Summary:
- This article discusses a new model developed by researchers at the Southwest Research Institute (SwRI) that helps explain the formation of exoplanetary systems with compact orbits.
- The model suggests that these compact exoplanetary systems may have formed from the gravitational collapse of a rotating cloud of gas and dust, similar to how our own solar system formed.
- The model provides insights into the diverse range of exoplanetary systems observed by astronomers, and helps to shed light on the processes that shape the formation and evolution of planetary systems beyond our own.