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Meteorite Delivery and Transport

Published online by Cambridge University Press:  19 July 2016

Paolo Farinella ,
Claude Froeschlé  and
Robert Gonczi
Paolo Farinella
Affiliation:
Dipartimento di Matematica, Università di Pisa, Via Buonarroti 2, I-56127 Pisa, Italy Observatoire de la Côte d'Azur, B.P. 229, F-06304 Nice Cedex 4, France E-mail: [email protected], ZAPPALA@OBS–NICE.FR
Claude Froeschlé
Affiliation:
Observatoire de la Côte d'Azur, B.P. 229, F–06304 Nice Cedex 4, France
Robert Gonczi
Affiliation:
Observatoire de la Côte d'Azur, B.P. 229, F–06304 Nice Cedex 4, France

Abstract

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Understanding how meteorites and near–Earth asteroids reach their Earth–crossing orbits starting as fragments from main–belt asteroids is a basic prerequisite to identifying the original parent bodies of these objects and building a self–consistent cosmogonical interpretation of the observed properties of meteorites. We review the recent progress made in this area and the most important remaining open problems. These concern the physics of asteroidal collisions, the size distribution of small main–belt asteroids, the efficiency of different dynamical routes, and the relationships between asteroid taxonomic types based on spectrophotometry data and meteorite classes having different thermal histories and compositions.

Type
Dynamics
Information
Symposium - International Astronomical Union , Volume 160: Asteroids, Comets, Meteors 1993 , 1994 , pp. 205 - 222
Copyright
Copyright © Kluwer 1994 

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