  Non-annihilating dark matter particles, owing to their interactions with
ordinary baryonic matter, can efficiently accumulate inside celestial objects.
For heavy mass, they gravitate toward the core of the celestial objects,
thermalize in a small core region, and eventually form tiny black holes via
core collapse, resulting destruction of the host objects. We demonstrate that
the existence of a variety of celestial objects provides stringent constraints
on strongly-interacting heavy dark matter, a blind-spot for the terrestrial
dark matter detectors as well as for the cosmological probes. Celestial objects
with larger sizes and lower core temperatures, such as Jupiter, are the most
optimal detectors to probe the strongly-interacting heavy non-annihilating dark
matter.
