Figure 1 from Formation of Close-in Super-Earths by Giant Impacts: Effects of Initial Eccentricities and Inclinations of Protoplanets

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Formation of Close-in Super-Earths by Giant Impacts: Effects of Initial Eccentricities and Inclinations of Protoplanets

Authors: Yuji Matsumoto and Eiichiro Kokubo

2017 The Astronomical Journal 154 27.

Provider: AAS Journals

Caption: Figure 1.

Typical orbital evolution of protoplanets in models N16e-3i-3.6 (a) and N16e-1i-3.6 (b). The time evolutions of the semimajor axes (red solid lines), and pericenter and apocenter distances (green dashed lines) are plotted.

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