TOI-2266.01 Archives

TOI-2266 b’s location in the period-radius plane with the currently known planets orbiting M dwarfs. The planets without sufficiently precise density estimates are shown as grey crosses (From exoplanet.eu, accessed 2023 April 24), while the planets with well-constrained densities from the catalogue by Luque & Pallé (2022) are separated by their likely type: rocky planets are shown as black dots, water worlds as blue circles, and sub-Neptunes as green circles. The upper radius limits for rocky planets for the gas-depleted formation and thermally-driven mass loss scenarios are drawn as dashed lines. -- astro-ph.EP

TOI-2266 b: A Keystone Super-Earth At The Edge Of The M dwarf Radius Valley

by Keith CowingJanuary 24, 2024January 23, 2024

We validate the Transiting Exoplanet Survey Satellite (TESS) object of interest TOI-2266.01 (TIC 348911) as a small transiting planet (most likely a super-Earth) orbiting a faint M5 dwarf (V=16.54) on […]

TOI-2266.01

TOI-2266 b: A Keystone Super-Earth At The Edge Of The M dwarf Radius Valley

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