  We calculate accretion mass of interstellar objects (ISOs) like `Oumuamua
onto low-mass population III stars (Pop.~III survivors), and estimate surface
pollution of Pop.~III survivors. An ISO number density estimated from the
discovery of `Oumuamua is so high ($\sim 0.2$~au$^{-3}$) that Pop.~III
survivors have chances at colliding with ISOs $\gtrsim 10^5$ times per $1$~Gyr.
`Oumuamua itself would be sublimated near Pop.~III survivors, since it has
small size, $\sim 100$~m. However, ISOs with size $\gtrsim 3$~km would reach
the Pop.~III survivor surfaces. Supposing an ISO cumulative number density with
size larger than $D$ is $n \propto D^{-\alpha}$, Pop.~III survivors can accrete
ISO mass $\gtrsim 10^{-16}M_\odot$, or ISO iron mass $\gtrsim 10^{-17}M_\odot$,
if $\alpha < 4$. This iron mass is larger than the accretion mass of
interstellar medium (ISM) by several orders of magnitude. Taking into account
material mixing in a convection zone of Pop.~III survivors, we obtain their
surface pollution is typically [Fe/H] $\lesssim -8$ in most cases, however the
surface pollution of Pop.~III survivors with $0.8M_\odot$ can be [Fe/H]
$\gtrsim -6$ because of the very shallow convective layer. If we apply to
Pop.III survivors located at the Galactocentric distance of 8 kpc, the
dependence of the metal pollustion is as follows. If $\alpha > 4$, Pop.~III
survivors have no chance at colliding with ISOs with $D \gtrsim 3$~km, and keep
metal-free. If $3 < \alpha < 4$, Pop.~III survivors would be most polluted by
ISOs up to [Fe/H] $\sim -7$. If $\alpha < 3$ up to $D \sim 10$~km, Pop.~III
survivors could hide in metal-poor stars so far discovered. Pop.~III survivors
would be more polluted with decreasing the Galactocentric distance. Although
the metal pollution depends on $\alpha$ and the Galactocentric distance, we
first show the importance of ISOs for the metal pollution of Pop.~III
survivors.
