TESS Hunt for Young and Maturing Exoplanets (THYME) IV: Three small planets orbiting a 120 Myr-old star in the Pisces--Eridanus stream

Autor:	Newton, Elisabeth R., Mann, Andrew W., Kraus, Adam L., Livingston, John H., Vanderburg, Andrew, Curtis, Jason L., Thao, Pa Chia, Hawkins, Keith, Wood, Mackenna L., Rizzuto, Aaron C., Soubkiou, Abderahmane, Tofflemire, Benjamin M., Zhou, George, Crossfield, Ian J. M., Pearce, Logan A., Collins, Karen A., Conti, Dennis M., Tan, Thiam-Guan, Villeneuva, Steven, Spencer, Alton, Dragomir, Diana, Quinn, Samuel N., Jensen, Eric L. N., Collins, Kevin I., Stockdale, Chris, Cloutier, Ryan, Hellier, Coel, Benkhaldoun, Zouhair, Ziegler, Carl, Briceño, César, Law, Nicholas, Benneke, Björn, Christiansen, Jessie L., Gorjian, Varoujan, Kane, Stephen R., Kreidberg, Laura, Morales, Farisa Y., Werner, Michael W, Twicken, Joseph D., Levine, Alan M., Ciardi, David R., Guerrero, Natalia M., Hesse, Katharine, Quintana, Elisa V., Shiao, Bernie, Smith, Jeffrey C., Torres, Guillermo, Ricker, George R., Vanderspek, Roland, Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Latham, David W.
Rok vydání:	2021
Předmět:	Astrophysics - Earth and Planetary Astrophysics Astrophysics - Solar and Stellar Astrophysics
Zdroj:	The Astronomical Journal, 2021, Volume 161, Issue 2
Druh dokumentu:	Working Paper
DOI:	10.3847/1538-3881/abccc6
Popis:	Young exoplanets can offer insight into the evolution of planetary atmospheres, compositions, and architectures. We present the discovery of the young planetary system TOI 451 (TIC 257605131, Gaia DR2 4844691297067063424). TOI 451 is a member of the 120-Myr-old Pisces--Eridanus stream (Psc--Eri). We confirm membership in the stream with its kinematics, its lithium abundance, and the rotation and UV excesses of both TOI 451 and its wide binary companion, TOI 451 B (itself likely an M dwarf binary). We identified three candidate planets transiting in the TESS data and followed up the signals with photometry from Spitzer and ground-based telescopes. The system comprises three validated planets at periods of 1.9, 9.2 and 16 days, with radii of 1.9, 3.1, and 4.1 Earth radii, respectively. The host star is near-solar mass with V=11.0 and H=9.3 and displays an infrared excess indicative of a debris disk. The planets offer excellent prospects for transmission spectroscopy with HST and JWST, providing the opportunity to study planetary atmospheres that may still be in the process of evolving. Comment: 20 pages, appendix on UV excess
Databáze:	arXiv
Externí odkaz:	http://arxiv.org/abs/2102.06049 Zobrazit plný text záznamu View this record from Arxiv