| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8136571 | Icarus | 2015 | 16 Pages |
Abstract
The technique used to constrain the composition described as part of this study introduces a new approach at investigating the surface chemistry of the very small and numerous objects that constitute the bulk of the TNO and centaur populations. This innovative method has the potential to provide constraints for irradiation theories and for models of dynamical and chemical evolution of the Solar System.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
C. Morea Dalle Ore, M.A. Barucci, J.P. Emery, D.P. Cruikshank, C. de Bergh, T.L. Roush, D. Perna, F. Merlin, L.V. Dalle Ore,