PHYSICAL PROPERTIES OF NEAR-EARTH ASTEROIDS FROM THERMAL INFRARED OBSERVATIONS AND THERMAL MODELING

dc.contributor.authorDelbó M.
dc.contributor.authorHarris A.W.
dc.date.accessioned2021-05-28T08:26:45Z
dc.date.available2021-05-28T08:26:45Z
dc.date.issued2002
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.identifierhttps://www.elibrary.ru/item.asp?id=14214964
dc.identifier.citationMeteoritics and Planetary Science, 2002, 37, 12, 1929-1936
dc.identifier.issn1086-9379
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/28749
dc.titlePHYSICAL PROPERTIES OF NEAR-EARTH ASTEROIDS FROM THERMAL INFRARED OBSERVATIONS AND THERMAL MODELING
dc.typeСтатья

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