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TOI-824 b: A New Planet on the Lower Edge of the Hot Neptune Desert
The Astronomical Journal ( IF 5.3 ) Pub Date : 2020-09-04 , DOI: 10.3847/1538-3881/abac0c
Jennifer A. Burt 1, 2 , Louise D. Nielsen 3 , Samuel N. Quinn 4 , Eric E. Mamajek 1 , Elisabeth C. Matthews 2 , George Zhou 4 , Julia V. Seidel 3 , Chelsea X. Huang 2 , Eric Lopez 5 , Maritza Soto 6 , Jon Otegi 3, 7 , Keivan G. Stassun 8, 9 , Laura Kreidberg 4 , Karen A. Collins 4 , Jason D. Eastman 4 , Joseph E. Rodriguez 10 , Andrew Vanderburg 11 , Samuel P. Halverson 1 , Johanna K. Teske 12 , Sharon X. Wang 12 , R. Paul Butler 13 , Franois Bouchy 3 , Xavier Dumusque 3 , Damien Segransen 3 , Stephen A. Shectman 12 , Jeffrey D. Crane 12 , Fabo Feng 13 , Benjamin T. Montet 14 , Adina D. Feinstein 15 , Yuri Beletski 16 , Erin Flowers 17 , Maximilian N. Gnther 2 , Tansu Daylan 2 , Kevin I. Collins 18 , Dennis M. Conti 19 , Tianjun Gan 20 , Eric L. N. Jensen 21 , John F. Kielkopf 22 , Thiam-Guan Tan 23 , Ravit Helled 7 , Caroline Dorn 7 , Jonas Haldemann 24 , Jack J. Lissauer 25 , George R. Ricker 2 , Roland Vanderspek 2 , David W. Latham 4 , S. Seager 2, 26, 27 , Joshua N. Winn 17 , Jon M. Jenkins 28 , Joseph D. Twicken 28, 29 , Jeffrey C. Smith 28, 29 , Peter Tenenbaum 28, 29 , Scott Cartwright 30 , Thomas Barclay 5, 31 , Joshua Pepper 32 , Gilbert Esquerdo 4 , William Fong 2
Affiliation  

We report the detection of a transiting hot Neptune exoplanet orbiting TOI-824 (SCR J1448-5735), a nearby (d = 64 pc) K4V star, using data from the \textit{Transiting Exoplanet Survey Satellite} (TESS). The newly discovered planet has a radius, $R_{\rm{p}}$ = 2.93 $\pm$ 0.20 R$_{\oplus}$, and an orbital period of 1.393 days. Radial velocity measurements using the Planet Finder Spectrograph (PFS) and the High Accuracy Radial velocity Planet Searcher (HARPS) spectrograph confirm the existence of the planet and we estimate its mass to be $M_{\rm{p}}$ = 18.47 $\pm$ 1.84 M$_{\oplus}$. The planet's mean density is $\rho_{\rm{p}}$ = 4.03$^{+0.98}_{-0.78}$ g cm$^{-3}$ making it more than twice as dense as Neptune. TOI-824 b's high equilibrium temperature makes the planet likely to have a cloud free atmosphere, and thus an excellent candidate for follow up atmospheric studies. The detectability of TOI-824 b's atmosphere from both ground and space is promising and could lead to the detailed characterization of the most irradiated, small planet at the edge of the hot Neptune desert that has retained its atmosphere to date.

中文翻译:

TOI-824 b:热海王星沙漠下缘的新行星

我们报告使用来自\textit{Transiting Exoplanet Survey Satellite} (TESS) 的数据,检测到一颗围绕TOI-824 (SCR J1448-5735) 运行的热海王星系外行星,这是一颗附近(d = 64 pc)K4V 恒星。这颗新发现的行星半径为 $R_{\rm{p}}$ = 2.93 $\pm$ 0.20 R$_{\oplus}$,公转周期为 1.393 天。使用行星探测器光谱仪 (PFS) 和高精度径向速度行星搜索仪 (HARPS) 光谱仪进行的径向速度测量证实了这颗行星的存在,我们估计它的质量为 $M_{\rm{p}}$ = 18.47 $\下午$ 1.84 M$_{\oplus}$。这颗行星的平均密度为 $\rho_{\rm{p}}$ = 4.03$^{+0.98}_{-0.78}$ g cm$^{-3}$,使其密度是海王星的两倍多。TOI-824 b 的高平衡温度使这颗行星可能有无云大气层,因此是后续大气研究的绝佳候选者。从地面和太空对 TOI-824 b 大气的可探测性是有希望的,并且可能导致对迄今为止仍保留其大气的炎热海王星沙漠边缘的受辐射最严重的小行星进行详细描述。
更新日期:2020-09-04
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