The Expected Yield of Venus Zone Terrestrial Planets from PLATO

The characterization of terrestrial exoplanets and the conditions that lead to divergent climate outcomes is a primary goal of exoplanetary science. The Venus Zone (VZ) provides a framework for identifying planets that may have experienced runaway greenhouse processes similar to Venus, and the statistical properties of such planets bear directly on models of planetary habitability. Here we present a quantitative estimate of the expected yield of VZ terrestrial planets from ESA's PLATO (PLAnetary Transits and Oscillations of stars) mission. We combine the predicted PLATO planet yield for Earth-size ($0.8$--$1.25~R_\oplus$) and super-Earth ($1.25$--$2.0~R_\oplus$) planets with empirical occurrence rates for VZ terrestrial planets derived from Kepler data. Under conservative assumptions, we estimate that PLATO will detect $\sim$170--280 VZ terrestrial planets ($0.8$--$2.0~R_\oplus$), including $\sim$40--80 Earth-size ($0.8$--$1.25~R_\oplus$) planets, during a nominal 4-year mission. For the bright P1 sample ($V \leq 11$), we estimate $\sim$50--85 terrestrial and $\sim$13--22 Earth-size VZ detections, enabling radial velocity mass determination and atmospheric characterization of the most favorable targets with JWST and future facilities. We discuss the implications of this yield for comparative studies of Earth-Venus divergence, synergies with the DAVINCI, VERITAS, and EnVision missions to Venus, and the role of PLATO in advancing our understanding of the runaway greenhouse boundary.