Image Details
Caption: Figure 1.
LTT 9779 b in context with the known population of transiting planets. In the period–mass and period–radius spaces, LTT 9779 b occupies a region which is sparsely populated. The majority of other planets on such a short orbital period are either stripped rocky cores or Jupiter-sized worlds.
© 2023. The Author(s). Published by the American Astronomical Society.