Modeling Spitzer 3.6 and 4.5 μm Eclipse Depths for the Inflated Hot Jupiter in the Evolved Binary System HD 202772

Modeling Spitzer 3.6 and 4.5 μm Eclipse Depths for the Inflated Hot Jupiter in the Evolved Binary System HD 202772

As an inflated hot Jupiter orbiting an early-type primary star in the evolved binary HD 202772 system, HD 202772 A b’s presence invites a study of how such a planet forms and evolves. As a prelude to potential atmospheric characterization with the latest generation of observatories, we present a red...

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Bibliographic Details
Main Authors: Arthur D. Adams, Kimberly Bott, Paul A. Dalba, Tara Fetherolf, Stephen R. Kane, Ian Crossfield, Drake Deming, Diana Dragomir, Varoujan Gorjian, Laura Kreidberg, Farisa Y. Morales, Michael W. Werner
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astronomical Journal
Subjects:
Exoplanet atmospheres
Exoplanets
Exoplanet systems
Extrasolar gaseous giant planets
Hot Jupiters
Planetary atmospheres
Online Access:https://doi.org/10.3847/1538-3881/ad7091
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https://doi.org/10.3847/1538-3881/ad7091

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