Dynamical Behaviour of Asteroids in the Region a < 2 AU View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

2002

AUTHORS

Francisco Lopez-Garcia , Adrian Brunini

ABSTRACT

We carried out a series of numerical simulations of the dynamical evolution of test particles and real asteroids in the inner region of the Solar System. We explored two different scenarios: i) including terrestrial planets plus Jupiter and Saturn and ii) including all the planets (except Pluto). We found that there are possible zones of orbital stability where planetesimals may survive 100 Myr. Secular resonances with the inner planets and mean motion commensurabilities with both the inner and outer planets play a key role in the dynamical evolution of this region. More... »

PAGES

417-422

References to SciGraph publications

Book

TITLE

Modern Celestial Mechanics: From Theory to Applications

ISBN

978-90-481-6078-5
978-94-017-2304-6

Author Affiliations

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-94-017-2304-6_33

DOI

http://dx.doi.org/10.1007/978-94-017-2304-6_33

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1015230117


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