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• W1635606138 abstract "The collision of Deep Impact with comet 9P/Tempel 1 generated a bright cloud of dust which dissipated during several days after the impact. The brightness variations of this cloud and the changes of its position and shape are governed by the physical properties of the dust grains. We use a Monte Carlo model to describe the evolution of the post-impact dust plume. The results of our dynamical simulations are compared to the data obtained with FORS2footnote{FORS stands for underline{FO}cal underline{R}educer and low dispersion underline{S}pectrograph for the underline{V}ery underline{L}arge underline{T}elescope (VLT) of the underline{E}uropean underline{S}outhern underline{O}bservatory (ESO).} to derive the particle size distribution and the total amount of material contained in the dust ejecta cloud." @default.
• W1635606138 created "2016-06-24" @default.
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• W1635606138 date "2008-10-17" @default.
• W1635606138 modified "2023-09-24" @default.
• W1635606138 title "Dynamical Modeling of the Deep Impact Dust Ejecta Cloud" @default.
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• W1635606138 doi "https://doi.org/10.1007/978-3-540-76959-0_22" @default.
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