TOI-4602b is a 5.5 Earth-mass sub-Neptune with density 2.1 g/cm³ that retains a tenuous envelope and sits just above the radius valley, making it suitable for atmospheric characterization.
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The GAPS Programme at TNG. LXXIII. Confirmation of the hot sub-Neptune TOI-4602 b (HD 25295 b), a key target for future atmospheric characterization
TOI-4602b is a 5.5 Earth-mass sub-Neptune with density 2.1 g/cm³ that retains a tenuous envelope and sits just above the radius valley, making it suitable for atmospheric characterization.