Shape models and dynamical properties of basaltic asteroids outside the dynamical Vesta family
Through numerical modeling, Nesvorny et al. (2008) showed that asteroids can migrate due to Yarkovsky drift and resonances to outside of the boundaries of the Vesta family. In particular, they found that objects which end up in the scattered resonances region (so-called Cell I, defined by orbital elements 2.2 AU < a < 2.3 AU, 0.05 < e < 0.2, 0 < i
Troianskyi, Volodymyr et al.
Fecha de publicación:
9
2021