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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Autors principals:	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
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2026-01-01
Col·lecció:	The Astronomical Journal
Matèries:	Exoplanets Exoplanet dynamics Transit photometry Exoplanet systems Stellar ages
Accés en línia:	https://doi.org/10.3847/1538-3881/ae78d0
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