  A possibility is discussed for experimental testing of the dark matter model
supported by a classic non-Abelian SU(3) gauge (Yang-Mills) field. Our approach
is based on the analysis of the motion of color-charged particles on the
background of color electric and magnetic fields using the Wong equations.
Estimating the magnitudes of the color fields near the edge of a galaxy, we
employ them in obtaining the general analytic solutions to the Wong equations.
Using the latter, we calculate the magnitude of the extra acceleration of
color-charged particles related to the possible presence of the color fields in
the neighbourhood of the Earth.
