The Occurrence of Small, Short-period Planets Younger than 200 Myr with TESS

The Occurrence of Small, Short-period Planets Younger than 200 Myr with TESS

Within the first few hundreds of millions of years, many physical processes sculpt the eventual properties of young planets. NASA’s Transiting Exoplanet Survey Satellite (TESS) mission has surveyed young stellar associations across the entire sky for transiting planets, providing glimpses into the v...

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Bibliographic Details
Main Authors: Sydney Vach, George Zhou, Chelsea X. Huang, James G. Rogers, L. G. Bouma, Stephanie T. Douglas, Michelle Kunimoto, Andrew W. Mann, Madyson G. Barber, Samuel N. Quinn, David W. Latham, Allyson Bieryla, Karen Collins
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astronomical Journal
Subjects:
Exoplanets
Mini Neptunes
Transit photometry
Exoplanet evolution
Planetary system evolution
Young star clusters
Online Access:https://doi.org/10.3847/1538-3881/ad3108

Internet

https://doi.org/10.3847/1538-3881/ad3108

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