Document Type
Article
Publication Date
1-23-2020
Publication Title
Monthly Notices of the Royal Astronomical Society
Publisher
Oxford University Press
Volume
492
Issue
4
First page number:
5399
Last page number:
5412
Abstract
The Transiting Exoplanet Survey Satellite, TESS, is currently carrying out an all-sky search for small planets transiting bright stars. In the first year of the TESS survey, a steady progress was made in achieving the mission’s primary science goal of establishing bulk densities for 50 planets smaller than Neptune. During that year, the TESS’s observations were focused on the southern ecliptic hemisphere, resulting in the discovery of three mini-Neptunes orbiting the star TOI-125, a V = 11.0 K0 dwarf. We present intensive HARPS radial velocity observations, yielding precise mass measurements for TOI-125b, TOI-125c, and TOI-125d. TOI-125b has an orbital period of 4.65 d, a radius of 2.726 ± 0.075 RE, a mass of 9.50 ± 0.88 ME, and is near the 2:1 mean motion resonance with TOI-125c at 9.15 d. TOI-125c has a similar radius of 2.759 ± 0.10 RE and a mass of 6.63 ± 0.99 ME, being the puffiest of the three planets. TOI-125d has an orbital period of 19.98 d and a radius of 2.93 ± 0.17 RE and mass 13.6 ± 1.2 ME. For TOI-125b and d, we find unusual high eccentricities of 0.19 ± 0.04 and 0.17+0.08−0.06, respectively. Our analysis also provides upper mass limits for the two low-SNR planet candidates in the system; for TOI-125.04 (RP = 1.36 RE, P = 0.53 d), we find a 2σ upper mass limit of 1.6 ME, whereas TOI-125.05 (RP=4.2+2.4−1.4 RE, P = 13.28 d) is unlikely a viable planet candidate with an upper mass limit of 2.7 ME. We discuss the internal structure of the three confirmed planets, as well as dynamical stability and system architecture for this intriguing exoplanet system.
Keywords
Planets and satellites: detection; Planets and satellites: individual: (TOI-125, TIC 52368076)
Disciplines
Cosmology, Relativity, and Gravity | The Sun and the Solar System
File Format
File Size
9.537 KB
Language
English
Creative Commons License
This work is licensed under a Creative Commons Attribution 4.0 License.
Repository Citation
Nielsen, L. D.,
Gandolfi, D.,
Armstrong, D. J.,
Jenkins, J. S.,
Fridlund, M.,
Santos, N. C.,
Dai, F.,
Adibekyan, V.,
Luque, R.,
Steffen, J. H.,
Esposito, M.,
Meru, F.,
Sabotta, S.,
Bolmont, E.,
Kossakowski, D.,
Otegi, J. F.,
Murgas, F.,
Stalport, M.,
Rodler, F.,
Diaz, M. R.,
Kurtovic, N. T.,
Ricker, G.,
Vanderspek, R.,
Latham, D. W.,
Seager, S.,
Winn, J. N.,
Jenkins, J. M.,
Allart, R.,
Almenara, J. M.,
Barrado, D.,
Barros, S. C.
(2020).
Mass Determinations of the Three Mini-Neptunes Transiting TOI-125.
Monthly Notices of the Royal Astronomical Society, 492(4),
5399-5412.
Oxford University Press.
http://dx.doi.org/10.1093/mnras/staa197