  In this article, a new family of asymptotically flat wormhole solutions in
the context of symmetric teleparallel gravity, i.e., $f(Q)$ theory of gravity,
are presented. Considering a power-law shape function and some different forms
for $f(Q)$ function, we show that a wide variety of wormhole solutions for
which the matter fields satisfy some energy conditions, are accessible. We
explore that the presence of $f(Q)$ gravity will be enough to sustain a
traversable wormhole without exotic matter. The influence of free parameters in
shape function and $f(Q)$ models on the energy conditions is investigated. The
equation of state and boundary conditions are analyzed.
