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NEOMOD: A New Orbital Distribution Model for Near-Earth Objects
Capture of irregular satellites at Jupiter
Satellite de-orbiting via controlled solar radiation pressure
Collisional Evolution of Meter- to Kilometer-sized Planetesimals in Mean Motion Resonances: Implications for Inward Planet Shepherding
Energy Dissipation in Large CollisionsāNo Change in Planet Formation Outcomes
Excitation of a Primordial Cold Asteroid Belt as an Outcome of Planetary Instability
Constraining the Giant Planetsā Initial Configuration from Their Evolution: Implications for the Timing of the Planetary Instability
Efficiency characterization of the V-shape asteroid family detection method
