The possibility of equilibrium of test particles with spin located in the S
chwarzschild-de Sitter spacetimes is investigated. The stationary equilibri
um conditions resulting from the equations of motion and the equations of s
pin dynamics have to be satisfied simultaneously. It is shown that the equi
librium conditions are independent of the spin of the test particles; they
are satisfied only at the so called static radius where the gravitational a
ttraction is compensated by the cosmological repulsion.