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\title{\bf TAURID METEOROID AND ASTEROID COMPLEX}
\author{Eduard M. Pittich$^{1}$ and Jozef Kla\v cka$^{2}$}
\date{
$^{1}$Astronomical Institute of the Slovak Academy of Sciences\\
D\'ubravsk\'a cesta 9, 842 28 Bratislava, Slovak Republic\\
E-mail: pittich@savba.sk\\[0.2cm]
$^{2}$Department of Astronomy and Astrophysics,
Faculty for Mathematics and Physics\\
Comenius University, Mlynsk\'{a} dolina, 842~15 Bratislava, Slovak Republic\\
E-mail: klacka@fmh.uniba.sk\\
}
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Origin of the Taurid meteor stream is investigated on the basis
of an assumption that the complete set of observable quantities may
be explained as a simultaneous action of nongravitational forces
acting on meteoroids ejected from the parent body represented only
by comet P/Encke. 

Discussion is concentrated on the problem if
the assumption about the importance of nongravitational forces
is acceptable. Numerical values for nongravitational acceleration
are found out. Time evolution from 10, 000 to 15,000 years is considered
and graphically presented.


The test is made for dust particles ejected at perihelia of the orbit of the
comet Encke. The particles are released at the speed of 40 m\,s$^{-1}$.
Gravitational perturbations of all planets and nongravitational effects
are considered. 
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