Earth, Moon, and Planets 102, 485–493 (2008)
DOI: 10.1007/s11038-007-9194-y
Analysis of a low density meteoroid with enhanced sodium
Jiri Borovicka, Pavel Koten, Pavel Spurny and
Rostislav Stork
Astronomical Institute of the Academy of
Sciences, Fricova 298, 25165 Ondrejov, Czech Republic
Abstract. We present an analysis of sporadic meteor number
07406018, observed by
image intensified video cameras at two stations, which showed a
pronounced deceleration along its trajectory. We have applied the
erosion model to analyze simultaneously the deceleration and light
curve. We have found that the meteoroid had a low density of about
500 kg m−3,
consistent with its cometary orbit. The meteoroid structure was,
nevertheless, markedly different from the Draconid meteoroids, studied
recently with the same model. The size of the constituent grains was
larger and the erosion energy was higher than in Draconids. The meteor
spectrum was also different from Draconid spectra and showed very
bright Na lines. The meteoroid composition was probably different from
normal cometary composition.
Keywords: meteors - meteoroids - comets -
composition
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