Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8135679 | Icarus | 2016 | 19 Pages |
Abstract
The visible spectra of the two targets of sample return missions, Asteroids Bennu and Ryugu, are compatible with the spectra of the asteroids in this region, supporting previous studies that suggested either the Polana family or the background population as the most likely origins of these NEAs.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
J. de León, N. Pinilla-Alonso, M. Delbo, H. Campins, A. Cabrera-Lavers, P. Tanga, A. Cellino, P. Bendjoya, J. Gayon-Markt, J. Licandro, V. Lorenzi, D. Morate, K.J. Walsh, F. DeMeo, Z. Landsman, V. AlÃ-Lagoa,