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The characterisation of planetary materials

The characterisation of planetary materials

ANSTO provides a range of capabilities using neutrons, X-rays and infrared radiation to study the solids, liquids and gases that might be found in materials in our solar system and beyond.

hills on Mars

The characterisation of planetary materials

ANSTO provides a range of capabilities using neutrons, X-rays and infrared radiation to study the solids, liquids and gases that might be found in materials in our solar system and beyond.

After your experiment clayton

After your experiment

Following your experiment at the Australian Synchrotron there are certain tasks that users can complete including a user feedback survey and claiming reimbursement for travel expenses.

Cryogenic Permanent Magnet Undulator (CPMU) source for the BRIGHT Nanoprobe beamline

Nanoprobe beamline (NANO) - under construction

The BRIGHT Nanoprobe beamline provides a unique facility capable of spectroscopic and full-field imaging. NANO will undertake high-resolution elemental mapping and ptychographic coherent diffraction imaging. Elemental mapping and XANES studies (after DCM upgrade) will be possible at sub-100 nm resolution, with structural features able to be studied down to 15 nm using ptychography.

Aerial image of ANSTO's Lucas Heights facility

Statement of Intent

In January 2026, Mr Michael Quigley AM, ANSTO Board Chair, shared ANSTO's Statement of Intent with the Minister for Industry and Innovation, and Minister for Science.

BioSAXS

Biological small angle X-ray scattering beamline (BioSAXS)

The Biological Small Angle X-ray Scattering beamline will be optimised for measuring small angle scattering of surfactants, nanoparticles, polymers, lipids, proteins and other biological macromolecules in solution. BioSAXS combines combine a state-of-the-art high-flux small angle scattering beamline with specialised in-line protein purification and preparation techniques for high-throughput protein analysis.

Infrared microspectroscopy

Infrared microspectroscopy

The Infrared Microspectroscopy beamline combines the high brilliance and collimation of the synchrotron beam through a Bruker V80v Fourier Transform Infrared (FTIR) spectrometer and into a Hyperion 3000 IR microscope to reach high signal-to-noise ratios at diffraction limited spatial resolutions between 3-8 μm.

MEX Hutch A

Medium Energy X-ray Absorption Spectroscopy Beamline (MEX-1 and MEX-2)

The Medium Energy- X-ray Absorption Spectroscopy beamlines will provide access to XANES and EXAFS data from a bending magnet source, optimised for cutting-edge applications in biological, agricultural and environmental science in an energy range that is not currently available at the Australia Synchrotron.

Pagination