An unusually low-density super-Earth transiting the bright early-type M-dwarf GJ 1018 (TOI-244)
Deleuil, M.; Zapatero Osorio, M. R.; Allende Prieto, C.; Palle, E.; Winn, J. N.; Cristiani, S.; Sozzetti, A.; Adibekyan, V.; Alibert, Y.; Sousa, S. G.; Barros, S. C. C.; Bonfils, X.; Demangeon, O. D. S.; Jenkins, J. M.; Lovis, C.; Seager, S.; Borsa, F.; Pepe, F.; Lillo-Box, J.; Di Marcantonio, P.; Figueira, P.; González Hernández, J. I.; Martins, C. J. A. P.; Nunes, N. J.; Suárez Mascareño, A.; Damasso, M.; Tabernero, H. M.; Astudillo-Defru, N.; Lavie, B.; Acuña, L.; Silva, A. M.; Castro-González, A.; Santos, N.; Davoult, J.; Aguichine, A.; Antoniadis-Karnavas, A.; Curto, G. Lo
Spain, Portugal, Switzerland, Germany, France, United States, Italy, Chile
Abstract
Context. Small planets located at the lower mode of the bimodal radius distribution are generally assumed to be composed of iron and silicates in a proportion similar to that of the Earth. However, recent discoveries are revealing a new group of low-density planets that are inconsistent with that description.
Aims: We intend to confirm and characterize the TESS planet candidate TOI-244.01, which orbits the bright (K = 7.97 mag), nearby (d = 22 pc), and early-type (M2.5 V) M-dwarf star GJ 1018 with an orbital period of 7.4 days.
Methods: We used Markov chain Monte Carlo methods to model 57 precise radial velocity measurements acquired by the ESPRESSO spectrograph together with TESS photometry and complementary HARPS data. Our model includes a planetary component and Gaussian processes aimed at modeling the correlated stellar and instrumental noise.
Results: We find TOI-244 b to be a super-Earth with a radius of Rp = 1.52 ± 0.12 R⊕ and a mass of Mp = 2.68 ± 0.30 M⊕. These values correspond to a density of ρ = 4.2 ± 1.1 g cm−3, which is below what would be expected for an Earth-like composition. We find that atmospheric loss processes may have been efficient to remove a potential primordial hydrogen envelope, but high mean molecular weight volatiles such as water could have been retained. Our internal structure modeling suggests that TOI-244 b has a 479−96+128 km thick hydrosphere over a 1.17 ± 0.09 R⊕ solid structure composed of a Fe-rich core and a silicate-dominated mantle compatible with that of the Earth. On a population level, we find two tentative trends in the density-metallicity and density-insolation parameter space for the low-density super-Earths, which may hint at their composition.
Conclusions: With a 8% precision in radius and 12% precision in mass, TOI-244 b is among the most precisely characterized super-Earths, which, together with the likely presence of an extended hydrosphere, makes it a key target for atmospheric observations.