  We analyze the effects of capture of dark matter (DM) particles, with
successive annihilations, predicted in the minimal walking technicolor model
(MWT) by the Sun and the Earth. We show that the Super-Kamiokande (SK) upper
limit on excessive muon flux disfavors the mass interval between 100-200 GeV
for MWT DM with a suppressed Standard Model interaction (due to a mixing
angle), and the mass interval between 0-1500 GeV for MWT DM without such
suppression, upon making the standard assumption about the value of the local
DM distribution. In the first case, the exclusion interval is found to be very
sensitive to the DM distribution parameters and can vanish at the extreme of
the acceptable values.
