If you were dreaming of moons made of cheese and cotton candy exoplanets, you may have to dream a little harder. “Super-puffs,” a strange class of exoplanets whose oblong appearance suggested they must have the density of cotton candy to exist, may have a slightly more complicated reality. New calculations, published late February in The Astronomical Journal, suggest the shape of such planets could be explained if they actually had rings.
Saturn Did it First
In our solar system, all gas and ice giant planets, like Saturn, have rings. But finding ringed exoplanets in other solar systems has proven surprisingly difficult. Measuring exoplanets’ radii is done in transit – that is, when a planet crosses in front of its star relative to Earth, the path dims the light of its star enough to be measured.
“We started to wonder, if you were to look back at us from a distant world, would you recognize Saturn as a ringed planet, or would it appear to be a puffy planet to an alien astronomer?” Shreyas Vissapragada, a researcher from the California Institute of Technology asked in a press release.
To test the theory, Vissapragada and team simulated what a ringed exoplanet would like in in transit to an astronomer at a distance, and how the material of the rings would affect its appearance. Their work determined the presence of rocky rings could explain some strange super-puffs, but not all of them. Unfortunately, following up on their simulations will require waiting for the launch of NASA’s heavily delayed James Web Telescope, assuming it launches next year.
READ MORE: What if mysterious ‘cotton candy’ planets actually sport rings? [Phys.org]
More on Super-puffs: These Rare Exoplanets Have the “Density of Cotton Candy”