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Abstract
Abstract We present the results of a long-term telescopic observation campaign of comet 21P/Giacobini–Zinner, parent body of the Draconid meteor shower, spanning ∼240 days during its 2018 apparition. Determinations of comet 21P’s dust production rate through the Afρ parameter derived from these images show that the comet had a highly asymmetric dust production rate that peaked ∼10–30 days before perihelion, when the comet was at a heliocentric distance of ∼1.02–1.08 au. The single highest Afρ measurement occurred on 2018 August 14 (27 days before perihelion), and had a measured value of Afρ = 1594 cm. The comet’s Afρ profile is well described by a double-exponential model that rises rapidly during ingress and declines even more rapidly during its egress. These results are fully consistent with observations of comet 21P’s dust and gas production rates during past apparitions, and suggest that the double-exponential model we have derived provides a reasonable and stable approximation for the comet’s activity over the past 30 to 40 years.
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