Stellar Obliquities of Young Systems, Atmospheres Undergoing Contraction and Escape (SOYSAUCE). II. A 135 Myr Planet on an Aligned Orbit with Transit Timing Variations

Young planets (<1 Gyr) provide opportunities to directly probe planet formation and evolution processes in action. However, due to heightened stellar activity, there is a lack of known transiting planets in adolescence (∼100–500 Myr). Here we present the validation of TIC 150070085 b, a 3.6 R _⊕ pla...

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Detalhes bibliográficos

Principais autores:	Madyson G. Barber, Andrew W. Mann, Sydney Vach, Leah J. Boff, Andrew W. Boyle, Andrew Vanderburg, Adam L. Kraus, Benjamin M. Tofflemire, Marshall C. Johnson, Allyson Bieryla, David W. Latham, Karen A. Collins, Steve B. Howell, Richard P. Schwarz, Gregorg Srdoc, Francis P. Wilkin, Felipe Murgas, Enric Palle, Chris Stockdale
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2026-01-01
Colecção:	The Astronomical Journal
Assuntos:	Exoplanets Exoplanet dynamics Transit photometry Exoplanet systems Stellar ages
Acesso em linha:	https://doi.org/10.3847/1538-3881/ae78d0
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