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Thermal stresses in small meteoroids
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SYSNO ASEP 0354050 Druh ASEP J - Článek v odborném periodiku Zařazení RIV J - Článek v odborném periodiku Poddruh J Článek ve WOS Název Thermal stresses in small meteoroids Tvůrce(i) Čapek, David (ASU-R) RID, ORCID
Vokrouhlický, D. (CZ)Zdroj.dok. Astronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
Roč. 519, Sept (2010), A75/1-A75/16Poč.str. 16 s. Jazyk dok. eng - angličtina Země vyd. FR - Francie Klíč. slova meteorites ; meteors ; meteoroids Vědní obor RIV BN - Astronomie a nebeská mechanika, astrofyzika CEP GP205/09/P455 GA ČR - Grantová agentura ČR CEZ AV0Z10030501 - ASU-R (2005-2011) UT WOS 000283297300075 DOI https://doi.org/10.1051/0004-6361/201014281 Anotace Our 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). Pracoviště Astronomický ústav Kontakt Anežka Melichárková, bibl@asu.cas.cz, Tel.: 323 620 326 Rok sběru 2011
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