  We present an approach to finding distances to young supernova remnants. Our
method is based on hydrodynamical simulations of Tycho's SNR using the SUPREMNA
code. For the explosion models, we use the classical W7 deflagration model and
the delayed detonation model that was previously shown to provide good fits to
the X-ray emission of Tycho's SNR. Combining our hydrodynamical simulations
with the Chandra high-resolution images of the remnant obtained in 2015, we
derive a distance estimate to Tycho's SNR of $2.8\pm 0.4$ kpc.
