  We show that the Higgsplosion mechanism makes a prediction for the mass and
coupling of a WIMP-like minimal scalar dark matter model. In particular the
currently favoured minimal value for the Higgsplosion scale, $E_\mathrm{H}\sim
25$ TeV, implies a dark matter mass $m_\mathrm{DM} \sim 1.25$ TeV and a
moderate quartic coupling with the Standard Model Higgs field
$\lambda_\mathrm{H,DM} \sim 0.4$. This point in the parameter space is still
allowed by all current experimental bounds, including direct detection (XENON),
indirect detection (HESS, Fermi, Planck) and collider searches. We have updated
the scalar dark matter bounds to reflect the latest results from XENON and HESS
experiments. We also comment on vacuum stability and dark matter
self-interactions in this model.
