title: Origin of multikilometer earth- and mars-crossing asteroids: A quantitative simulation
abstract: Orbital dynamic simulations show that many asteroids in the main asteroid belt are driven toward Mars-crossing orbits by numerous weak mean motion resonances, which slowly increase the orbital ellipticity of the asteroids. In addition, half of the Mars-crossing asteroids (MCAs) transition to Earth-crossing asteroids (ECAs) in less than 20 million years. This scenario quantitatively explains the observed number of large ECAs and MCAs.
authors.affiliation: F. Migliorini, Armagh Observatory, College Hill BT61 9DG, Northern Ireland, United Kingdom, and Osservatorio Astronomico di Torino, I-10025 Pino Torinese, Italy. P. Michel, Osservatorio Astronomico di Torino, I-10025 Pino Torinese, Italy, and Obse.
authors.initials: F
authors.lastname: Migliorini
authors.initials: P
authors.lastname: Michel
authors.initials: A
authors.lastname: Morbidelli
authors.initials: D
authors.lastname: Nesvorny
authors.initials: V
authors.lastname: Zappala