over $4500 in prizes for students and schools!
Snapshots of an unprecedented double element-hydrogen bond activation at a transition metal centre.
Australia part of global renaissance in fusion power research symbolised by ITER experiment
A collaboration of Australian scientists has used ANSTO’s Australian Synchrotron to measure the amount of carbon that is captured in microscopic seams of deep-sea limestone, which acts as a carbon sink.
Exploring the interaction of polystyrene nanoplastics and blood plasma proteins.
nandin is ANSTO’s Innovation Centre where science and technology entrepreneurs, startups and graduates meet industry expertise to experiment, co-create, innovate, and commercialise, creating new jobs in the high-growth industries of tomorrow.
ANSTO's OPAL reactor is one of the world's most advanced and reliable research reactors today. To ensure we can continue operating OPAL safely and reliably and maximise utilisation, ANSTO must regularly carry out maintenance and upgrades.
Collaboration across the Tasman has enabled Australian and New Zealand researchers and scientists to shed light on a protein involved in diseases such as Parkinson’s disease, gastric cancer and melanoma.
International palaeontologists have used advanced imaging techniques at ANSTO’S Australian Synchrotron to clarify the role that the earliest fruit-eating birds of the Cretaceous period may have had in helping fruit-producing plants to evolve.
Soft x-rays are generally understood to be x-rays in the energy range 100-3,000 eV. They have insufficient energy to penetrate the beryllium window of a hard x-ray beamline but have energies higher than that of extreme ultraviolet light.