The extended phase space of an elementary (relativistic) system is int
roduced in the spirit of Souriau's definition of the 'space of motions
' for such a system. Our 'modification' consists in taking into accoun
t not only the symmetry (Poincare) group but also its action on the (M
inkowski) spacetime, i.e. the full covariant system. This yields a gen
eral procedure to construct spaces in which the equations of motion ca
n be formulated: phase trajectories of the system are identified as ch
aracteristics on some constraint submanifold ('mass and spin shell') i
n the extended phase space. Our formulation is generally applicable to
any homogeneous spacetime (e.g, de Sitter) and also to Poisson action
s. Calculations concerning the Minkowski case for non-zero spin partic
les show an intriguing alternative: we should either accept two-dimens
ional trajectories or (Poisson) non-commuting spacetime coordinates.