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Spectral analogues of Barbarian asteroids among CO and CV chondrites by Mahlke, Max; Eschrig, Jolantha; Carry, Benoit; Bonal, Lydie; Beck, Pierre is a scholarly article available to read on EtoBox.
What is Spectral analogues of Barbarian asteroids among CO and CV chondrites about?
K- and L-type asteroids are considered to be the parent bodies of CV and CO chondrites. Spectral models of L-types invoke an enrichment in CAI with respect to the chondrites in the meteorite collection. Barbarian asteroids are associated to L-type asteroids yet the relationship between these populations is still not clear. We aim to investigate the link between the K- and L-type and Barbarian asteroids and the CV and CO chondrites by means of spectral matching of a large number of reflectance spectra of objects from either population. We seek to identify matches based on observed rather than modelled spectral features. We employ a matching criterion that accounts for the residuals and the correlation of the spectral features. The only free parameter in the comparison is the degree of alteration of the asteroids with respect to the meteorites expressed via an exponential model. We derive an absolute scale of similarity between the spectra using laboratory data from irradiation experiments. CVOxA chondrites are the best match to the asteroids, in particular to K-type (7 out of 11 asteroids matched) and Barbarians (11 out of 16). CO chondrites provide convincing matches for K-types (5
- Author
- Mahlke, Max; Eschrig, Jolantha; Carry, Benoit; Bonal, Lydie; Beck, Pierre
- Published
- 2023
- Language
- EN
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