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Oligarchic growth is the second-to-last stage in the formation of terrestrial planets and giant planet cores. During this stage, the largest planetary embryos grow quickly while the smallest grow slowly, leading to a bifurcated mass distribution with a number of lunar- to Mars-mass embryos embedded in a swarm of smaller planetesimals. Oligarchic growth transitions to chaotic growth when the planetary embryos become large enough to overcome eccentricity damping due to dynamical friction from smaller planetesimals. This leads to embryo–embryo collisions and signals the last stage of accretion of terrestrial planets and giant planet cores.
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© 2014 Springer-Verlag Berlin Heidelberg
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Mandell, A.M. (2014). Oligarchic Growth. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_1102-4
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DOI: https://doi.org/10.1007/978-3-642-27833-4_1102-4
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Publisher Name: Springer, Berlin, Heidelberg
Online ISBN: 978-3-642-27833-4
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