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The diameter and albedo of 1943 AnterosThe results of broadband visual and infrared photometry of the Apollo-Amor asteroid 1943 Anteros during its 1980 apparition are reported. By means of a radiometric model, a diameter of 2.3 + or - 0.2 km and a visual geometric albedo of 0.13 + or - 0.03 is calculated. The albedo and reflectance spectrum of Anteros imply that it is a type S asteroid. Thus, Anteros may have a silicate surface similar to other Apollo-Amor asteroids as well as some stony-iron meteorites.
Document ID
19810058939
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Veeder, G. J.
(Arizona Univ. Tucson, AZ, United States)
Tedesco, E. F.
(Arizona Univ. Tucson, AZ, United States)
Tholen, D. J.
(Arizona, University Tucson, AZ, United States)
Tokunaga, A.
(Hawaii, University Honolulu, HI, United States)
Matthews, K.
(Arizona Univ. Tucson, AZ, United States)
Neugebauer, G.
(Arizona Univ. Tucson, AZ, United States)
Soifer, B. T.
(Palomar Observatory Pasadena, CA, United States)
Kowal, C.
(Arizona Univ. Tucson, AZ, United States)
Date Acquired
August 11, 2013
Publication Date
May 1, 1981
Publication Information
Publication: Icarus
Volume: 46
Subject Category
Lunar And Planetary Exploration
Accession Number
81A43343
Funding Number(s)
CONTRACT_GRANT: NAS7-100
Distribution Limits
Public
Copyright
Other

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