The Formation and Dynamics of Super-Earth Planets

TL;DR

This paper reviews the current understanding of how super-Earth planets form and evolve dynamically, highlighting their significance in exoplanet research and potential habitability.

Contribution

It provides a comprehensive overview of models and recent discoveries related to super-Earth formation and evolution.

Findings

Super-Earths can retain atmospheres and possibly support plate tectonics.

Recent discoveries suggest some super-Earths are potentially habitable.

Understanding formation models is crucial for interpreting exoplanet observations.

Abstract

Super-Earths, objects slightly larger than Earth and slightly smaller than Uranus, have found a special place in exoplanetary science. As a new class of planetary bodies, these objects have challenged models of planet formation at both ends of the spectrum and have triggered a great deal of research on the composition and interior dynamics of rocky planets in connection to their masses and radii. Being relatively easier to detect than an Earth-sized planet at 1 AU around a G star, super-Earths have become the focus of worldwide observational campaigns to search for habitable planets. With a range of masses that allows these objects to retain moderate atmospheres and perhaps even plate tectonics, super-Earths may be habitable if they maintain long-term orbits in the habitable zones of their host stars. Given that in the past two years a few such potentially habitable super-Earths have in fact been discovered, it is necessary to develop a deep understanding of the formation and dynamical evolution of these objects. This article reviews the current state of research on the formation of super-Earths and discusses different models of their formation and dynamical evolution.