4.5 Article

A new material for the icy Galilean moons: The structure of sulfuric acid hexahydrate

Journal

JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
Volume 118, Issue 9, Pages 1895-1902

Publisher

AMER GEOPHYSICAL UNION
DOI: 10.1002/jgre.20124

Keywords

Hydrates; Icy moons; Europa; Ganymede

Funding

  1. Australian Synchrotron

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This study presents a newly identified water-rich crystalline form of sulfuric acid hydrate, H2SO4 center dot 6H(2)O, a hexahydrate. The method of formation of this material suggests that sulfuric acid hexahydrate (SAHx) could be an abundant material on the surface of Jupiter's Galilean ice moons, Europa, Ganymede, and Callisto. The structure of SAHx was determined by the combined use of synchrotron X-ray and neutron powder diffraction data. The structural arrangement of SAHx exhibits the same water layer topology that has been determined for sulfuric acid octahydrate (SAO), but differs in the stacking of this water layer and the interlayer species. SAHx is observed to form over a large range of solution compositions and displays stability over the temperature range 80 to 190K.

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