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A six-part collisional model of the main asteroid belt

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F14%3A10286599" target="_blank" >RIV/00216208:11320/14:10286599 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1016/j.icarus.2014.07.016" target="_blank" >http://dx.doi.org/10.1016/j.icarus.2014.07.016</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1016/j.icarus.2014.07.016" target="_blank" >10.1016/j.icarus.2014.07.016</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    A six-part collisional model of the main asteroid belt

  • Original language description

    In this work, we construct a new model for the collisional evolution of the main asteroid belt. Our goals are to test the scaling law of Benz and Asphaug (Benz, W., Asphaug, E. [1999]. Icarus, 142, 5-20) and ascertain if it can be used for the whole belt. We want to find initial size-frequency distributions (SEDs) for the considered six parts of the belt (inner, middle, "pristine", outer, Cybele zone, high-inclination region) and to verify if the number of synthetic asteroid families created during thesimulation matches the number of observed families as well. We used new observational data from the WISE satellite (Masiero et al., 2011) to construct the observed SFDs. We simulate mutual collisions of asteroids with a modified version of the Boulder code (Morbidelli, A., et al. [2009]. Icarus, 204, 558-573), where the results of hydrodynamic (SPH) simulations of Durda et al. (Durda, D.D., et al. 120071 Icarus, 498-516) and Benavidez et al. (Benavidez, P.G., et al. [2012]. 219, 57-76) a

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    <a href="/en/project/GA13-01308S" target="_blank" >GA13-01308S: Dynamics of small bodies in the solar system</a><br>

  • Continuities

    Z - Vyzkumny zamer (s odkazem do CEZ)<br>S - Specificky vyzkum na vysokych skolach

Others

  • Publication year

    2014

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Icarus

  • ISSN

    0019-1035

  • e-ISSN

  • Volume of the periodical

    241

  • Issue of the periodical within the volume

    říjen

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    15

  • Pages from-to

    358-372

  • UT code for WoS article

    000343617900026

  • EID of the result in the Scopus database