Image Details
Caption: Figure 15.
Mass–metallicity diagram for sub-Saturn-sized planets (R p = 4–8 R ⊕) from Figure 12, including TOI-4010c and d. This population shows a tentative positive correlation between mass and host-star metallicity. TOI-4010 d is one of the most massive sub-Saturns discovered in a multiplanet system. TOI-4010 follows the general trend of more massive sub-Saturns orbiting higher-metallicity stars.
© 2023. The Author(s). Published by the American Astronomical Society.