The search for extra-solar planets has turned up some very interesting discoveries. Aside planets that are more-massive versions of their Solar counterparts (aka. Super-Jupiters and Super-Earths), there have been plenty of planets that straddle the line between classifications. And then there were times when follow-up observations have led to the discovery of multiple planetary systems.
This was certainly the case when it came to K2-18, a red dwarf star system located about 111 light-years from Earth in the constellation Leo. Using the ESO’s High Accuracy Radial Velocity Planet Searcher (HARPS), an international team of astronomers was recently examining a previously-discovered exoplanet in this system (K2-18b) when they noted the existence of a second exoplanet.
When K2-18b was first discovered in 2015, it was found to be orbiting within the star’s habitable zone (aka. “Goldilocks Zone“). The team responsible for the discovery also determined that given its distance from its star, K2-18b’s surface received similar amounts of radiation as Earth. However, the initial estimates of the planet’s size left astronomers uncertain as to whether the planet was a Super-Earth or a mini-Neptune.