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Author  |
Trifonov, T.; Brahm, R.; Espinoza, N.; Henning, T.; Jordan, A.; Nesvorny, D.; Dawson, R.I.; Lissauer, J.J.; Lee, M.H.; Kossakowski, D.; Rojas, F.I.; Hobson, M.J.; Sarkis, P.; Schlecker, M.; Bitsch, B.; Bakos, G.A.; Barbieri, M.; Bhatti, W.; Butler, R.P.; Crane, J.D.; Nandakumar, S.; Diaz, M.R.; Shectman, S.; Teske, J.; Torres, P.; Suc, V.; Vines, J.I.; Wang, S.R.X.; Ricker, G.R.; Shporer, A.; Vanderburg, A.; Dragomir, D.; Vanderspek, R.; Burke, C.J.; Daylan, T.; Shiao, B.; Jenkins, J.M.; Wohler, B.; Seager, S.; Winn, J.N. |

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Title |
A Pair of Warm Giant Planets near the 2:1 Mean Motion Resonance around the K-dwarf Star TOI-2202* |
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Year |
2021 |
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Astronomical Journal |
Abbreviated Journal |
Astron. J. |
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162 |
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6 |
Pages |
283 |
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Keywords |
EARTH-SIZED PLANET; SUPER-EARTH; HOT JUPITERS; TESS; SYSTEMS; TRANSIT; NEPTUNE; MODEL; PERIODOGRAM; SCATTERING |
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Abstract |
TOI-2202 b is a transiting warm Jovian-mass planet with an orbital period of P = 11.91 days identified from the Full Frame Images data of five different sectors of the TESS mission. Ten TESS transits of TOI-2202 b combined with three follow-up light curves obtained with the CHAT robotic telescope show strong transit timing variations (TTVs) with an amplitude of about 1.2 hr. Radial velocity follow-up with FEROS, HARPS, and PFS confirms the planetary nature of the transiting candidate (a (b) = 0.096 +/- 0.001 au, m (b) = 0.98 +/- 0.06 M (Jup)), and a dynamical analysis of RVs, transit data, and TTVs points to an outer Saturn-mass companion (a (c) = 0.155 +/- 0.002 au, m (c) = 0.37 +/- 0.10 M (Jup)) near the 2:1 mean motion resonance. Our stellar modeling indicates that TOI-2202 is an early K-type star with a mass of 0.82 M (circle dot), a radius of 0.79 R (circle dot), and solar-like metallicity. The TOI-2202 system is very interesting because of the two warm Jovian-mass planets near the 2:1 mean motion resonance, which is a rare configuration, and their formation and dynamical evolution are still not well understood. |
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0004-6256 |
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WOS:000725244600001 |
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UAI @ alexi.delcanto @ |
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1511 |
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