Modeling Spitzer 3.6 and 4.5 μm Eclipse Depths for the Inflated Hot Jupiter in the Evolved Binary System HD 202772 Article Swipe
Arthur D. Adams
,
Kimberly Bott
,
Paul A. Dalba
,
Tara Fetherolf
,
Stephen R. Kane
,
Ian J. M. Crossfield
,
Drake Deming
,
Diana Dragomir
,
Varoujan Gorjian
,
Laura Kreidberg
,
Farisa Y. Morales
,
M. W. Werner
·
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.3847/1538-3881/ad7091
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.3847/1538-3881/ad7091
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 reduction and analysis of eclipse light-curve observations of HD 202772 A b acquired with the Spitzer Space Telescope using the 3.6 and 4.5 μ m channels. We find eclipse depths of 680 ± 68 and ppm, respectively, corresponding to dayside effective temperatures of and K. The corresponding Bond albedos are consistent with the distribution of albedos for hot Jupiters observed with both Spitzer and Transiting Exoplanet Survey Satellite. The heat redistribution efficiencies consistent with the Bond albedo range predicted by one-dimensional atmospheric models in radiative-convective equilibrium are 0.71 ± 0.10 and , respectively, indicating a weak day–night contrast for the former and a strong contrast for the latter. Given this, and the unique environment in which this planet resides, we recommend follow-up observations with JWST to more precisely constrain its atmospheric composition and structure, as well as its host stellar environment, to elucidate if and how the atmospheres of these close-in giants evolve with host stars in binaries past the main sequence.
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- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-3881/ad7091
- https://iopscience.iop.org/article/10.3847/1538-3881/ad7091/pdf
- OA Status
- gold
- References
- 53
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4404241658
All OpenAlex metadata
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- OpenAlex ID
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https://openalex.org/W4404241658Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3847/1538-3881/ad7091Digital Object Identifier
- Title
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Modeling Spitzer 3.6 and 4.5 μm Eclipse Depths for the Inflated Hot Jupiter in the Evolved Binary System HD 202772Work title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2024Year of publication
- Publication date
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2024-11-11Full publication date if available
- Authors
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Arthur D. Adams, Kimberly Bott, Paul A. Dalba, Tara Fetherolf, Stephen R. Kane, Ian J. M. Crossfield, Drake Deming, Diana Dragomir, Varoujan Gorjian, Laura Kreidberg, Farisa Y. Morales, M. W. WernerList of authors in order
- Landing page
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https://doi.org/10.3847/1538-3881/ad7091Publisher landing page
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https://iopscience.iop.org/article/10.3847/1538-3881/ad7091/pdfDirect link to full text PDF
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YesWhether a free full text is available
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goldOpen access status per OpenAlex
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https://iopscience.iop.org/article/10.3847/1538-3881/ad7091/pdfDirect OA link when available
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Physics, Eclipse, Jupiter (rocket family), Astrophysics, Astronomy, Binary number, Hot Jupiter, Light curve, Astrobiology, Planet, Exoplanet, Spacecraft, Mathematics, ArithmeticTop concepts (fields/topics) attached by OpenAlex
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0Total citation count in OpenAlex
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53Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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| countries_distinct_count | 3 |
| institutions_distinct_count | 12 |
| corresponding_institution_ids | https://openalex.org/I103635307, https://openalex.org/I4210104270, https://openalex.org/I51556381 |
| citation_normalized_percentile.value | 0.18091305 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | False |