Statistics – Computation
Scientific paper
Apr 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989icar...78..270i&link_type=abstract
(Conference on Asteroids II, Tucson, AZ, Mar. 8-11, 1988) Icarus (ISSN 0019-1035), vol. 78, April 1989, p. 270-279.
Statistics
Computation
3
Asteroid Belts, Cosmology, Dynamic Models, Gravitational Effects, Orbital Mechanics, Solar System, Computational Astrophysics, Monte Carlo Method, Orbital Resonances (Celestial Mechanics), Perturbation Theory, Planetesimals, Size, Injection, Asteroid Belt, Source, Accretion, Gravity Effects, Scattering, Monte Carlo Methods, Models, Dynamics, Perturbations, Orbits, Simulations, Composition, Mixing, Calculations, Orbital Elements
Scientific paper
The present Monte Carlo model of a system of planetoids' simultaneous accretion and gravitational scattering in the terrestrial planetary region gives attention to the dynamical consequence of the coaccretion of many lunar- and Martian-size objects, as well as to the possible injection of some of these planetoids into the asteroid belt. On average, two or three such objects may scatter into the main-belt region at different intervals of the 10 million-year accretion process; the terrestrial zone bodies could therefore help to perturb the original asteroid population into eccentric orbits.
No associations
LandOfFree
Dynamical injection of Mars-sized planetoids into the asteroidal belt from the terrestrial planetary accretion zone does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Dynamical injection of Mars-sized planetoids into the asteroidal belt from the terrestrial planetary accretion zone, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamical injection of Mars-sized planetoids into the asteroidal belt from the terrestrial planetary accretion zone will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1737445