Edited.
No if you talk about the escape velocity form Earth. This follows simply from the fact that energy EE is conserved. An object that is not gravitationally bound to Earth has E>0E>0 and hence v>vmathrmescv>vmathrmesc when hitting ground.
Yes, if you meant the escape velocity from the Solar system, because the Earth moves with vrmEarth=vrmescape/sqrt2vrmEarth=vrmescape/sqrt2 relative to (but not towards) the Sun. Here vrmescape=sqrt2GModot/1rmAUvrmescape=sqrt2GModot/1rmAU is the local escape speed from the Sun, while vrmEarth=sqrtGModot/1rmAUvrmEarth=sqrtGModot/1rmAU is the speed of the local circular orbit. An object at 1AU form the Sun and bound to the Sun cannot have speed greater than vrmescapevrmescape.
Now, the impact speed of an object that moves at vrmescapevrmescape can be as low vrmescape−vrmEarth=vrmescape(1−1/sqrt2)vrmescape−vrmEarth=vrmescape(1−1/sqrt2) if it hits Earth "from behind", i.e. moving in the same direction as Earth at the time of impact.
Note also that meterors typically move not faster than vrmescapevrmescape, for they don't come from outer space, but from the Solar system.
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