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

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dc.contributor.authorVernazza, P
dc.contributor.authorDelbo, M
dc.contributor.authorKing, Penelope
dc.contributor.authorIzawa, M
dc.contributor.authorOlofsson, J
dc.contributor.authorLamy, P
dc.contributor.authorCipriani, F
dc.contributor.authorBinzel, R
dc.contributor.authorMarchis, F
dc.contributor.authorMerin, B
dc.contributor.authorTamanai, A
dc.date.accessioned2015-12-08T22:23:32Z
dc.date.issued2012
dc.date.updated2016-02-24T11:40:37Z
dc.description.abstractEmission 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
dc.identifier.issn0019-1035
dc.identifier.urihttp://hdl.handle.net/1885/32904
dc.publisherAcademic Press
dc.sourceIcarus
dc.subjectKeywords: Asteroids; Composition; Infrared observations; Meteorites; Regoliths
dc.titleHigh surface porosity as the origin of emissivity features in asteroid spectra
dc.typeJournal article
local.bibliographicCitation.lastpage1172
local.bibliographicCitation.startpage1162
local.contributor.affiliationVernazza, P, European Southern Observatory
local.contributor.affiliationDelbo, M, UNS–CNRS–Observatoire de la Côte d’Azur,
local.contributor.affiliationKing, Penelope, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationIzawa, M, University of Western Ontario
local.contributor.affiliationOlofsson, J, Max Planck Institute for Astronomy
local.contributor.affiliationLamy, P, Laboratoire d’Astrophysique de Marseille
local.contributor.affiliationCipriani, F, European Space Agency
local.contributor.affiliationBinzel, R, Massachusetts Institute of Technology
local.contributor.affiliationMarchis, F, SETI Institute
local.contributor.affiliationMerin, B, Herschel Science Centre
local.contributor.affiliationTamanai, A, Kirchhoff-Institut für Physik
local.contributor.authoruidKing, Penelope, u3482508
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor040299 - Geochemistry not elsewhere classified
local.identifier.absseo970104 - Expanding Knowledge in the Earth Sciences
local.identifier.ariespublicationU8501506xPUB96
local.identifier.citationvolume221
local.identifier.doi10.1016/j.icarus.2012.04.003
local.identifier.scopusID2-s2.0-84860592265
local.identifier.thomsonID000312434300056
local.type.statusPublished Version

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