  Over these past few years several quantum-gravity research groups have been
exploring the possibility that in some Planck-scale nonclassical descriptions
of spacetime one or another form of nonclassical spacetime symmetries might
arise. One of the most studied scenarios is based on the use of Hopf algebras,
but previous attempts were not successful in deriving constructively the
properties of the conserved charges one would like to obtain from the Hopf
structure, and this in turn did not allow a crisp physical characterization of
the new concept of spacetime symmetry. Working within the example of
$\kappa$-Minkowski noncommutative spacetime, known to be particularly
troublesome from this perspective, we observe that these past failures in the
search of the charges originated from not recognizing the crucial role that the
noncommutative differential calculus plays in the symmetry analysis. We show
that, if the properties of the $\kappa$-Minkowski differential calculus are
correctly taken into account, one can easily perform all the steps of the
Noether analysis and obtain an explicit formula relating fields and
energy-momentum charges. Our derivation also exposes the fact that an apparent
source of physical ambiguity in the description of the Hopf-algebra rules of
action, which was much emphasized in the literature, actually only amounts to a
choice of conventions and in particular does not affect the formulas for the
charges.
