Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8134269 | Icarus | 2018 | 17 Pages |
Abstract
The two observables that spectroscopically separate the different meteorites groups (and thus the different types of parent bodies) are the pyroxene-olivine feature strength ratio and the peak shift of the olivine spectral features due to an increase in the iron concentration of the olivine.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
B.L. de Vries, H. Skogby, L.B.F.M. Waters, M. Min,