TESS Hunt for Young and Maturing Exoplanets (THYME) III: a two-planet system in the 400 Myr Ursa Major Group

Exoplanets can evolve significantly between birth and maturity, as their atmospheres, orbits, and structures are shaped by their environment. Young planets (\(

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Bibliographische Detailangaben
Veröffentlicht in:	arXiv.org 2020-10
Hauptverfasser:	Mann, Andrew W, Johnson, Marshall C, Vanderburg, Andrew, Kraus, Adam L, Rizzuto, Aaron C, Wood, Mackenna L, Bush, Jonathan L, Keighley Rockcliffe, Newton, Elisabeth R, Latham, David W, Mamajek, Eric E, Zhou, George, Quinn, Samuel N, Pa Chia Thao, Benatti, Serena, Cosentino, Rosario, Desidera, Silvano, Harutyunyan, Avet, Lovis, Christophe, Mortier, Annelies, Pepe, Francesco A, Poretti, Ennio, Wilson, Thomas G, Kristiansen, Martti H, Gagliano, Robert, Jacobs, Thomas, LaCourse, Daryll M, Omohundro, Mark, Hans Martin Schwengeler, Terentev, Ivan A, Kane, Stephen R, Hill, Michelle L, Rabus, Markus, Esquerdo, Gilbert A, Berlind, Perry, Collins, Karen A, Murawski, Gabriel, Sallam, Nezar Hazam, Aitken, Michael M, Massey, Bob, Ricker, George R, Vanderspek, Roland, Seager, Sara, Winn, Joshua N, Jenkins, Jon M, Barclay, Thomas, Caldwell, Douglas A, Dragomir, Diana, Doty, John P, Glidden, Ana, Tenenbaum, Peter, Torres, Guillermo, Twicken, Joseph D, Villanueva, Steven
Format:	Artikel
Sprache:	eng
Schlagworte:	Extrasolar planets Kinematics Light curve Lithium Physics - Earth and Planetary Astrophysics Physics - Solar and Stellar Astrophysics Planet formation Planetary evolution Planetary orbits Planetary systems Radial velocity
Online-Zugang:	Volltext
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Beschreibung
Zusammenfassung:	Exoplanets can evolve significantly between birth and maturity, as their atmospheres, orbits, and structures are shaped by their environment. Young planets (\(
ISSN:	2331-8422
DOI:	10.48550/arxiv.2005.00047