Sandwiched planet formation: restricting the mass of a middle planet
Matthew Pritchard, Farzana Meru, Sahl Rowther, David Armstrong and, Kaleb Randall

TL;DR
This paper uses hydrodynamical simulations to show how a second outer planet can limit the growth of an inner planet, potentially leading to a 'sandwiched' smaller planet between two larger ones, challenging typical planet formation trends.
Contribution
It introduces a new model explaining the formation of smaller middle planets between larger neighbors due to pressure profile effects in protoplanetary discs.
Findings
Outer planets influence inner planet's material accumulation.
Sandwiched smaller planets can form between larger planets.
Observed planetary systems support the model.
Abstract
We conduct gas and dust hydrodynamical simulations of protoplanetary discs with one and two embedded planets to determine the impact that a second planet located further out in the disc has on the potential for subsequent planet formation in the region locally exterior to the inner planet. We show how the presence of a second planet has a strong influence on the collection of solid material near the inner planet, particularly when the outer planet is massive enough to generate a maximum in the disc's pressure profile. This effect in general acts to reduce the amount of material that can collect in a pressure bump generated by the inner planet. When viewing the inner pressure bump as a location for potential subsequent planet formation of a third planet, we therefore expect that the mass of such a planet will be smaller than it would be in the case without the outer planet, resulting in…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Astro and Planetary Science · Molecular Spectroscopy and Structure
