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Macroscopic dark matter (macros) are a broad class of alternative candidatesto particle dark matter. These candidates would transfer energy primarilythrough elastic scattering, and this linear energy deposition would produceobservable signals if a macro were to pass through the atmosphere. We produceconstraints for low mass macros from the null observation of bolides formed bya passing macro, across two extensive networks of cameras built originally toobserve meteorites. The parameter space that could be probed with plannedupgrades to the existing array of cameras in one of these networks stillcurrently in use, the Desert Fireball Network in Australia, is estimated.

Macroscopic Dark Matter Constraints from Bolide Camera Networks