# Formation of Massive Rocky Exomoons by Giant Impact

## TL;DR

This paper proposes that giant impacts between rocky exoplanets can produce debris disks that may form large, detectable moons, highlighting impact velocity as a key factor in moon formation.

## Contribution

It introduces a new mechanism for exomoon formation via impact-generated debris disks, emphasizing the importance of impact velocity, which was previously overlooked.

## Key findings

- Collisions can produce massive debris disks capable of forming moons.
- Impacts onto 2-7 Earth-mass planets can create detectable exomoons.
- Impact velocity critically influences disk mass and moon formation potential.

## Abstract

The formation of satellites is thought to be a natural by-product of planet formation in our Solar System, and thus, moons of extrasolar planets (exomoons) may be abundant in extrasolar planetary systems, as well. Exomoons have yet to be discovered. However, moons larger than 0.1 Earth masses can be detected and characterized using current transit techniques. Here, we show that collisions between rocky planets with masses between a quarter to ten Earth masses can create impact-generated debris disks that could accrete into moons. Collisions between like-sized objects, at oblique impact angles, and velocities near escape speed create disks massive enough to form satellites that are dynamically stable against planetary tides. Impacts of this type onto a superearth between 2 to 7 Earth masses can launch into orbit enough mass to create a satellite large enough to be detected in Kepler transit data. Impact velocity is a crucial controlling factor on disk mass, which has been overlooked in all prior studies of moon formation via planetary collision.