Number of the records: 1  

Thermal stresses in small meteoroids

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    SYSNO ASEP0354050
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleThermal stresses in small meteoroids
    Author(s) Čapek, David (ASU-R) RID, ORCID
    Vokrouhlický, D. (CZ)
    Source TitleAstronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
    Roč. 519, Sept (2010), A75/1-A75/16
    Number of pages16 s.
    Languageeng - English
    CountryFR - France
    Keywordsmeteorites ; meteors ; meteoroids
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    R&D ProjectsGP205/09/P455 GA ČR - Czech Science Foundation (CSF)
    CEZAV0Z10030501 - ASU-R (2005-2011)
    UT WOS000283297300075
    DOI10.1051/0004-6361/201014281
    AnnotationOur results indicate that the onset of thermal failure in the meteoroid depends on a number of parameters including the heliocentric distance, the size, the rotation frequency, and the orientation of the spin axis with respect to the solar direction. In our case, we find large, centimeter- to meter-size, slowly rotating meteoroids or those with a spin axis pointing towards the Sun or both, are the most susceptible to the thermal bursting. This may have implications for the (i) size distribution of meteoroids in various streams depending on their heliocentric orbit and the physical characteristics of their parent bodies; (ii) orbital distribution of sporadic complexes of meteoroids in the planet-crossing zone; and/or (iii) fate of fragments released during comet disintegration events, especially those with low perihelia (e.g., Kreutz class).
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2011
Number of the records: 1  

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