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dc.contributor.authorDelbó, M.
dc.contributor.authorHarris, A. W.
dc.date.accessioned2021-02-12T20:55:54Z
dc.date.available2021-02-12T20:55:54Z
dc.date.issued2002-01-01
dc.identifier.citationDelbó, M., & Harris, A. W. (2002). Physical properties of near‐Earth asteroids from thermal infrared observations and thermal modeling. Meteoritics & Planetary Science, 37(12), 1929-1936.
dc.identifier.issn1945-5100
dc.identifier.doi10.1111/j.1945-5100.2002.tb01174.x
dc.identifier.urihttp://hdl.handle.net/10150/655614
dc.description.abstractWe review the physical principles on which asteroid thermal models are based and their application in the derivation of asteroid sizes and albedos. In particular, the use of simple thermal models to derive reliable diameters and albedos of near-Earth asteroids is discussed.
dc.language.isoen
dc.publisherThe Meteoritical Society
dc.relation.urlhttps://meteoritical.org/
dc.rightsCopyright © The Meteoritical Society
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjectasteroids
dc.subjectthermal models
dc.subjectalbedos
dc.subjectnear-Earth asteroids
dc.titlePhysical properties of near-Earth asteroids from thermal infrared observations and thermal modeling
dc.typeArticle
dc.typetext
dc.identifier.journalMeteoritics & Planetary Science
dc.description.collectioninformationThe Meteoritics & Planetary Science archives are made available by the Meteoritical Society and the University of Arizona Libraries. Contact lbry-journals@email.arizona.edu for further information.
dc.eprint.versionFinal published version
dc.description.admin-noteMigrated from OJS platform February 2021
dc.source.volume37
dc.source.issue12
dc.source.beginpage1929
dc.source.endpage1936
refterms.dateFOA2021-02-12T20:55:54Z


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