Tracing the formation and migration history: molecular signatures in the atmosphere of misaligned hot Jupiter WASP-94 A b using JWST NIRSpec/G395H Article Swipe
Eva-Maria Ahrer
,
Siddharth Gandhi
,
Lili Alderson
,
James Kirk
,
Johanna Teske
,
Richard A Booth
,
Catriona H McDonald
,
Duncan Christie
,
Alastair B Claringbold
,
Rebecca Nealon
,
Vatsal Panwar
,
Dimitri Veras
,
Hannah R. Wakeford
,
P. J. Wheatley
,
Maria Zamyatina
·
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.1093/mnras/staf819
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.1093/mnras/staf819
The discovery of hot Jupiters that orbit very close to their host stars has long challenged traditional models of planetary formation and migration. Characterizing their atmospheric composition – mainly in the form of the carbon-to-oxygen (C/O) ratio and metallicity – can provide insights into their formation locations and evolution pathways. With JWST, we can characterize the atmospheres of these types of planets more precisely than previously possible, primarily because it allows us to determine both their atmospheric oxygen and carbon composition. Here, we present a JWST NIRSpec (Near-Infrared Spectrograph)/G395H transmission spectrum from 2.8 to 5.1 $\mu {\rm m}$ of WASP-94 A b, an inflated hot Jupiter with a retrograde misaligned orbit around its F-type host star. We find a relatively cloud-free atmosphere, with absorption features of ${\rm H}_{2}{\rm O}$ and ${\rm CO}_{2}$ at detection significances of ${\sim} 4\sigma$ and ${\sim} 11\sigma$, respectively. In addition, we detect tentative evidence of ${\rm CO}$ absorption at ${\sim} 3\sigma$, as well as hints of sulphur with the detection of ${\rm H}_{2}{\rm S}$ at a ${\sim} 2.5\sigma$ confidence level. Our favoured equilibrium chemistry model determines a C/O ratio of $0.49^{+0.08}_{-0.13}$ for WASP-94 A b’s atmosphere, which is substellar compared to the star’s C/O ratio of $0.68 \pm 0.10$. The retrieved atmospheric metallicity is similar to the star’s metallicity, as both are ${\sim} 2\times$ solar. We find that this substellar C/O ratio and stellar metallicity can be best explained by pebble accretion or planetesimal accretion in combination with large-distance migration of the planet.
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- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1093/mnras/staf819
- https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/staf819/63236687/staf819.pdf
- OA Status
- gold
- Cited By
- 1
- References
- 146
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4410484389
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4410484389Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.1093/mnras/staf819Digital Object Identifier
- Title
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Tracing the formation and migration history: molecular signatures in the atmosphere of misaligned hot Jupiter WASP-94 A b using JWST NIRSpec/G395HWork title
- Type
-
articleOpenAlex work type
- Language
-
enPrimary language
- Publication year
-
2025Year of publication
- Publication date
-
2025-05-19Full publication date if available
- Authors
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Eva-Maria Ahrer, Siddharth Gandhi, Lili Alderson, James Kirk, Johanna Teske, Richard A Booth, Catriona H McDonald, Duncan Christie, Alastair B Claringbold, Rebecca Nealon, Vatsal Panwar, Dimitri Veras, Hannah R. Wakeford, P. J. Wheatley, Maria ZamyatinaList of authors in order
- Landing page
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https://doi.org/10.1093/mnras/staf819Publisher landing page
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https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/staf819/63236687/staf819.pdfDirect link to full text PDF
- Open access
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YesWhether a free full text is available
- OA status
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goldOpen access status per OpenAlex
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https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/staf819/63236687/staf819.pdfDirect OA link when available
- Concepts
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Physics, Tracing, Astrobiology, Atmosphere (unit), Astronomy, Jupiter (rocket family), Hot Jupiter, Astrophysics, Planet, Exoplanet, Meteorology, Operating system, Space Shuttle, Computer scienceTop concepts (fields/topics) attached by OpenAlex
- Cited by
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1Total citation count in OpenAlex
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2025: 1Per-year citation counts (last 5 years)
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146Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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