TOI-1136 is a Young, Coplanar, Aligned Planetary System in a Pristine Resonant Chain

Autor: Dai, Fei, Masuda, Kento, Beard, Corey, Robertson, Paul, Goldberg, Max, Batygin, Konstantin, Bouma, Luke, Lissauer, Jack J., Knudstrup, Emil, Albrecht, Simon, Howard, Andrew W., Knutson, Heather A., Petigura, Erik A., Weiss, Lauren M., Isaacson, Howard, Kristiansen, Martti Holst, Osborn, Hugh, Wang, Songhu, Wang, Xian-Yu, Behmard, Aida, Greklek-McKeon, Michael, Vissapragada, Shreyas, Batalha, Natalie M., Brinkman, Casey L., Chontos, Ashley, Crossfield, Ian, Dressing, Courtney, Fetherolf, Tara, Fulton, Benjamin, Hill, Michelle L., Huber, Daniel, Kane, Stephen R., Lubin, Jack, MacDougall, Mason, Mayo, Andrew, Močnik, Teo, Murphy, Joseph M. Akana, Rubenzahl, Ryan A., Scarsdale, Nicholas, Tyler, Dakotah, Van Zandt, Judah, Polanski, Alex S., Schwengeler, Hans Martin, Terentev, Ivan A., Benni, Paul, Bieryla, Allyson, Ciardi, David, Falk, Ben, Furlan, E., Girardin, Eric, Guerra, Pere, Hesse, Katharine M., Howell, Steve B., Lillo-Box, J., Matthews, Elisabeth C., Twicken, Joseph D., Villaseñor, Joel, Latham, David W., Jenkins, Jon M., Ricker, George R., Seager, Sara, Vanderspek, Roland, Winn, Joshua N.

Convergent disk migration has long been suspected to be responsible for forming planetary systems with a chain of mean-motion resonances (MMR). Dynamical evolution over time could disrupt the delicate resonant configuration. We present TOI-1136, a 70

Externí odkaz: http://arxiv.org/abs/2210.09283