Exoplanets have been detected since 1992 when two, named named Poltergeist and Phobetor, were found orbiting the pulsar PSR B1257+12. Thousands have been detected indirectly but because they are less bright due to being 'drowned out' by light from their star, direct observation is a challenge. So the two most common methods of detection look for its effect rather than direct viewing. TWA 7 from the Very Large Telescope’s SPHERE instrument with an image from JWST’s MIRI overlayed reveals the empty area around TWA 7 B in the R2 ring (CC #1). The new planet is comparable in size to Saturn, but that is 10 times lighter than those captured in previous images, and has been named TWA 7 b.