  Spherically symmetric solutions for f(T) gravity models are derived by the so
called Noether Symmetry Approach. First, we present a full set of Noether
symmetries for some minisuperspace models. Then, we compute analytical
solutions and find that spherically symmetric solutions in f(T) gravity can be
recast in terms of Schwarzschild-like solutions modified by a distortion
function depending on a characteristic radius. The obtained solutions are more
general than those obtained by the usual solution methods.
