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High surface porosity as the origin of emissivity features in asteroid spectra

Vernazza, P; Delbo, M; King, Penelope; Izawa, M; Olofsson, J; Lamy, P; Cipriani, F; Binzel, R; Marchis, F; Merin, B; Tamanai, A

Description

Emission features in the mid-IR domain (7-25 μm) are quite ubiquitous among large asteroids and therefore offer the potential to uncover their surface composition. However, when comparing these spectra with the actual laboratory spectra of both minerals

CollectionsANU Research Publications
Date published: 2012
Type: Journal article
URI: http://hdl.handle.net/1885/32904
Source: Icarus
DOI: 10.1016/j.icarus.2012.04.003

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