  Most stars form as part of a stellar group. These young stars are mostly
surrounded by a disk from which potentially a planetary system might form.
Both, the disk and later on the planetary system, may be affected by the
cluster environment due to close fly-bys. The here presented database can be
used to determine the gravitational effect of such fly-bys on non-viscous disks
and planetary systems. The database contains data for fly-by scenarios spanning
mass ratios between the perturber and host star from 0.3 to 50.0, periastron
distances from 30 au to 1000 au, orbital inclination from $0^{\circ}$ to
${180^\circ}$ and angle of periastron of $0^{\circ}$, ${45^\circ}$ and
${90^\circ}$. Thus covering a wide parameter space relevant for fly-bys in
stellar clusters. The data can either be downloaded to perform one's own
diagnostics like for e.g. determining disk size, disk mass, etc. after specific
encounters, obtain parameter dependencies or the different particle properties
can be visualized interactively. Currently the database is restricted to
fly-bys on parabolic orbits, but it will be extended to hyperbolic orbits in
the future. All of the data from this extensive parameter study is now publicly
available as DESTINY.
