This synthesis highlights the research efforts in micro black holes in recent years and points to future prospects. Synthesizing recently published articles shows that micro black holes can have a variety of properties. This paper explores articles discussing the instantaneous evaporation of micro black holes due to Hawking Radiation, the inability of a micro black hole to accrete matter, the intense recoil effects that occur if a micro black hole absorbs matter, the stability of micro black holes, as well as the spin and electric charge they may possess. Modern methods of detecting black holes have been described as looking for specific particle signatures that match a predicted profile of Hawking Radiation from a micro black hole and looking for possible signs of a micro black hole remnant. Expectations suggest that planned future projects will aid in the search for micro black holes by taking advantage of high-energy cosmic particle collisions.