There are 5,599 confirmed exoplanets in 4,163 star systems and 10,157 candidates awaiting confirmation.
Most have been identified indirectly using Transit Photometry (74.4%) and Radial Velocity measurements (19.4%).
Only nineteen (1.2%) were identified via Direct Imaging, which uses light reflected from an exoplanet's atmosphere or surface to detect and characterize it.
New high-contrast and high-angular resolution tools are changing this.
This includes the James Webb Space Telescope's upgraded mirrors and infrared imaging equipment.
The MIRI mid-INfrared Disk Survey (MINDS) recently analyzed a very young variable star (PDS 70) 370 light-years away with two verified protoplanets using Webb's Near-Infrared Camera (NIRCam) data.
The system and its extended debris disk revealed a third putative protoplanet orbiting the star.
These observations may improve our knowledge of planetary systems in formation.