  The CRESST-II collaboration have announced evidence for the direct detection
of dark matter in 730 kg-days exposure of a CaWO$_4$ target. We examine these
new results, along with DAMA and CoGeNT data, in the context of the mirror dark
matter framework. We show that all three experiments can be simultaneously
explained via kinetic mixing induced elastic scattering of a mirror metal
component off target nuclei. This metal component can be as heavy as Fe$'$ if
the galactic rotational velocity is relatively low: $v_{rot} \stackrel{<}{\sim}
220$ km/s. This explanation is consistent with the constraints from the other
experiments, such as CDMS/Ge, CDMS/Si and XENON100 when modest $\sim 20-30%$
uncertainties in energy scale are considered.
