Please use this identifier to cite or link to this item: https://apo.ansto.gov.au/dspace/handle/10238/12056
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dc.contributor.authorMaynard-Casely, HE-
dc.contributor.authorBrand, HEA-
dc.contributor.authorCable, ML-
dc.contributor.authorHodyss, R-
dc.date.accessioned2021-10-22T04:34:46Z-
dc.date.available2021-10-22T04:34:46Z-
dc.date.issued2016-11-29-
dc.identifier.citationMaynard-Casely, H. E., Brand, H. E. A., Cable, M. L., & Hodyss, R. (2016). Characterising new planetary materials with neutron diffraction. Paper presented at 13th AINSE-ANBUG Neutron Scattering Symposium, Sydney, NSW, Australia, 29-30 November 2016.en_US
dc.identifier.urihttps://apo.ansto.gov.au/dspace/handle/10238/12056-
dc.description.abstractThere’s a lot of hydrogen in the outer solar system; locked up with water on the icy Galilean moons of Jupiter, within the small organic molecules that rain down on Saturn’s moons Titan or even in an elusive metallic form within the centers of the gas giants. The intrinsic hydrogen-domination of planetary ices, makes studying these materials with laboratory powder diffraction very challenging. Insights into their crystalline phase behavior and the extraction of a number of thermal and mechanical properties is often only accessible with high-flux synchrotron x-ray diffraction or with neutron diffraction. Here, we will present how both the ECHIDNA and WOMBAT instruments at ACNS have been used to gain insights into new materials that have be found to exist under planetary conditions.en_US
dc.language.isoenen_US
dc.publisherAustralian Institute of Nuclear Science and Engineeringen_US
dc.subjectX-ray diffrationen_US
dc.subjectNeutron diffractionen_US
dc.subjectPlanetsen_US
dc.subjectIceen_US
dc.subjectSatellite atmospheresen_US
dc.subjectANSTOen_US
dc.titleCharacterising new planetary materials with neutron diffractionen_US
dc.typeConference Abstracten_US
dc.date.statistics2021-10-11-
Appears in Collections:Conference Publications

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