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From the following article:

Compositional differences between meteorites and near-Earth asteroids

P. Vernazza, R. P. Binzel, C. A. Thomas, F. E. DeMeo, S. J. Bus, A. S. Rivkin & A. T. Tokunaga

Nature 454, 858-860(14 August 2008)

doi:10.1038/nature07154

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Figure 2

Model results for the ratio of olivine to olivine+orthopyroxene for 57 ordinary chondrites and 38 S- and Q-type NEAs.

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