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

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Authors

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

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Academic Press

Abstract

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

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Source

Icarus

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Restricted until

2037-12-31