B. Lavie, F. Bouchy, C. Lovis, M. R. Zapatero Osorio, A. Deline, S. C. C. Barros, P. Figueira, A. Sozzetti, J. I. González Hernández, J. Lillo-Box, J. Rodrigues, A. Mehner, M. Damasso, V. Zh. Adibekyan, Y. Alibert, C. Allende Prieto, S. Cristiani, V. D'Odorico, P. Di Marcantonio, D. Ehrenreich, R. Génova Santos, G. Lo Curto, C. J. A. P. Martins, G. Micela, P. Molaro, N. J. Nunes, E. Palle, F. Pepe, E. Poretti, R. Rebolo, N. C. Santos, S. G. Sousa, A. Suárez Mascareño, H. M. Tabernero, S. Udry
Abstract
We present radial velocity follow-up obtained with ESPRESSO of the M-type star LTT 1445A (TOI-455), for which a transiting planet b with an orbital period of 5.4 days was detected by TESS. We report the discovery of a second transiting planet (LTT 1445A c) and a third non-transiting candidate planet (LTT 1445A d) with orbital periods of 3.12 and 24.30 days, respectively. The host star is the main component of a triple M-dwarf system at a distance of 6.9 pc. We used 84 ESPRESSO high-resolution spectra to determine accurate masses of 2.3 ± 0.3 M⊕ and 1.0 ± 0.2 M⊕ for planets b and c and a minimum mass of 2.7 ± 0.7 M⊕ for planet d. Based on its radius of 1.43 ± 0.09 R⊕ as derived from the TESS observations, LTT 1445A b has a lower density than the Earth and may therefore hold a sizeable atmosphere, which makes it a prime target for the James Webb Space Telescope (JWST). We used a Bayesian inference approach with the nested sampling algorithm and a set of models to test the robustness of the retrieved physical values of the system. There is a probability of 85% that the transit of planet c is grazing, which results in a retrieved radius with large uncertainties at 1.60−0.34+0.67 R⊕. LTT 1445A d orbits the inner boundary of the habitable zone of its host star and could be a prime target for the JWST.
Keywords
planets and satellites: detection / planets and satellites: terrestrial planets / techniques: radial velocities / techniques: photometric / stars: individual: TOI-455 / stars: individual: LTT 1445
Notes
- RV and activity indices for ESPRESSO are only available at the CDS via anonymous ftp to cdsarc.cds.unistra.fr (130.79.128.5) or via https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/673/A69
- Based on Guaranteed Time Observations collected at the European Southern Observatory under ESO programme(s) 1104.C-0350, 106.21M2.002 by the ESPRESSO Consortium.
Astronomy & Astrophysics
Volume 673, Article Number A69, Number of pages 29
2023 May
