NASA-Funded Project Shares Theory On Missing Planets That Are 2-3 Times Bigger Than Earth
As scientists and astronomers investigate the universe, two mysteries seem to keep popping up. The first is known as the "radius valley," which refers to the rarity of exoplanets with a radius of around 1.8 times that of Earth. The second mystery, known as "peas in a pod," is in reference to neighboring planets of similar size that have been detected in hundreds of planetary systems. However, a team at Rice's NASA-funded CLEVER Planets project believes they may have created a model that solves these two riddles.
"I believe we are the first to explain the radius valley using a model of planet formation and dynamical evolution that self-consistently accounts for multiple constraints of observations," remarked Andre Izidoro, corresponding author of a study published in Astrophysical Journal Letters this week. "We're also able to show that a planet-formation model incorporating giant impacts is consistent with the peas-in-a-pod feature of exoplanets."

"The migration of young planets towards their host stars creates overcrowding and frequently results in cataclysmic collisions that strip planets of their hydrogen-rich atmospheres," explains Izidoro. "That means giant impacts, like the one that formed our moon, are probably a generic outcome of planet formation."

Now that the team has made its findings available, the predictions can be tested by NASA's James Webb Space Telescope (JWST). If the findings hold true, the team suggests that a fraction of planets about twice that of Earth's size will both retain their primordial hydrogen-rich atmosphere and be rich in water.