Planetary Perturbers in Debris Disks

被引：0
|
作者：
Marc J. Kuchner
机构：
[1] Smithsonian Astrophysica1 Observatory,
来源：
Earth, Moon, and Planets | 2003年 / 92卷
关键词：
Recent Progress; Outer Edge; Planetary System; Eccentric Orbit; Kuiper Belt;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
Neptune dominates the dynamics of the Kuiper Belt. By examining images of debris disks around other stars, we may be able to infer what kinds of planets shape the outer edges of other planetary systems. The last few years have seen a burst of progress in the modeling of azimuthal structures in debris disks created by planetary perturbers; new models incorporate planets on substantially eccentric orbits. I review this recent progress in debris disk dynamics and discuss the Kuiper Belt as a key example.
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页码：435 / 445
页数：10
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