Observations of asteroids in the 3- to 4-micron region

Details Observations of asteroids in the 3- to 4-micron region Observations of asteroids in the 3- to 4-micron region

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icar...55..245e&link_type=abstract

Icarus (ISSN 0019-1035), vol. 55, Aug. 1983, p. 245-249. Sponsorship: Science and Engineering Research Council.

Astronomy and Astrophysics

Astronomy

10

Absorption Spectra, Asteroids, Infrared Astronomy, Chemical Composition, Reflectance, Spectrum Analysis, Asteroids, Observations, Spectra, 1 Ceres, 2 Pallas, 8 Flora, Catalog, Wavelengths, S Asteroids, M Asteroids, C Asteroids, Absorption, Data, Classification, Surface, Composition, Photometry, Infrared, 10 Hygeria, 15 Eunomia, 16 Psyche, 22 Kalliope, 83 Beatrix, 433 Eros, 386 Siegena, 471 Papagena, Reflectivity, Comparisons

Scientific paper

Spectra of eleven asteroids (1, 2, 8, 10, 15, 16, 22, 83, 386, 433, 471) have been obtained in the 3- to 4-μm region. Of these, only 1 Ceres and 2 Pallas have previously been observed in this wavelength region. Spectra of the S- and M-type asteroids are generally featureless, but 8 Flora may be an exception. None of the three new C-type spectra show significant absorption.

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