by an empirical model during the rebound phase that balances a lift force against gravity. We estimate constraints on projectile radius, velocity and impact angle that would allow projectiles on asteroids to ricochet or roll away from impact, finally coming to rest distant from their initial impact sites.'
address:
- 'Department of Physics and Astronomy, University of Rochester, Rochester, NY 14627, USA'
- 'Dept. of Computer Science, University of Rochester, Rochester, NY, 14627, USA'
- 'Colorado Center for Astrodynamics Research, The University of Colorado Boulder, UCB 431, Boulder, CO 80309-0431, United States'
- 'Department of Mechanical Engineering, University of Rochester, Rochester, NY 14627, USA'
- 'Department of Earth and Environmental Sciences, University of Rochester, Rochester, NY 14627, USA'
- 'Lunar and Planetary Lab, University of Arizona, Tucson, AZ, USA'
- 'Laboratoire Lagrange, Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, C.S. 34229, 06304 Nice Cedex 4, France'
author:
- Esteban Wright
- 'Alice C. Quillen'
- Juliana South
- 'Randal C. Nelson'
- Paul Sánchez
- John Siu
- Hesam Askari
- Miki Nakajima
- 'Stephen R. Schwartz'
bibliography:
- 'ricochet\_v03.bib'
title: Ricochets on Asteroids
---

Introduction
============

Impact crater ejecta curtains, seismicity associated with impacts (e.g. @wright19), and 