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- W2953906191 abstract "The Rosetta space mission included three main instruments for solid dust particle analysis. The combined microscope and mass spectrometer COSIMA (Cometary Secondary Ion Mass Analyser) [1], the atomic force microscope MIDAS (Micro-Imaging Dust Analysis System) [2], and the impact detector GIADA (Grain Impact Analyser and Dust Accumulator) [3]. These three instruments provide complementary insights into dust particles properties over a wide range of sizes/masses (10nm to 1mm). GIADA and MIDAS observed a major contribution from compact dust particles together with a population of porous particles with a low fractal dimension (Df~1,7 for MIDAS [4]) [5, 6]. The fractal dust component of the nucleus and its properties give constraints on the formation of comets in the early solar system [5].In this work, we analyseresults from a simple numerical model of dust aggregates compactionto assess the initial physical properties of the dust populations." @default.
- W2953906191 created "2019-07-12" @default.
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- W2953906191 date "2018-03-19" @default.
- W2953906191 modified "2023-09-27" @default.
- W2953906191 title "Compacted loose particles from numerical simulations compared to Rosetta collected particles" @default.
- W2953906191 hasPublicationYear "2018" @default.
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