| Issue |
A&A
Volume 701, September 2025
|
|
|---|---|---|
| Article Number | A276 | |
| Number of page(s) | 21 | |
| Section | Planets, planetary systems, and small bodies | |
| DOI | https://doi.org/10.1051/0004-6361/202553724 | |
| Published online | 25 September 2025 | |
Quantifying thermal water dissociation in the dayside photosphere of WASP-121 b using NIRPS
1
Institut Trottier de recherche sur les exoplanètes, Département de Physique, Université de Montréal, Montréal,
Québec,
Canada
2
Department of Earth, Planetary, and Space Sciences, University of California,
Los Angeles,
CA
90095,
USA
3
Observatoire de Genève, Département d’Astronomie, Université de Genève,
Chemin Pegasi 51,
1290
Versoix,
Switzerland
4
Univ. Grenoble Alpes, CNRS, IPAG,
38000
Grenoble,
France
5
European Southern Observatory (ESO),
Karl-Schwarzschild-Str. 2,
85748
Garching bei München,
Germany
6
University Observatory, Faculty of Physics, Ludwig-Maximilians-Universität München,
Scheinerstr. 1,
81679
Munich,
Germany
7
Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas,
4150-762
Porto,
Portugal
8
Observatoire du Mont-Mégantic,
Québec,
Canada
9
Departamento de Física e Astronomia, Faculdade de Ciências, Universidade do Porto, Rua do Campo Alegre,
4169-007
Porto,
Portugal
10
Department of Physics, University of Toronto,
Toronto,
ON
M5S 3H4,
Canada
11
Departamento de Física Teórica e Experimental, Universidade Federal do Rio Grande do Norte, Campus Universitário,
Natal,
RN
59072-970,
Brazil
12
Department of Physics & Astronomy, McMaster University,
1280 Main St W,
Hamilton,
ON,
L8S 4L8,
Canada
13
Department of Physics, McGill University,
3600 rue University,
Montréal,
QC
H3A 2T8,
Canada
14
Department of Earth & Planetary Sciences, McGill University,
3450 rue University,
Montréal,
QC,
H3A 0E8,
Canada
15
Departamento de Física, Universidade Federal do Ceará,
Caixa Postal 6030, Campus do Pici,
Fortaleza,
Brazil
16
Centre Vie dans l’Univers, Faculté des sciences de l’Université de Genève,
Quai Ernest-Ansermet 30,
1205
Geneva,
Switzerland
17
Instituto de Astrofísica de Canarias (IAC), Calle Vía Láctea s/n,
38205
La Laguna, Tenerife,
Spain
18
Departamento de Astrofísica, Universidad de La Laguna (ULL),
38206
La Laguna, Tenerife,
Spain
19
Space Research and Planetary Sciences, Physics Institute, University of Bern,
Gesellschaftsstrasse 6,
3012
Bern,
Switzerland
20
Consejo Superior de Investigaciones Científicas (CSIC),
28006
Madrid,
Spain
21
Bishop’s Univeristy, Dept of Physics and Astronomy,
Johnson-104E, 2600 College Street,
Sherbrooke,
QC
J1M 1Z7,
Canada
22
Department of Physics, Engineering Physics, and Astronomy, Queen’s University,
99 University Avenue,
Kingston,
ON
K7L 3N6,
Canada
23
Department of Physics and Space Science, Royal Military College of Canada,
13 General Crerar Cres.,
Kingston,
ON
K7P 2M3,
Canada
24
Instituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências da Universidade de Lisboa, Campo Grande,
1749-016
Lisboa,
Portugal
25
Departamento de Física da Faculdade de Ciências da Universidade de Lisboa,
Edifício C8,
1749-016
Lisboa,
Portugal
26
Centre of Optics, Photonics and Lasers, Université Laval,
Québec,
Canada
27
Herzberg Astronomy and Astrophysics Research Centre, National Research Council of Canada,
Canada
28
Center for Space and Habitability, University of Bern,
Gesellschaftsstrasse 6,
3012
Bern,
Switzerland
29
Aix Marseille Univ, CNRS, CNES, LAM,
Marseille,
France
30
European Southern Observatory (ESO),
Av. Alonso de Cordova 3107, Casilla
19001,
Santiago de Chile,
Chile
31
Planétarium de Montréal, Espace pour la Vie,
4801 av. Pierre-de Coubertin, Montréal,
Québec,
Canada
32
Lund Observatory, Division of Astrophysics, Department of Physics, Lund University,
Box 118,
221 00
Lund,
Sweden
33
York University,
4700 Keele St,
North York,
ON
M3J 1P3,
Canada
34
University of British Columbia,
2329 West Mall,
Vancouver,
BC
V6T 1Z4,
Canada
35
Western University, Department of Physics & Astronomy and Institute for Earth and Space Exploration,
1151 Richmond Street,
London,
ON
N6A 3K7,
Canada
36
Light Bridges S.L., Observatorio del Teide, Carretera del Observatorio, s/n Guimar,
38500,
Tenerife, Canarias,
Spain
37
Department of Astronomy & Astrophysics, University of Chicago,
5640 South Ellis Avenue,
Chicago,
IL
60637,
USA
38
Laboratoire Lagrange, Observatoire de la Côte d’Azur, CNRS, Université Côte d’Azur,
Nice,
France
★ Corresponding author: luc.bazinet@umontreal.ca
Received:
10
January
2025
Accepted:
4
August
2025
The intense stellar irradiation of ultra-hot Jupiters results in some of the most extreme atmospheric environments in the planetary regime. On their daysides, temperatures can be sufficiently high for key atmospheric constituents to thermally dissociate into simpler molecular species and atoms. This dissociation drastically changes the atmospheric opacities and, in turn, critically alters the temperature structure, atmospheric dynamics, and day-night heat transport. To date, however, simultaneous detections of the dissociating species and their thermally dissociation products in exoplanet atmospheres have remained rare. In this work we present the simultaneous detections of H2O and its thermally dissociation product OH on the dayside of the ultra-hot Jupiter WASP-121 b based on high-resolution emission spectroscopy with the recently commissioned Near InfraRed Planet Searcher (NIRPS). We retrieved a photospheric abundance ratio of log10(OH/H2O) = −0.15 ± 0.20, indicating that there is about as much OH as H2O at photospheric pressures, which confirms predictions from chemical equilibrium models. We compared the dissociation on WASP-121 b with other ultra-hot Jupiters and show that a trend in agreement with equilibrium models arises. We also discuss an apparent velocity shift of 4.79−0.97+0.93 km s−1 in the H2O signal, which is not reproduced by current global circulation models. Finally, in addition to H2O and OH, the NIRPS data reveal evidence of Fe and Mg, from which we inferred a Fe/Mg ratio consistent with the solar and host star ratios. Our results demonstrate that NIRPS can be an excellent instrument to obtain simultaneous measurements of refractory and volatile molecular species, thus paving the way for many future studies on the atmospheric composition, chemistry, and the formation history of close-in exoplanets.
Key words: atmospheric effects / instrumentation: spectrographs / techniques: spectroscopic / planets and satellites: atmospheres / planets and satellites: gaseous planets
© The Authors 2025
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
This article is published in open access under the Subscribe to Open model. Subscribe to A&A to support open access publication.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.