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Published online by Cambridge University Press: 12 April 2016
There are three factors that inhibit detecting small comets relative to large comets: 1. They must pass closer to the Earth than large comets to be detected. 2. The resulting higher angular velocity for nearby comets means that, at comparable apparent magnitudes, there is less time available to discover a small comet relative to a large comet. 3. Small comets physically decay and vanish faster than do large comets. With these three factors, it can be shown that if the small comet input distribution gi (Rn) in varies as , where Rn is the nuclear radius of the comet, then the observed distribution will vary as