An ultra-short-period transiting super-Earth orbiting the M3 dwarf TOI-1685
Dynamical histories of planetary systems, as well as the atmospheric evolution of highly irradiated planets, can be studied by characterizing the ultra-short-period planet population, which the TESS mission is particularly well suited to discover. Here, we report on the follow-up of a transit signal...
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
8 June 2021
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| In: |
Astronomy and astrophysics
Year: 2021, Jahrgang: 650, Pages: -17 |
| ISSN: | 1432-0746 |
| DOI: | 10.1051/0004-6361/202140688 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1051/0004-6361/202140688 Verlag, lizenzpflichtig, Volltext: https://www.aanda.org/articles/aa/abs/2021/06/aa40688-21/aa40688-21.html 
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| Verfasserangaben: | P. Bluhm, E. Pallé, K. Molaverdikhani, J. Kemmer, A.P. Hatzes, D. Kossakowski, S. Stock, J.A. Caballero, J. Lillo-Box, V.J.S. Béjar, M.G. Soto, P.J. Amado, P. Brown, C. Cadieux, R. Cloutier, K.A. Collins, K.I. Collins, M. Cortés-Contreras, R. Doyon, S. Dreizler, N. Espinoza, A. Fukui, E. González-Álvarez, Th. Henning, K. Horne, S.V. Jeffers, J.M. Jenkins, E.L.N. Jensen, A. Kaminski, J.F. Kielkopf, N. Kusakabe, M. Kürster, D. Lafrenière, R. Luque, F. Murgas, D. Montes, J.C. Morales, N. Narita, V.M. Passegger, A. Quirrenbach, P. Schöfer, S. Reffert, A. Reiners, I. Ribas, G.R. Ricker, S. Seager, A. Schweitzer, R.P. Schwarz, M. Tamura, T. Trifonov, R. Vanderspek, J. Winn, M. Zechmeister, and M.R. Zapatero Osorio |
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| 245 | 1 | 3 | |a An ultra-short-period transiting super-Earth orbiting the M3 dwarf TOI-1685 |c P. Bluhm, E. Pallé, K. Molaverdikhani, J. Kemmer, A.P. Hatzes, D. Kossakowski, S. Stock, J.A. Caballero, J. Lillo-Box, V.J.S. Béjar, M.G. Soto, P.J. Amado, P. Brown, C. Cadieux, R. Cloutier, K.A. Collins, K.I. Collins, M. Cortés-Contreras, R. Doyon, S. Dreizler, N. Espinoza, A. Fukui, E. González-Álvarez, Th. Henning, K. Horne, S.V. Jeffers, J.M. Jenkins, E.L.N. Jensen, A. Kaminski, J.F. Kielkopf, N. Kusakabe, M. Kürster, D. Lafrenière, R. Luque, F. Murgas, D. Montes, J.C. Morales, N. Narita, V.M. Passegger, A. Quirrenbach, P. Schöfer, S. Reffert, A. Reiners, I. Ribas, G.R. Ricker, S. Seager, A. Schweitzer, R.P. Schwarz, M. Tamura, T. Trifonov, R. Vanderspek, J. Winn, M. Zechmeister, and M.R. Zapatero Osorio |
| 264 | 1 | |c 8 June 2021 | |
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| 500 | |a Gesehen am 19.07.2022 | ||
| 520 | |a Dynamical histories of planetary systems, as well as the atmospheric evolution of highly irradiated planets, can be studied by characterizing the ultra-short-period planet population, which the TESS mission is particularly well suited to discover. Here, we report on the follow-up of a transit signal detected in the TESS sector 19 photometric time series of the M3.0 V star TOI-1685 (2MASS J04342248+4302148). We confirm the planetary nature of the transit signal, which has a period of <i>P<i/><sub>b<sub/> = d, using precise radial velocity measurements taken with the CARMENES spectrograph. From the joint photometry and radial velocity analysis, we estimate the following parameters for TOI-1685 b: a mass of <i>M<i/><sub>b<sub/> = <i>M<i/><sub>⊕<sub/>, a radius of <i>R<i/><sub>b<sub/> = <i>R<i/><sub>⊕<sub/>, which together result in a bulk density of <i>ρ<i/><sub>b<sub/> = g cm<sup>−3<sup/>, and an equilibrium temperature of <i>T<i/><sub>eq<sub/> = K. TOI-1685 b is the least dense ultra-short-period planet around an M dwarf known to date. TOI-1685 b is also one of the hottest transiting super-Earth planets with accurate dynamical mass measurements, which makes it a particularly attractive target for thermal emission spectroscopy. Additionally, we report with moderate evidence an additional non-transiting planet candidate in the system, TOI-1685 [c], which has an orbital period of <i>P<i/><sub>c<sub/> = d. | ||
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| 700 | 1 | |a Cortés-Contreras, M. |e VerfasserIn |4 aut | |
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