Close encounters between star-planet systems and stellar intruders. II - Effect of the mass and impact velocity of the intruder

Statistics – Computation

Scientific paper

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Collision Parameters, Extrasolar Planets, Impact Acceleration, Stars, Stellar Mass, Computational Astrophysics, Dissociation, Eccentricity, Globular Clusters, Interacting Galaxies

Scientific paper

Results are reported from over 300,000 simulations of encounters between a planet-star binary system and intruders whose masses range from 0.1 to 100 times the mass of the home star of the planet-star system. These calculations were done at a large number of collision velocities and impact parameters. Cross sections for dissociation, for exchange collisions, for changing the orbital energy, and for changing the orbital eccentricity were determined.

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