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Onset of oligarchic growth and implication for accretion histories of dwarf planets
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文摘

Oligarchic growth commences when the velocity dispersion relative to the largest body’s Hill velocity takes its minimum.

Planetary mass at the onset of oligarchic growth is close to the masses of the dwarf planets.

Size distribution of KBOs is reproduced if the initial planetesimal mass is 1021g.

Size distribution of asteroids is reproduced if initial planetesimals are very small and the asteroid seed mass is 1019g.

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