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• W2770279397 abstract "$mathit{Context.}$ The thermal conductivity of highly porous dust aggregates is a key parameter for many subjects in planetary science; however, it is not yet fully understood. $mathit{Aims.}$ In this study, we investigate the thermal conductivity of fluffy dust aggregates with filling factors of less than $10^{-1}$. $mathit{Methods.}$ We determine the temperature structure and heat flux of the porous dust aggregates calculated by $N$-body simulations of static compression in the periodic boundary condition. $mathit{Results.}$ We derive an empirical formula for the thermal conductivity through the solid network $k_{rm sol}$ as a function of the filling factor of dust aggregates $phi$. The results reveal that $k_{rm sol}$ is approximately proportional to ${phi}^{2}$, and the thermal conductivity through the solid network is significantly lower than previously assumed. In light of these findings, we must reconsider the thermal histories of small planetary bodies." @default.
• W2770279397 created "2017-12-04" @default.
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• W2770279397 date "2017-12-01" @default.
• W2770279397 modified "2023-10-13" @default.
• W2770279397 title "Thermal conductivity of porous aggregates" @default.
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• W2770279397 doi "https://doi.org/10.1051/0004-6361/201732182" @default.
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