Collisional parameters of planetesimal belts, precursor of debris disks, perturbed by a nearby giant...
Collisional parameters of planetesimal belts, precursor of debris disks, perturbed by a nearby giant planet
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Contents
Planetesimal belts are invoked to explain the prolonged existence of debris disks. Important parameters to model their collisional evolution and to compute the dust production rate are the intrinsic probability of collision \(P_i\) and the mean impact velocity \(U_c\). If a planet orbits close to the belt, the values of both these parameters are af...
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Collisional parameters of planetesimal belts, precursor of debris disks, perturbed by a nearby giant planet
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TN_cdi_proquest_journals_2074624477
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2074624477
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1612.08635
