Meteoritics & Planetary Science 38, 1005--1021 (2003)
The Moravka meteorite fall:
3. Meteoroid initial size, history, structure and composition
J. Borovicka1, H.W. Weber2, T. Jopek3,
P. Jakes4, Z. Randa5, P.G. Brown6,
D.O. ReVelle7, P. Kalenda8, L. Schultz2,
J. Kucera5, J. Haloda4, P. Tycova4, J.
Fryda9, and F. Brandstatter10
1Astronomical Institute of the Academy of Sciences,
25165 Ondrejov, The Czech Republic
2Max-Plank-Institut für Chemie, Joh. J.-Becher-Weg 27,
D-55128 Mainz, Germany
3Astronomical Observatory of A.Mickiewicz University,
Sloneczna 36, 60286 Poznan, Poland
4Institute of Geochemistry, Mineralogy and Mineral
Resources, Faculty of Science, Charles University, Albertov 6, 12843
Prague 2, The Czech Republic
5Nuclear Physics Institute, Academy of Sciences, 25068 Rez
near Prague, The Czech Republic
6Department of Physics and Astronomy, University of Western
Ontario, London, Ontario N6A 3K7, Canada
7Los Alamos National Laboratory, P.O. Box 1663, MS J557, Los
Alamos, New Mexico 87545, USA
8CoalExp, Kosmonautu 2, 70030 Ostrava 3, The Czech Republic
9Czech Geological Survey, Geologicka 6, 15200 Prague 5, The
Czech Republic
10Department of Mineralogy and Petrography, Museum of
Natural History, Burgring 7, A-1010 Vienna, Austria
Abstract. The properties and history of the parent meteoroid of
the Morávka H5-6 ordinary chondrites have been studied by a
combination of various methods. The pre-atmospheric mass of the
meteoroid was computed from fireball radiation, infrasound, seismic
signal and the content of noble gases in the meteorites. All methods
gave consistent results. The best estimate of the pre-atmospheric mass
is (1500 ± 500) kg. The fireball integral bolometric luminous
efficiency was 9% and the acoustic efficiency was 0.14%. The meteoroid
cosmic ray exposure age was determined to be (6.7 ± 1.0) x 106
years. The meteorite shows a clear deficit of helium, both 3He
and 4He. This deficit can be explained by solar heating.
Numerical backward integration of the meteoroid orbit (determined in a
previous paper from video records of the fireball) shows that the
perihelion distance was probably lower than 0.5 AU and possibly as low
as 0.1 AU five million years ago. The collision which excavated
Morávka probably occurred while the parent body was on a
near-Earth orbit, as opposed to being confined entirely to the main
asteroid belt. An overview of meteorite macroscopic properties,
petrology, mineralogy and chemical composition is given. The meteorites
show all mineralogical features of H chondrites. The shock level is S2.
Minor deviations from other H chondrites in abundances of trace
elements La, Ce, Cs, and Rb were found. The ablation crust is enriched
with siderophile elements.
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