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

dc.contributor.author	Delbó M.
dc.contributor.author	Harris A.W.
dc.date.accessioned	2021-05-28T08:26:45Z
dc.date.available	2021-05-28T08:26:45Z
dc.date.issued	2002
dc.identifier	https://www.elibrary.ru/item.asp?id=14214964
dc.identifier.citation	Meteoritics and Planetary Science, 2002, 37, 12, 1929-1936
dc.identifier.issn	1086-9379
dc.identifier.uri	https://repository.geologyscience.ru/handle/123456789/28749
dc.description.abstract	We 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.title	PHYSICAL PROPERTIES OF NEAR-EARTH ASTEROIDS FROM THERMAL INFRARED OBSERVATIONS AND THERMAL MODELING
dc.type	Статья

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