  We study the kinematic relative velocity of general test particles with
respect to stationary observers (using spherical coordinates) in Schwarzschild
spacetime, obtaining that its modulus does not depend on the observer, unlike
Fermi, spectroscopic and astrometric relative velocities. We study some
fundamental particular cases, generalizing some results given in other work
about stationary and radial free-falling test particles. Moreover, we give a
new result about test particles with circular geodesic orbits: the modulus of
their kinematic relative velocity with respect to any stationary observer
depends only on the radius of the circular orbit, and so, it remains constant.
