On the spectral similarity of carbonaceous chondrites and some hydrated and oxidized asteroids

Details On the spectral similarity of carbonaceous chondrites and some hydrated and oxidized asteroids On the spectral similarity of carbonaceous chondrites and some hydrated and oxidized asteroids

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.500..933b&link_type=abstract

In: Proceedings of Asteroids, Comets, Meteors - ACM 2002. International Conference, 29 July - 2 August 2002, Berlin, Germany. Ed

Computer Science

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Minor Planets: Carbonaceous Chondrites

Scientific paper

We have obtained visible and near-IR reflectance spectra of the CI-, CM2-, CO3- and CV3-chondrites with the purpose of comparing them with the reflectance spectra of selected asteroids. Several absorption bands, mainly in the region of 600-1000 nm, resembling to those of hydrated silicates, were found. Similar absorption features are seen in the reflectance spectra of C-type asteroids and hydrated or highly oxidized M-, E- and S-asteroids. On this basis we assume that a carbonaceous chondrite material may be present on the surfaces of these celestial bodies.

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