Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acm..proc..167f&link_type=abstract
In Lunar and Planetary Inst., Asteroids, Comets, Meteors 1991 p 167-170 (SEE N93-19113 06-90)
Astronomy and Astrophysics
Astronomy
1
Asteroids, Astronomical Models, Collisions, Fragments, Meteorites, Orbital Resonances (Celestial Mechanics), Asteroid Belts, Mathematical Models
Scientific paper
We have quantitatively modeled the chance insertion of asteroid collisional fragments into the 3:1 and g = g6 resonances, through which they can achieve Earth-approaching orbits. Although the results depend on some poorly known parameters, they indicate that most meteorites and near-earth asteroids probably come from a small and non-representative sample of asteroids, located in the neighborhood of the two resonances.
Farinella Paolo
Froeschlé Christiane
Froeschle' Claude
Gonczi Robert
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