The discovery of TOI-6894b — an exoplanet around 86% the size of Jupiter in orbit around a 0.2-solar-mass red dwarf — highlights the need for a better understanding of giant planet formation mechanisms and the protoplanetary disk environments in which they occur. An artist’s illustration of TOI-6894b behind its host star. Image credit: Mark Garlick / University of Warwick. The TOI-6894 system is located approximately 73 parsecs (238...
