  The Kuiper belt objects (KBOs) exhibit an orbital clustering of the outer
planets lying at perihelion distances larger than Neptune and semimajor axes
greater than 150 AU from the Sun. This implies a hitherto unknown dynamical
mechanism to counter randomizing of the orbital elements caused by the giant
solar system planets. Using the toroidal field induced frame-dragging we deduce
here the observed range of the Kuiper belt region, the semi-major axis of Sedna
like objects in the Kuiper belt, as well as the orbital clustering of the KBOs
in the ecliptic, without assuming dynamical effects induced by
trans-Neptunian-objects (TNOs). We also calculate the orbital precession rates
for the inner planets and show their correspondence, within the range of
observational accuracy, with recent planetary ephemerides.
