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Properties of small meteoroids studied by meteor video observations

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    0517163 - ASÚ 2020 RIV FR eng J - Článek v odborném periodiku
    Vojáček, Vlastimil - Borovička, Jiří - Koten, Pavel - Spurný, Pavel - Štork, Rostislav
    Properties of small meteoroids studied by meteor video observations.
    Astronomy & Astrophysics. Roč. 621, January (2019), č. článku A68. ISSN 0004-6361. E-ISSN 1432-0746
    Grant CEP: GA ČR(CZ) GA16-00761S
    Institucionální podpora: RVO:67985815
    Klíčová slova: meteorites * meteors * meteoroids
    Obor OECD: Astronomy (including astrophysics,space science)
    Impakt faktor: 5.636, rok: 2019
    Způsob publikování: Open access

    he complex study of millimetre-sized meteoroids can reveal more about the structure and origin of population of these meteoroids. The variety of properties among millimetre-sized meteoroids proved different sources and histories of this material. Meteoroids that contain small grains tend to release their sodium early. For given grain sizes, the sodium in Na-poor meteoroids is released earlier than in meteors without sodium depletion. Overall, meteoroids with sodium depletion are revealed to have different structures: they have stronger material without very small grains and they do not show very bright wakes. Two iron meteoroids on Halley-type orbits were observed, thereby supporting the idea of large-scale mixing of material in the early solar system. The distribution of grain sizes of Jupiter-family members was in good agreement with results from the COSIMA instrument on the ROSETTA probe.
    Trvalý link: http://hdl.handle.net/11104/0302450

     
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