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Characterization of the Compact Multiplanet System TOI-789: Validation of Three Terrestrial Planets, Dynamical Characterization, and Detection of a Fourth Temperate Candidate

  • Authors: Juan F. Pagés Navarrete

Juan F. Pagés Navarrete 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 8.

Top-down, to-scale view of the TOI-789 architecture. The four planetary orbits are drawn around the M3 host (center); symbol size scales with planetary radius and symbol color with equilibrium temperature (color bar). The candidate .04 is drawn with a dashed outline. Shaded annular bands mark, from the inside out, the Venus zone (S. R. Kane et al. 2014), the temperate region defined by Teq = 273–400 K, and the inner edge of the R. K. Kopparapu et al. (2014) habitable zone. The four planets form a sequence of decreasing insolation that crosses the Venus zone, with the candidate .04 near the inner edge of the habitable zone.

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