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Binary asteroid population. 2. Anisotropic distribution of orbit poles of small, inner main-belt binaries

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F12%3A10129181" target="_blank" >RIV/00216208:11320/12:10129181 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985815:_____/12:00388364

  • Result on the web

    <a href="http://dx.doi.org/10.1016/j.icarus.2011.11.026" target="_blank" >http://dx.doi.org/10.1016/j.icarus.2011.11.026</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1016/j.icarus.2011.11.026" target="_blank" >10.1016/j.icarus.2011.11.026</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Binary asteroid population. 2. Anisotropic distribution of orbit poles of small, inner main-belt binaries

  • Original language description

    Our photometric observations of 18 main-belt binary systems in more than one apparition revealed a strikingly high number of 15 having positively re-observed mutual events in the return apparitions. Our simulations of the survey showed that it cannot bedue to an observational selection effect and that the data strongly suggest that poles of mutual orbits between components of binary asteroids in the primary size range 3-8 km are not distributed randomly: The null hypothesis of an isotropic distributionof the orbit poles is rejected at a confidence level greater than 99.99%. Binary orbit poles concentrate at high ecliptic latitudes, within 300 of the poles of the ecliptic. We propose that the binary orbit poles oriented preferentially up/down-right are due to either of the two processes: (i) the YORP tilt of spin axes of their parent bodies toward the asymptotic states near obliquities 0 degrees and 180 degrees (pre-formation mechanism) or (ii) the YORP tilt of spin axes of the primar

  • 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

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)

Others

  • Publication year

    2012

  • 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

    218

  • Issue of the periodical within the volume

    1

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    19

  • Pages from-to

    125-143

  • UT code for WoS article

    000301637700011

  • EID of the result in the Scopus database