论文标题

TOI 122B和TOI 237b,两个旋转的小型行星旋转的小矮人,由\ textit {tess}找到

TOI 122b and TOI 237b, two small warm planets orbiting inactive M dwarfs, found by \textit{TESS}

论文作者

Waalkes, William C., Berta-Thompson, Zachory K., Collins, Karen A., Feinstein, Adina D., Tofflemire, Benjamin M., Rojas-Ayala, Bárbara, Silverstein, Michele L., Newton, Elisabeth, Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, S., Winn, Joshua N., Jenkins, Jon M., Christiansen, Jessie, Goeke, Robert F., Levine, Alan M., Osborn, H. P., Rinehart, S. A., Rose, Mark E., Ting, Eric B., Twicken, Joseph D., Barkaoui, Khalid, Bean, Jacob L., Briceño, César, Ciardi, David R., Collins, Kevin I., Conti, Dennis, Gan, Tianjun, Gillon, Michaël, Isopi, Giovanni, Jehin, Emmanuël, Jensen, Eric L. N., Kielkopf, John F., Law, Nicholas, Mallia, Franco, Mann, Andrew W., Montet, Benjamin T., Pozuelos, Francisco J., Relles, Howard, Libby-Roberts, Jessica E., Ziegler, Carl

论文摘要

我们报告了TOI 122B和TOI 237b的发现和验证,这是两个温暖的行星,经过\ textit {tess}观察到的未活跃m矮人。 Our analysis shows TOI 122b has a radius of 2.72$\pm$0.18 R$_\rm{e}$ and receives 8.8$\pm$1.0$\times$ Earth's bolometric insolation, and TOI 237b has a radius of 1.44$\pm$0.12 R$_\rm{e}$ and receives 3.7$\pm$0.5$\times$泥土的突破性,跨越了6.7 $ \ times $ erser汞从阳光中收到的泥土损失。这使得这两个较冷的行星尚未在\ textit {tess}中发现,即使在其5.08天和5.43天轨道上也是如此。它们共同跨越了小型行星半径谷,提供了有用的实验室,以探索M矮人周围的挥发性进化。它们相对附近的距离(62.23 $ \ pm $ 0.21 pc和38.11 $ \ pm $ 0.23 PC)使它们成为可能可行的目标,以实现未来的径向速度随访和大气表征,尽管这种观察结果可能需要在大型望远镜上进行大量时间投资。

We report the discovery and validation of TOI 122b and TOI 237b, two warm planets transiting inactive M dwarfs observed by \textit{TESS}. Our analysis shows TOI 122b has a radius of 2.72$\pm$0.18 R$_\rm{e}$ and receives 8.8$\pm$1.0$\times$ Earth's bolometric insolation, and TOI 237b has a radius of 1.44$\pm$0.12 R$_\rm{e}$ and receives 3.7$\pm$0.5$\times$ Earth insolation, straddling the 6.7$\times$ Earth insolation that Mercury receives from the sun. This makes these two of the cooler planets yet discovered by \textit{TESS}, even on their 5.08-day and 5.43-day orbits. Together, they span the small-planet radius valley, providing useful laboratories for exploring volatile evolution around M dwarfs. Their relatively nearby distances (62.23$\pm$0.21 pc and 38.11$\pm$0.23 pc, respectively) make them potentially feasible targets for future radial velocity follow-up and atmospheric characterization, although such observations may require substantial investments of time on large telescopes.

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