The Super-puff WASP-193 b is on a Well-aligned Orbit

The “super-puffs” are a population of planets that have masses comparable to that of Neptune but radii similar to Jupiter, leading to extremely low bulk densities ( ρ _p  ≲ 0.2 g cm ^−3 ) that are not easily explained by standard core accretion models. Interestingly, several of these super-puffs are...

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Bibliographic Details
Published in:The Astronomical Journal
Main Authors: Samuel W. Yee, Gudmundur Stefánsson, Daniel Thorngren, Andy Monson, Joel D. Hartman, David B. Charbonneau, Johanna K. Teske, R. Paul Butler, Jeffrey D. Crane, David Osip, Stephen A. Shectman
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Subjects:
Exoplanet astronomy
Hot Jupiters
Exoplanets
Online Access:https://doi.org/10.3847/1538-3881/adba5f

Internet

https://doi.org/10.3847/1538-3881/adba5f

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