An article published in the journal “Monthly Notices of the Royal Astronomical Society” reports the discovery of an exoplanet belonging to the mini-Neptune class in an orbit close to its star, where a planet of that type should not exist, so much that it’s called Neptunian Desert. A team of astronomers coordinated by the University of Warwick used the Next-Generation Transit Survey (NGTS) array in Chile to locate the exoplanet, which was therefore cataloged as NGTS-4b. It may have got closer to its star or was originally larger but part of its atmosphere was consumed by stellar radiation.