A planetary system with two transiting mini-Neptunes near the radius valley transition around the bright M dwarf TOI-776
We report the discovery and characterization of two transiting planets around the bright M1 V star LP 961-53 (TOI-776, J = 8.5 mag, M = 0.54 ± 0.03 M⊙) detected during Sector 10 observations of the Transiting Exoplanet Survey Satellite (TESS). Combining the TESS photometry with HARPS radial velociti...
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| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Article (Journal) |
| Language: | English |
| Published: |
05 January 2021
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| In: |
Astronomy and astrophysics
Year: 2021, Volume: 645, Pages: 1-24 |
| ISSN: | 1432-0746 |
| DOI: | 10.1051/0004-6361/202039455 |
| Online Access: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1051/0004-6361/202039455 Verlag, lizenzpflichtig, Volltext: https://www.aanda.org/articles/aa/abs/2021/01/aa39455-20/aa39455-20.html |
| Author Notes: | R. Luque, L.M. Serrano, K. Molaverdikhani, M.C. Nixon, J.H. Livingston, E.W. Guenther, E. Pallé, N. Madhusudhan, G. Nowak, J. Korth, W.D. Cochran, T. Hirano, P. Chaturvedi, E. Goffo, S. Albrecht, O. Barragán, C. Briceño, J. Cabrera, D. Charbonneau, R. Cloutier, K.A. Collins, K.I. Collins, K.D. Colón, I.J.M. Crossfield, Sz. Csizmadia, F. Dai, H.J. Deeg, M. Esposito, M. Fridlund, D. Gandolfi, I. Georgieva, A. Glidden, R.F. Goeke, S. Grziwa, A.P. Hatzes, C.E. Henze, S.B. Howell, J. Irwin, J.M. Jenkins, E.L.N. Jensen, P. Kábath, R.C. Kidwell, J.F. Kielkopf, E. Knudstrup, K.W.F. Lam, D.W. Latham, J.J. Lissauer, A.W. Mann, E.C. Matthews, I. Mireles, N. Narita, M. Paegert, C.M. Persson, S. Redfield, G.R. Ricker, F. Rodler, J.E. Schlieder, N.J. Scott, S. Seager, J. Šubjak, T.G. Tan, E.B. Ting, R. Vanderspek, V. Van Eylen, J.N. Winn, and C. Ziegler |
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| 245 | 1 | 2 | |a A planetary system with two transiting mini-Neptunes near the radius valley transition around the bright M dwarf TOI-776 |c R. Luque, L.M. Serrano, K. Molaverdikhani, M.C. Nixon, J.H. Livingston, E.W. Guenther, E. Pallé, N. Madhusudhan, G. Nowak, J. Korth, W.D. Cochran, T. Hirano, P. Chaturvedi, E. Goffo, S. Albrecht, O. Barragán, C. Briceño, J. Cabrera, D. Charbonneau, R. Cloutier, K.A. Collins, K.I. Collins, K.D. Colón, I.J.M. Crossfield, Sz. Csizmadia, F. Dai, H.J. Deeg, M. Esposito, M. Fridlund, D. Gandolfi, I. Georgieva, A. Glidden, R.F. Goeke, S. Grziwa, A.P. Hatzes, C.E. Henze, S.B. Howell, J. Irwin, J.M. Jenkins, E.L.N. Jensen, P. Kábath, R.C. Kidwell, J.F. Kielkopf, E. Knudstrup, K.W.F. Lam, D.W. Latham, J.J. Lissauer, A.W. Mann, E.C. Matthews, I. Mireles, N. Narita, M. Paegert, C.M. Persson, S. Redfield, G.R. Ricker, F. Rodler, J.E. Schlieder, N.J. Scott, S. Seager, J. Šubjak, T.G. Tan, E.B. Ting, R. Vanderspek, V. Van Eylen, J.N. Winn, and C. Ziegler |
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| 520 | |a We report the discovery and characterization of two transiting planets around the bright M1 V star LP 961-53 (TOI-776, J = 8.5 mag, M = 0.54 ± 0.03 M⊙) detected during Sector 10 observations of the Transiting Exoplanet Survey Satellite (TESS). Combining the TESS photometry with HARPS radial velocities, as well as ground-based follow-up transit observations from the MEarth and LCOGT telescopes, for the inner planet, TOI-776 b, we measured a period of Pb = 8.25 d, a radius of Rb = 1.85 ± 0.13 R⊕, and a mass of Mb = 4.0 ± 0.9 M⊕; and for the outer planet, TOI-776 c, a period of Pc = 15.66 d, a radius of Rc = 2.02 ± 0.14 R⊕, and a mass of Mc = 5.3 ± 1.8 M⊕. The Doppler data shows one additional signal, with a period of ~34 d, associated with the rotational period of the star. The analysis of fifteen years of ground-based photometric monitoring data and the inspection of different spectral line indicators confirm this assumption. The bulk densities of TOI-776 b and c allow for a wide range of possible interior and atmospheric compositions. However, both planets have retained a significant atmosphere, with slightly different envelope mass fractions. Thanks to their location near the radius gap for M dwarfs, we can start to explore the mechanism(s) responsible for the radius valley emergence around low-mass stars as compared to solar-like stars. While a larger sample of well-characterized planets in this parameter space is still needed to draw firm conclusions, we tentatively estimate that the stellar mass below which thermally-driven mass loss is no longer the main formation pathway for sculpting the radius valley is between 0.63 and 0.54 M⊙. Due to the brightness of the star, the TOI-776 system is also an excellent target for the James Webb Space Telescope, providing a remarkable laboratory in which to break the degeneracy in planetary interior models and to test formation and evolution theories of small planets around low-mass stars. | ||
| 700 | 1 | |a Serrano, L. M. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Molaverdikhani, Karan |d 1982- |e VerfasserIn |0 (DE-588)1205499784 |0 (DE-627)1691167576 |4 aut | |
| 700 | 1 | |a Nixon, M. C. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Livingston, J. H. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Guenther, E. W. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Pallé, E. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Madhusudhan, N. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Nowak, G. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Korth, J. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Cochran, W. D. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Hirano, T. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Chaturvedi, P. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Goffo, E. |e VerfasserIn |4 aut | |
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| 700 | 1 | |a Colón, K. D. |e VerfasserIn |4 aut | |
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| 700 | 1 | |a Esposito, M. |e VerfasserIn |4 aut | |
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| 700 | 1 | |a Irwin, J. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Jenkins, J. M. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Jensen, E. L. N. |e VerfasserIn |4 aut | |
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| 700 | 1 | |a Matthews, E. C. |e VerfasserIn |4 aut | |
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| 700 | 1 | |a Narita, N. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Paegert, M. |e VerfasserIn |4 aut | |
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| 700 | 1 | |a Ricker, G. R. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Rodler, F. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Schlieder, J. E. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Scott, N. J. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Seager, S. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Šubjak, J. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Tan, T. G. |e VerfasserIn |4 aut | |
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| 700 | 1 | |a Eylen, V. Van |e VerfasserIn |4 aut | |
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| 700 | 1 | |a Ziegler, C. |e VerfasserIn |4 aut | |
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