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The GAPS Programme at TNG XXXIX. Multiple molecular species in the atmosphere of the warm Giant Planet WASP-80 b unveiled at high resolution with GIANO-B*

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Carleo, Ilaria, Giacobbe, Paolo, Guilluy, Gloria, Cubillos, Patricio E., Bonomo, Aldo S., Sozzetti, Alessandro, Brogi, Matteo, Gandhi, Siddharth, Fossati, Luca, Turrini, Diego et al.
(2022) The GAPS Programme at TNG XXXIX. Multiple molecular species in the atmosphere of the warm Giant Planet WASP-80 b unveiled at high resolution with GIANO-B*. The Astronomical Journal, 164 (3). 101. doi:10.3847/1538-3881/ac80bf ISSN 1538-3881.

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Official URL: https://doi.org/10.3847/1538-3881/ac80bf

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Abstract

Detections of molecules in the atmosphere of gas giant exoplanets allow us to investigate the physico-chemical properties of the atmospheres. Their inferred chemical composition is used as tracer of planet formation and evolution mechanisms. Currently, an increasing number of detections is showing a possible rich chemistry of the hotter gaseous planets, but whether this extends to cooler giants is still unknown. We observed four transits of WASP-80 b, a warm transiting giant planet orbiting a late-K dwarf star with the near-infrared GIANO-B spectrograph installed at the Telescopio Nazionale Galileo and performed high-resolution transmission spectroscopy analysis. We report the detection of several molecular species in its atmosphere. Combining the four nights and comparing our transmission spectrum to planetary atmosphere models containing the signature of individual molecules within the cross-correlation framework, we find the presence of H2O, CH4, NH3, and HCN with high significance, tentative detection of CO2, and inconclusive results for C2H2 and CO. A qualitative interpretation of these results, using physically motivated models, suggests an atmosphere consistent with solar composition and the presence of disequilibrium chemistry and we therefore recommend the inclusion of the latter in future modeling of sub-1000 K planets.

Item Type: Journal Article
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Faculty of Science, Engineering and Medicine > Science > Physics
SWORD Depositor: Library Publications Router
Library of Congress Subject Headings (LCSH): Extrasolar planets , Extrasolar planets -- Atmopsheres, Extrasolar planets -- Detection, Astronomical photometry , Molecular spectroscopy
Journal or Publication Title: The Astronomical Journal
Publisher: The American Astronomical Society
ISSN: 1538-3881
Official Date: 18 August 2022
Dates:
DateEvent
18 August 2022Published
11 July 2022Accepted
Volume: 164
Number: 3
Article Number: 101
DOI: 10.3847/1538-3881/ac80bf
Status: Peer Reviewed
Publication Status: Published
Reuse Statement (publisher, data, author rights): ** From IOP Publishing via Jisc Publications Router ** History: received 03-05-2022; rev-recd 25-06-2022; accepted 11-07-2022; oa-requested 11-07-2022; epub 18-08-2022; open-access 18-08-2022; ppub 01-09-2022. ** Licence for this article: http://creativecommons.org/licenses/by/4.0/
Access rights to Published version: Open Access (Creative Commons)
Date of first compliant deposit: 11 October 2022
Date of first compliant Open Access: 11 October 2022
RIOXX Funder/Project Grant:
Project/Grant IDRIOXX Funder NameFunder ID
PRIN INAF 2019European Commissionhttp://dx.doi.org/10.13039/501100000780
2018-16-HHAgenzia Spaziale Italianahttp://dx.doi.org/10.13039/501100003981
J4595-NAustrian Science Fundhttp://dx.doi.org/10.13039/501100002428
ST/T000406/1[STFC] Science and Technology Facilities Councilhttp://dx.doi.org/10.13039/501100000271
CUP: C54I19000700005)INAF - Osservatorio Astrofisico di Cataniahttp://dx.doi.org/10.13039/501100006486
2021-5-HH.0Agenzia Spaziale Italianahttp://dx.doi.org/10.13039/501100003981
2021-5-HH.0INAF - Osservatorio Astrofisico di Cataniahttp://dx.doi.org/10.13039/501100006486
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