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- W2024163154 abstract "Abstract The formation conditions of the binary system Pluto-Charon in the protoplanetary disk are analyzed. Particular attention is paid to its high content of angular momentum that would make the system rotationally unstable in the ideal case that Pluto and Charon coalesced into a single body. Among several possible formation scenarios, the acquisition of such a large amount of angular momentum is explained as the result of the accumulation process of planetesimals in heliocentric orbits with masses up to a few tenths of the mass of the proto-Pluto itself. Numerical simulations of accreting planetesimals show that a significant fraction (5–20%) of the Pluto-sized bodies formed reach rotational instability. Under these circumstances, the Pluto-Charon system may have already formed before it acquired its highly eccentric and inclined orbit." @default.
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- W2024163154 date "1991-10-01" @default.
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- W2024163154 title "The angular momentum of the Pluto-Charon system: considerations about its origin" @default.
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- W2024163154 doi "https://doi.org/10.1016/0019-1035(91)90214-e" @default.
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