# Stellar Flybys Interrupting Planet-Planet Scattering Generates Oort Planets

## TL;DR

This paper proposes a new mechanism involving stellar flybys that can produce distant 'Oort' planets through planet-planet scattering interruption, supported by numerical simulations and efficiency analysis.

## Contribution

It introduces a novel process where stellar flybys halt planet scattering, leading to the formation of distant Oort-like planets, expanding understanding of wide-orbit exoplanets.

## Key findings

- Less than 1% of gas giants become Oort planets via this mechanism.
- Up to a few percent of Neptunes and super-Earths may become Oort planets.
- Numerical simulations support the efficiency of stellar flybys in creating Oort planets.

## Abstract

Wide-orbit exoplanets are starting to be detected, and planetary formation models are under development to understand their properties. We propose a population of "Oort" planets around other stars, forming by a mechanism analogous to how the Solar System's Oort cloud of comets was populated. Gravitational scattering among planets is inferred from the eccentricity distribution of gas-giant exoplanets measured by the Doppler technique. This scattering is thought to commence while the protoplanetary disk is dissipating, $10^6-10^7$ yr after formation of the star, or perhaps soon thereafter, when the majority of stars are expected to be part of a natal cluster. Previous calculations of planet-planet scattering around isolated stars have one or more planets spending $10^4-10^7$ yr at distances >100 AU before ultimately being ejected. During that time, a close flyby of another star in the cluster may dynamically lift the periastron of the planet, ending further scattering with the inner planets. We present numerical simulations demonstrating this mechanism as well as an analysis of the efficiency. We estimate an occurrence of planets between 100 and 5000 AU by this mechanism to be <1% for gas giants and up to a few percent for Neptunes and super-Earths.