T. A. Plattner, I. Mishra, S. Banerjee, and 16 more authors
Ceres, the largest object in the asteroid belt, is a relict ocean world with recent geological activity, including water vapor and bright evaporite deposits linked to simple organics. We propose a lander mission to investigate Ceres’ exosphere, subsurface, organics, and astrobiological potential. Key objectives include determining the source of water vapor, assessing interior hydrothermal processes, evaluating the origin of complex organics, and analyzing evaporite deposits for life-essential elements. A suite of instruments—including a UV imaging spectrometer, GC-MS, X-ray spectrometer, magnetotelluric sounder, and cameras—would enable orbital and in-situ studies. Launch in the early 2030s would allow 11 months of orbital reconnaissance and 1 month of landed operations, providing unprecedented insights into Ceres and ocean worlds more broadly.